Geometry of Nonlinear Supersymmetry in Curved Spacetime and Unity of Nature

Μέγεθος: px
Εμφάνιση ξεκινά από τη σελίδα:

Download "Geometry of Nonlinear Supersymmetry in Curved Spacetime and Unity of Nature"

Transcript

1 Proceedings of Institute of Mathematics of NAS of Ukraine 00, Vol. 43, Part, Geometry of Nonlinear Supersymmetry in Curved Spacetime and Unity of Nature Kazunari SHIMA Laboratory of Physics, Saitama Institute of Technology, Okabe-machi, Saitama , Japan A new Einstein Hilbert type action of superon-graviton model SGM for space-time and matter is obtained based upon the geometrical arguments of the higher symmetric SGM space-time. SGM action is invariant under [global NL SUSY] [local GL4, R] [local Lorentz] [global SON]. The explicit form of SGM action is given in terms of the fields of the graviton and superons by using the affine connection formalism. Some characteristic structures of the gravitational coupling of superons are manifested in two dimensional space-time with some details of the calculations. SGM cosmology is discussed briefly. 1 Introduction To explore the new physics and the new framework for the unification of space-time and matter beyond the standard mode SM, new gauge symmetries and new particles yet to be observed are introduced in the model building. Supersymmetry [1, ] may be the most promising notion beyond SM, especially for the unification of space-time and matter. In the previous paper [3] we have introduced a new fundamental constituent with spin 1/ superon and proposed superon-graviton model SGM as a model for unity of space-time and matter. In SGM, the fundamental entities of nature are the graviton with spin- and a quintet of superons with spin-1/. They are the elementary gauge fields corresponding to the local GL4, R and the global nonlinear supersymmetry NL SUSY with a global SO10, respectively. All observed elementary particles including gravity are assigned to a single massless irreducible representation of SO10 super-poincaré SP symmetry and reveal a remarkable potential for the phenomenology, e.g. the three-generations structure of quarks and leptons, stability of proton, mixings, etc. [3]. And except graviton they are supposed to be the massless composite-eigenstates of superons of SO10 SP symmetry [4] of space-time and matter. The uniqueness of N = 10 among all SON SP is pointed out. The arguments are group theoretical so far. In order to obtain the fundamental action of SGM which is invariant at least under local GL4, R, local Lorentz, global NL SUSY transformations and global SO10, we have performed the similar arguments to Einstein general relativity theory EGRT in the SGM space-time, where the tangent Riemann-flat Minkowski space-time is specified by the coset space SL, C coordinates corresponding to Nambu Goldstone N G fermion of NL SUSY of Volkov Akulov V A [] in addition to the ordinary Lorentz SO3, 1 coordinates [3], which are locally homomorphic groups. As shown in Ref. [5] the SGM action obtained by the geometrical arguments of SGM space-time is naturally the analogue of Einstein Hilbert E H action of GR and has the similar concise expression. The similar systematic arguments are applicable to spin 3/ N G case [6]. In this article, after a brief review of SGM for the self contained arguments we expand SGM action in terms of the fields of graviton and superons in order to see some characteristic structures of our model and to show some details of the calculations. For the sake of simplicity the expansion is performed by the affine connection formalism.

2 Geometry of Nonlinear Supersymmetry 531 Finally some hidden symmetries and a potential cosmology, especially the birth of the universe are mentioned briefly. Fundamental action of superon-graviton model SGM SGM space-time is defined as the space-time whose tangentflat space-time is specified by SO1, 3 Lorentz coordinates x a and the coset space SL, C coordinates ψ of NL SUSY of Volkov Akulov V A []. The unified vierbein w a µ and the unified metric s µν x w a µ xw aν x of SGM space-time are defined by generalizing the NL SUSY invariant differential forms of V A to the curved space-time [5]. SGM action is given as follows [5] c3 L SGM = w Ω + Λ, 1 16πG w =detw a µ =dete a µ + t a µ, t a µ = κ i 10 j=1 ψ j γ a µ ψ j µ ψj γ a ψ j, where κ is an arbitrary constant of V A up now with the dimension of the fourth power of length, e a µ and ψ j j =1,,...,10 are the fundamental elementary fields of SGM, i.e. the vierbein of EGRT and the superons of N G fermion of NL SUSY of Volkov Akulov [], respectively. Λ is a cosmological constant which is necessary for SGM action to reduce to V A model with the first order derivative terms of the superon in the Riemann-flat space-time. Ω is a unified scalar curvature of SGM space-time analogous to the Ricci scalar curvature R of EGRT. SGM action 1 is invariant under the following new SUSY transformations δψ i x =ζ i + iκ ζ j γ ρ ψ j x ρ ψ i x, 3 δe a µx =iκ ζ j γ ρ ψ j xd [ρ e a µ]x, 4 where ζ i,i =1,...,10 is a constant spinor, D [ρ e a µ]x =D ρ e a µ D µ e a ρ and D µ is a covariant derivative containing a symmetric affine connection. The explicit expression of Ω is obtained by just replacing e µ a x inricciscalarr of EGRT by the vierbein w µ a x =e µ a + t µ a of the SGM curved space-time, which gives the gravitational interaction of ψx invariant under 3 and 4. The overall factor of our model is fixed to c3 16πG, which reproduces E H action of GR in the absence of superonsmatter. Also in the Riemann-flat space-time, i.e. e µ a x δ µ a, it reproduces V A action of NL SUSY[] with κ 1 V A = c3 16πGΛ in the first order derivative terms of the superon. Therefore our model SGM predicts a small non-zero cosmological constant, provided κ V A O1, and posesses two mass scales. Furthermore it fixes the coupling 1 constant of superon N G fermion with the vacuum to c 3 16πG Λ from the low energy theorem viewpoint, which may be relevant to the birth of the universe. It is interesting that our action is the vacuum matter free action in SGM space-time as read off from 1 but gives in ordinary Riemann space-time the E H action with matter superons accompanying the spontaneous supersymmetry breaking. The commutators of new SUSY transformations induce the generalized general coordinate transformations [δ ζ1,δ ζ ]ψ =Ξ µ µ ψ, 5 [δ ζ1,δ ζ ]e a µ =Ξ ρ ρ e a µ + e a ρ µ Ξ ρ, 6 where Ξ µ is defined by Ξ µ =ia ζ γ µ ζ 1 ξ ρ 1 ξσ e a µ D [ρ e a σ]. 7

3 53 K. Shima We have shown that our action is invariant at least under [7] [global NL SUSY] [local GL4, R] [local Lorentz] [global SON], 8 which is isomorphic to N = 10 extended global SO10 SP symmetry through which SGM reveals the spectrum of all observed particles in the low energy [4]. In contrast with the ordinary SP SUSY, SGM SUSY may be regarded as a square root of a generalized GL4, R. The usual local GL4, R invariance is obvious by the construction. The simple expression 1 invariant under the above symmetry may be universal for the gravitational coupling of Nambu Goldstone N G fermion, for by performing the parallel arguments we obtain the same expression for the gravitational interaction of the spin-3/ N G fermion [6]. Now to clarify the characteristic features of SGM we focus on N = 1 SGM for simplicity without loss of generality and write down the action explicitly in terms of t a µ or ψ andg µν or e a µ. We will see that the graviton and superons matter are complementary in SGM and contribute equally to the curvature of SGM space-time. Contrary to its simple expression 1, it has rather complicated and rich structures. We use the Minkowski tangent space metric 1 γa,γ b = η ab = +,,, andσ ab = i 4 [γa,γ b ]. Latin a,b,... and Greek µ,ν,... are the indices for local Lorentz and general coordinates, respectively. By requiring that the unified action of SGM space-time should reduce to V A in the flat space-time which is specified by x a and ψx and that the graviton and superons contribute equally to the unified curvature of SGM space-time, it is natural to consider that the unified vierbein w a µx and the unified metric s µν x of unified SGM space-time are defined through the NL SUSY invariant differential forms ω a of V A [] as follows: ω a = w a µdx µ, 9 w a µx =e a µx+t a µx, 10 where e a µx is the vierbein of EGRT and t a µx isdefinedby t a µx =iκ ψγ a µ ψ, 11 where the first and the second indices of t a µ represent those of the γ matrices and the general covariant derivatives, respectively. We can easily obtain the inverse w a µ of the vierbein w a µ in the power series of t a µ as follows, which terminates with t 4 for 4 dimensional space-time: w a µ = e a µ t µ a + t ρ at µ ρ t ρ at σ ρt µ σ + t ρ at σ ρt κ σt µ κ. 1 Similarly a new metric tensor s µν x and its inverse s µν x are introduced in SGM curved space-time as follows: s µν x w a µxw aν x =w a µxη ab w b νx =g µν + t µν + t νµ + t ρ µt ρν, 13 s µν x w µ a xw aν x =g µν t µν t νµ + t ρµ t ν ρ + t ρν t µ ρ + t µρ t ν ρ t ρµ t σ ρt ν σ We can easily show t ρν t σ ρt µ ρ t µσ t ρ σt ν ρ t νρ t σ ρt µ σ + t ρµ t σ ρt κ σt ν κ + t ρν t σ ρt κ σt µ κ + t µσ t ρ σt σ ρt ν σ + t νσ t ρ σt σ ρt µ σ + t ρκ t σ κt µ ρt ν σ. 14 w a µ w bµ = η ab, s µν w a µ w b ν = η ab. 15 Furthermore they have generalized GL4, R transformations under 3 and 4 [5, 7]. It is obvious from the above general covariant arguments that 1 is invariant under the ordinaly GL4, R and under 3 and 4.

4 Geometry of Nonlinear Supersymmetry 533 By using 10, 1, 13 and 14 we can express SGM action 1 in terms of e a µxandψ j x, which describes explicitly the fundamental interaction of graviton with superons. The expansion of the action in terms of the power series of κ or t a µ can be carried out straightforwardly. After the lengthy calculations concerning the complicated structures of the indices we obtain [ L SGM = c3 Λ 16πG e w V-A c3 16πG er + c3 16πG e t µν R µν g µν ρ t µσ σ g ρν g µν ρ t µν σ g ρσ g µν g ρσ κ t ρσ κ g µν +t µ ρt ρν + t ν ρt ρµ + t µρ t ν ρ R βµ + 1 tµν g ρσ µ ν t ρσ g ρσ ρ µ t σν + g µν ρ ρ t µν t µν ρ ρ g µν t µρ t ν ρr µν + t µρ t νσ R µνρσ + O t 3 + O t O t 10 ], 16 where e =dete a µ, t µν = t µν + t νµ, t µν = t µν + t νµ,and w V A =detw a b is the flat space V A action [] containing up to O t 4 and R and R µν are the Ricci curvature tensors of GR. Remarkably the first term can be regarded as a space-time dependent cosmological term and reduces to V A action [] with κ 1 V A = c3 16πG Λ in the Riemann-flat e a µ x δ µ a space-time. The second term is the familiar E H action of GR. These expansions show the complementary relation of graviton and the stress-energy tensor of superons. The existence of in the Riemannflat space-time NL SUSY invariant terms with the second order derivatives of the superons beyond V A model is manifested. For example, such terms of the lowest order appear in O t and have the following expressions up to the total derivative terms +ɛ abcd ɛ a efg c t be f t dg. 17 Existence of such derivative terms in addition to the original V A model are already pointed out and exemplified in part in [8]. Note that 17 vanishes in dimensional space-time. Here we just mention that we can consider two types of the flat space in SGM, which are not equivalent. One is SGM-flat, i.e. w µ a x δ µ a, space-time and the other is Riemann-flat, i.e. e µ a x δ µ a, space-time, where SGM action reduces to c3 Λ 16πG and c3 Λ 16πG w V A c3 16πG derivative terms, respectively. Note that SGM-flat space-time may allow Riemann spacetime, e.g. t µ a x e µ a + δ µ a realizes Riemann space-time and SGM-flat space-time. The cosmological implications are mentioned in the discussions. 3 SGM in two dimensional space-time Now we go to two dimensional SGM space-time to simplify the arguments without loss of generality and demonstrate some details of the computations. It is well known that two dimensional GR has no physical degrees of freedom due to the local GL, R. SGM in SGM space-time is also the case. However the general covariant arguments shed light on the universal characteristic features of the theory in any space-time dimensions. Especialy for SGM, it is also useful to see explicitly the superon-graviton coupling in two dimensional Riemann space-time which is realized spontaneously from SGM space-time. We adopt the affine connection formalism. Knowledge of the complete structure of SGM action including the surface terms is useful to linearize SGM into the equivalent linear theory and to find the symmetry breaking of the model. Following EGRT the scalar curvature tensor Ω of SGM space-time is given as follows [ ] Ω=s βµ Ω α βµα = s βµ µ Γ λ βα +Γ α λµγ λ βα lower indices µ α, 18

5 534 K. Shima where the Christoffel symbol of the second kind of SGM space-time is Γ α βµ = 1 sαρ β s ρµ + µ s βρ ρ s µβ. 19 The straightforward expression of SGM action 1 in two dimensional space-time which is 3 6 times more complicated than the dimensional GR is given as follows c3 L dsgm = 16πG e [ 1 µ t a a + 1 t a at b b t a bt b a g βµ t βµ + t βµ g ασ t ασ + t ασ β g σ α + t σ α + t σ α g ασ t ασ + t ασ µ β g σ α + t σ α + t σ α lower indices µ α 1 g ασ t ασ + t ασ 4 λ g σ µ + t σ µ + t σ µ g λρ t λρ + t λρ β g ρ α + t ρ α + t ρ α lower indices µ α c3 Λ 16πG e w V A, 0 where we have put s αβ = g αβ + t αβ + t αβ, s αβ = g αβ t αβ + t αβ, t µν = t µν + t νµ, t µν = t ρ µt ρν, t µν = t µν + t νµ, t µν = t µ ρt ρν + t ν ρt ρµ + t µρ t ν ρ, 1 and the Christoffel symbols of the first kind of SGM space-time contained in 19 are abbreviated as µ g σ ν = µ g σν + ν g µσ σ g νµ, µ t σ ν = µ t σν + ν t µσ σ t νµ, µ t σ ν = µ t σν + ν t µσ σ t νµ. By expanding the scalar curvature Ω in the power series of t which terminates with t 4,wehave the following complete expression of two dimensional SGM, [ L dsgm = c3 Λ 16πG e w V A c3 16πG e w V A R t µν R µν + 1 g µν ρ ρ t µν t µν ρ ρ g µν + g µν ρ t µσ σ g ρν g µν ρ t µν σ g ρσ g µν g ρσ κ t ρσ κ g µν ] + t βµ R βµ + t βµ t ασ R µασβ 1 t βµ g ασ µ β t ασ σ β t σµ + µ t ασ β g σα µ g ασ β t σα + α g ασ β t σµ α t ασ β g σµ + ρ t σµ σ g βρ g ασ λ t σµ λ g αβ + g ασ g λρ µ t λσ β g ρα g ασ ρ t σα β g ρµ + g ασ λ t σα λ g µβ g βµ µ g ασ β t σα + t ασ β g σα t ασ β t σα

6 Geometry of Nonlinear Supersymmetry 535 t ασ β t σµ σ t µβ + g βµ α g ασ β t σµ σ t µβ + t ασ β g σµ σ g µβ + α g λµ g βλ µ t αβ α t βρg µρ + t λρ λ g σµ g βµ σ g βρ ρ g αβ t λρ λ g σµ g ασ µ t ρα ρ t αβ g βµ + ρ t σµ g βµ σ t βρ ρ t αβ g ασ + t ασ t λρ β g λσ β g ρα + λ g σµ g µβ α g βρ ρ g αβ t λρ λ t σµ g βµ σ g βρ ρ g αβ g ασ ρ g σα g σα µ t ρµ ρ t µβg βµ ρ t σα µ g ρµ g σα λ g µβ g µβ t λρ λ g σα g σα µ g ρµ ρ g µβ g µβ t ασ ρ g σα µ g ρµ ρ g µβ g µβ t λρ λ g σα g ασ µ t ρµ ρ t µβ g βµ t ασ ρ t σα µ g ρµ ρ g µβ g βµ + g ασ ρ t σα µ t ρµ ρ t µβ g βµ + t ασ t λρ λ g σα g ασ µ g ρµ ρ g µβ g βµ t λρ λ t σα g ασ µ g ρµ ρ g µβ g βµ t ασ ρ g σα µ t ρµ ρ t µβ g βµ + 1 t βµ g ασ µ β t ασ σ β t σµ + µ t ασ β g σα µ g ασ β t σα + α g ασ β t σµ α t ασ β g σµ + ρ t σµ σ g βρ g ασ λ t σµ λ g αβ + g ασ g λρ µ t λσ β g ρα g ασ ρ t σα β g ρµ + g ασ λ t σα λ g µβ 1 t βµ µ g ασ β t σα t ασ β t σα + µ t ασ β g σα + α g ασ β t σµ σ t µβ t ασ β t σµ σ t µβ + α t ασ β g σµ σ g µβ + α g λµ g βλ µ t αβ α t βρg µρ + t λρ λ g σµ g βµ σ g βρ ρ g αβ t λρ λ g σµ g ασ µ t ρα ρ t αβ g βµ + ρ t σµ g βµ σ t βρ ρ t αβ g ασ + t ασ t λρ β g λσ β g ρα + λ g σµ g µβ α g βρ ρ g αβ t λρ λ t σµ g βµ σ g βρ ρ g αβ g ασ ρ g σα g σα µ t ρµ ρ t µβg βµ ρ t σα µ g ρµ g σα λ g µβ g µβ t λρ λ g σα g σα µ g ρµ ρ g µβ g µβ t ασ ρ g σα µ g ρµ ρ g µβ g µβ t λρ λ g σα g ασ µ t ρµ ρ t µβ g βµ t ασ ρ t σα µ g ρµ ρ g µβ g βµ + g ασ ρ t σα µ t ρµ ρ t µβ g βµ + t ασ t λρ λ g σα g ασ µ g ρµ ρ g µβ g βµ t λρ λ t σα g ασ µ g ρµ ρ g µβ g βµ t ασ ρ g σα µ t ρµ ρ t µβ g βµ + β t ασ β t σα t ασ β t σα g βµ α t ασ β t σµ σ t µβ t ασ β t σµ β t µβ + 1 g ασ λ g σµ + µ g λσ σ g µλ t λρ g βµ β t ρα + α t βρ ρ t αβ + g ασ λ t σµ + µ g λσ σ t µλ t λρ t λρ g βµ β g ρα + α g βρ ρ g αβ g ασ λ g σµ + µ g λσ σ g µλ t λρ g βµ β t ρα + α t βρ ρ t αβ g ασ λ t σµ + µ t λσ σ t µλ t λρ g βµ β g ρα + α g βρ ρ g αβ

7 536 K. Shima + t ασ λ g σµ + µ g λσ σ g µλ t λρ g βµ β t ρα + α t βρ ρ t αβ g ασ λ t σµ + µ g λσ σ t µλ t λρ g βµ β t ρα + α t βρ ρ t αβ t ασ λ t σµ + µ g λσ σ t µλ g λρ g βµ β t ρα + α t βρ ρ t αβ g ασ λ g σα t λρ g βµ β t ρµ ρ t µβ + g ασ λ t σα t λρ β g ρµ ρ g µβ + g ασ λ g σα t λρ g βµ β t ρµ ρ t µβ + g ασ λ t σµ t λρ g βµ β g ρµ ρ g µβ t ασ λ g σα t λρ g βµ β t ρµ ρ t µβ + g ασ λ t σα t λρ g βµ β t ρµ ρ t µβ + t ασ λ t σα + α g λσ σ t αλ g λρ g βµ β t ρµ + µ t βρ ρ t µβ t βµ 1 µ t ασ β t σα µ t ασ βt σα + t ασ µ β t σα α t ασ β t σµ σ t µβ + α t ασ β t σµ σ t µβ t ασ α β t σµ σ t µβ + 1 g ασ λ t 4 σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ g ασ λ t σµ + µ g λσ σ t µλ t λρ β t ρα + α t βρ ρ t αβ + g ασ λ t σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ t ασ λ t σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ g ασ λ t σα g λρ β t ρµ ρ t µβ + g ασ λ t σα t λρ β t ρµ ρ t µβ g ασ λ t σαg λρ β t ρµ ρ t µβ + t ασ λ t σα g λρ β t ρµ ρ t µβ + g βµ 1 µ t ασ β t σα + t ασ µ β t σα α t ασ β t σµ σ t µβ t ασ α β t σµ σ t µβ + 1 g ασ λ t σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ 4 g ασ λ t σµ + µ t λσ σ t µλ t λρ β t ρα + α t βρ ρ t αβ + g ασ λ t σµ + µ t λσ σ t µλ t λρ β t ρα + α t βρ ρ t αβ g ασ λ t σµ + µ t λσ σ t µλ t λρ β t ρα + α t βρ ρ t αβ t ασ λ t σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ + t ασ λ t σµ + µ t λσ σ t µλ t λρ β t ρα + α t βρ ρ t αβ + t ασ λ t σµ + µ t λσ σ t µλ g λρ β t ρα + α t βρ ρ t αβ g ασ λ t σµg λρ β t ρµ ρ t µβ + g ασ λ t σα t λρ β t ρµ ρ t µβ g ασ λ t σα t λρ β t ρµ ρ t µβ + g ασ λ t σµ t λρ β t ρµ ρ t µβ + t ασ λ t σα g λρ β t ρµ ρ t µβ t ασ λ t σα t λρ β t ρµ ρ t µβ t ασ λ t σα g λρ β t ρµ ρ t µβ ], 3

8 Geometry of Nonlinear Supersymmetry 537 where R µνρσ, R µν and R are the curvature tensors of Riemann space and w V A = 1+t a a + 1 ta at b b t a bt b a is V A model in two dimensional flat space. 4 Discussions We have shown that contrary to its simple expression 1 in unified SGM space-time the complete expansion of SGM action posesses the very complicated and rich structures describing the graviton-superon interactions in Riemann space-time, even in two dimensional space-time. The SGM in four dimensional space-time has far much more complicated structures, which may be unavoidable features for a unified theory to describe the rationale of beings of all elementary particles. Note that the total number of elementary particles in SGM is at most a few hundreds and most of them are heavy massive. Here we just emphasize that SGM action in SGM space-time is a nontrivial generalization of E H action in Riemann space-time despite the liner relation w a µ = e a µ + t a µ. In fact, by the redefinitionsvariations e a µ e a µ + δe a µ = e a µ t a µ and δe µ a = e ν a e µ b δe b ν =+t µ a the inverse w µ a = e µ a t µ a+t ρ at µ ρ t ρ at σ ρt µ σ+t ρ at σ ρt κ σt µ κ does not reduce to e µ a, i.e. the nonlinear terms in t µ a in the inverse w µ a can not be eliminated. Because t a µ is not a vierbein. Such a redefinition breaks the metric properties of w a µ and w µ a. Note that SGM action posesses two inequivalent flat spaces, i.e. SGM-flat w a µ δ a µ and Riemann-flat e a µ δ a µ. The expansion of SGM action in terms of e a µ and t a µ is a spontaneous breakdown of space-time from SGM space-time to Riemann space-time connecting with Riemann-flat space-time. Concerning the above-mentioned two inequivalent flat-spaces i.e. the vacuum of the gravitational energy of SGM action we can interprete them as follows. SGM action 1 written by the vierbein w µ a x and metric s µν x of SGM space-time is invariant under besides the ordinary local GL4, R the general coordinate transformation [7] with a generalized parameter iκ ζγ µ ψx originating from the global supertranslation in SGM space-time []. As proved for E H action of GR the positive definitness of Einstein Hilbert actionwas proved by E. Witten [10], the energy of SGM action of E H type is expected to be positive for positive Λ. Regarding the scalar curvature tensor Ω for the unified metric tensor s µν x asananalogueof the Higgs potential for the Higgs scalar, we can observe that at least the vacuum of SGM action i.e. SGM-flat w a µx δ a ν space-time, which allows Riemann space-time and has a positive energy density with the positive cosmological constant c3 Λ 16πG indicating the spontaneous SUSY breaking, is unstable i.e. degenerates against the supertransformation 3 and 4 with the global spinor parameter ζ in SGM space-time and breaks down spontaneously to Riemann space-time w a µx =e a µx+t a super GL4,R µx withn Gfermionssuperons corresponding to GL4,R. Note that SGM-flat space-time allows Riemann space-time. Remarkably the observed Riemann space-time of EGRT and mattersuperons appear simultaneously from the vacuum of SGM action by the spontaneous SUSY breaking. The investigation of the structures of the vacuum of Riemann-flat space-time described by N = 10 V A action with derivative terms like 17 plays an important role to linearize SGM and to derive SM as the low energy effective theory of SGM, which remain to be challenged. Such higher derivative terms can be rewritten in the tractable forms similar to 17 up to the total derivative terms. As for the linearization, the linearization of the flat-space N = 1 V A model was already carried out [9]. They proved that the linear SUSY action of a scalar supermultiplet with SUSY breaking is equivalent to V A action under SUSY invariant constraints obtained by the systematic arguments. Recently we have shown explicitly that the action of U1 vector supermultiplet with Feyet Iliopoulos term is equivalent to N = 1 V A model [11]. It is remarkable that the renormalizable low energy effective U1 gauge theory is derived from the highly nonlinear theo-

9 538 K. Shima ry by systematic arguments. While, in the linearization of SGM i.e. V A model in curved space-time it should be taken into consideration further that the algebra gauge symmetry would be changed from 8 to broken SO10 SP symmetry. From the physical point of view the linearization of the flat-space N = V Amodelis very important as a toy model, for it may be equivalent to the following Higgs Kibble Dirac Lagrangian composed of N = SP off-shell multiplet L HKD = 1 4 F µν + ψγ µ D µ ψ + 1 µφ i +gφ i ψψ gdφi + 1 D + F, 4 where F µν is a gauge field, ψ is a Dirac field, φ i i =1, is a real scalar field and the fields D, and F are auxiliary fields. This, speculative so far, is remarkable, for the U1 gauge field including the gauge coupling constant is expressed in terms of the superons and the the fundamental coupling constant of V A model including the order parameter of the symmetry breaking. A nonlinear N = SUSY equivalent to N = SUSY Yang Mills theory investigated by Seiberg and Witten [1] may be a realistic case. Furthermore the baryon abundance of the universe should be explained by the spontaneous symmetry breaking of the linearized low energy effective theory. Finally we just mention the hidden symmetries characteristic to SGM. It is natural to expect that SGM action may be invariant under a certain exchange between e a µ and t a µ, for they contribute equally to the unified SGM vierbein w a µ as seen in 10. In fact we find, as a simple example, that SGM action is invariant under the following exchange of e a µ and t a µ [13] in 4 dimensional space-time. e a µ t a µ, t a µ e a µ t a µ, e a µ e a µ. 5 The physical meaning of such symmetries remains to be studied. Also SGM action has Z symmetry ψ j ψ j but not e a µ e a µ. Beside the composite picture of SGM it is interesting to consider elementary field SGM with the extra dimensions and their compactifications. The compactification of w A M = e A M + t A M, A, M = 0, 1..., D 1 produces rich spectrum of particles and hidden internal symmetries and may give a new framework for the unification of space-time and matter. Acknowledgements The author is grateful to Motomu Tsuda for collaborating on this work. Also he would like to express sincere gratitude to the organizers for the patient help in processing the final version of the manuscript. The work is supported in part by High-Tech Research Program of Saitama Institute of Technology. [1] Wess J. and Zumino B., Supergauge transformation, Phys. Lett. B, 1974, V.49, 5 56 SUSY was found independently from the different motivations; Golfand Yu.A. and Likhtman E.P., Extension of the algebra of Poincaré group generators and violation of p invariance, JETP. Lett., 1971, V.13, [] Volkov D.V. and Akulov V.P., Is neutrino a Goldstone particle?, Phys. Lett. B, 1973, V.46, [3] Shima K., Superon-quintet and graviton model for supersymmetric spacetime and matter, European Phys. J. C, 1999, V.7, [4] Shima K., SON supergravity and unification of all fundamental forces, Z. Phys. C, 1983, V.18, 5 9. [5] Shima K., Supersymmetric structure of spacetime and matter: superon-graviton model, Phys. Lett. B, 001, V.501, [6] Shima K. and Tsuda M., On gravitational interaction of spin 3/ Nambu Goldstone fermion, Phys. Lett. B, 001, V.51,

10 Geometry of Nonlinear Supersymmetry 539 [7] Shima K. and Tsuda M., New supersymmetry algebra on gravitational interaction of Nambu Goldstone fermion, Phys. Lett. B, 001, V.507, [8] Samuel S. and Wess J., A superfield formulation of the non-linear realization of supersymmetry and its coupling to supergravity, Nucl. Phys. B, 1983, V.1, [9] Roček M., Linearlizing the Volkov Akulov model, Phys. Rev. Lett., 1978, V.41, ; Ivanov E.A. and Kapustnikov A.A., General relationship between linear and nonlinear realization of supersymmetry, J. Phys., 1978, ; Uematsu T. and Zachos C.K., Structure of phenomenological Lagrangians of broken supersymmetry, Nucl. Phys. B, 198, V.01, ; Wess J., Nonlinear realization of N = 1 supersymmetry, Karlsruhe University preprint, Festschrift for J. Lopszanski, 198. [10] Witten E., A new proof of the positive energy theorem, Commun. Math. Phys., 1981, V.80, [11] Shima K., Tsuda M. and Tanii Y., On linearlization of N = 1 Volkov Akulov model, Phys. Lett. B, to appear. [1] Seiberg N. and Witten E., Electric-magnetic duality, monopole condensation, and confinement in N = supersymmetric Yang Mills theory, Nucl. Phys. B, 1994, V.46, [13] Shima K. and Tsuda M., in preparation.

6.1. Dirac Equation. Hamiltonian. Dirac Eq.

6.1. Dirac Equation. Hamiltonian. Dirac Eq. 6.1. Dirac Equation Ref: M.Kaku, Quantum Field Theory, Oxford Univ Press (1993) η μν = η μν = diag(1, -1, -1, -1) p 0 = p 0 p = p i = -p i p μ p μ = p 0 p 0 + p i p i = E c 2 - p 2 = (m c) 2 H = c p 2

Διαβάστε περισσότερα

Space-Time Symmetries

Space-Time Symmetries Chapter Space-Time Symmetries In classical fiel theory any continuous symmetry of the action generates a conserve current by Noether's proceure. If the Lagrangian is not invariant but only shifts by a

Διαβάστε περισσότερα

Higher Derivative Gravity Theories

Higher Derivative Gravity Theories Higher Derivative Gravity Theories Black Holes in AdS space-times James Mashiyane Supervisor: Prof Kevin Goldstein University of the Witwatersrand Second Mandelstam, 20 January 2018 James Mashiyane WITS)

Διαβάστε περισσότερα

Symmetric Stress-Energy Tensor

Symmetric Stress-Energy Tensor Chapter 3 Symmetric Stress-Energy ensor We noticed that Noether s conserved currents are arbitrary up to the addition of a divergence-less field. Exploiting this freedom the canonical stress-energy tensor

Διαβάστε περισσότερα

Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3

Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3 Lecture 2: Dirac notation and a review of linear algebra Read Sakurai chapter 1, Baym chatper 3 1 State vector space and the dual space Space of wavefunctions The space of wavefunctions is the set of all

Διαβάστε περισσότερα

Phys460.nb Solution for the t-dependent Schrodinger s equation How did we find the solution? (not required)

Phys460.nb Solution for the t-dependent Schrodinger s equation How did we find the solution? (not required) Phys460.nb 81 ψ n (t) is still the (same) eigenstate of H But for tdependent H. The answer is NO. 5.5.5. Solution for the tdependent Schrodinger s equation If we assume that at time t 0, the electron starts

Διαβάστε περισσότερα

2 Composition. Invertible Mappings

2 Composition. Invertible Mappings Arkansas Tech University MATH 4033: Elementary Modern Algebra Dr. Marcel B. Finan Composition. Invertible Mappings In this section we discuss two procedures for creating new mappings from old ones, namely,

Διαβάστε περισσότερα

HOMEWORK 4 = G. In order to plot the stress versus the stretch we define a normalized stretch:

HOMEWORK 4 = G. In order to plot the stress versus the stretch we define a normalized stretch: HOMEWORK 4 Problem a For the fast loading case, we want to derive the relationship between P zz and λ z. We know that the nominal stress is expressed as: P zz = ψ λ z where λ z = λ λ z. Therefore, applying

Διαβάστε περισσότερα

4.6 Autoregressive Moving Average Model ARMA(1,1)

4.6 Autoregressive Moving Average Model ARMA(1,1) 84 CHAPTER 4. STATIONARY TS MODELS 4.6 Autoregressive Moving Average Model ARMA(,) This section is an introduction to a wide class of models ARMA(p,q) which we will consider in more detail later in this

Διαβάστε περισσότερα

= {{D α, D α }, D α }. = [D α, 4iσ µ α α D α µ ] = 4iσ µ α α [Dα, D α ] µ.

= {{D α, D α }, D α }. = [D α, 4iσ µ α α D α µ ] = 4iσ µ α α [Dα, D α ] µ. PHY 396 T: SUSY Solutions for problem set #1. Problem 2(a): First of all, [D α, D 2 D α D α ] = {D α, D α }D α D α {D α, D α } = {D α, D α }D α + D α {D α, D α } (S.1) = {{D α, D α }, D α }. Second, {D

Διαβάστε περισσότερα

EE512: Error Control Coding

EE512: Error Control Coding EE512: Error Control Coding Solution for Assignment on Finite Fields February 16, 2007 1. (a) Addition and Multiplication tables for GF (5) and GF (7) are shown in Tables 1 and 2. + 0 1 2 3 4 0 0 1 2 3

Διαβάστε περισσότερα

derivation of the Laplacian from rectangular to spherical coordinates

derivation of the Laplacian from rectangular to spherical coordinates derivation of the Laplacian from rectangular to spherical coordinates swapnizzle 03-03- :5:43 We begin by recognizing the familiar conversion from rectangular to spherical coordinates (note that φ is used

Διαβάστε περισσότερα

Homework 3 Solutions

Homework 3 Solutions Homework 3 Solutions Igor Yanovsky (Math 151A TA) Problem 1: Compute the absolute error and relative error in approximations of p by p. (Use calculator!) a) p π, p 22/7; b) p π, p 3.141. Solution: For

Διαβάστε περισσότερα

Every set of first-order formulas is equivalent to an independent set

Every set of first-order formulas is equivalent to an independent set Every set of first-order formulas is equivalent to an independent set May 6, 2008 Abstract A set of first-order formulas, whatever the cardinality of the set of symbols, is equivalent to an independent

Διαβάστε περισσότερα

Math221: HW# 1 solutions

Math221: HW# 1 solutions Math: HW# solutions Andy Royston October, 5 7.5.7, 3 rd Ed. We have a n = b n = a = fxdx = xdx =, x cos nxdx = x sin nx n sin nxdx n = cos nx n = n n, x sin nxdx = x cos nx n + cos nxdx n cos n = + sin

Διαβάστε περισσότερα

Strain gauge and rosettes

Strain gauge and rosettes Strain gauge and rosettes Introduction A strain gauge is a device which is used to measure strain (deformation) on an object subjected to forces. Strain can be measured using various types of devices classified

Διαβάστε περισσότερα

Congruence Classes of Invertible Matrices of Order 3 over F 2

Congruence Classes of Invertible Matrices of Order 3 over F 2 International Journal of Algebra, Vol. 8, 24, no. 5, 239-246 HIKARI Ltd, www.m-hikari.com http://dx.doi.org/.2988/ija.24.422 Congruence Classes of Invertible Matrices of Order 3 over F 2 Ligong An and

Διαβάστε περισσότερα

MATH423 String Theory Solutions 4. = 0 τ = f(s). (1) dτ ds = dxµ dτ f (s) (2) dτ 2 [f (s)] 2 + dxµ. dτ f (s) (3)

MATH423 String Theory Solutions 4. = 0 τ = f(s). (1) dτ ds = dxµ dτ f (s) (2) dτ 2 [f (s)] 2 + dxµ. dτ f (s) (3) 1. MATH43 String Theory Solutions 4 x = 0 τ = fs). 1) = = f s) ) x = x [f s)] + f s) 3) equation of motion is x = 0 if an only if f s) = 0 i.e. fs) = As + B with A, B constants. i.e. allowe reparametrisations

Διαβάστε περισσότερα

Statistical Inference I Locally most powerful tests

Statistical Inference I Locally most powerful tests Statistical Inference I Locally most powerful tests Shirsendu Mukherjee Department of Statistics, Asutosh College, Kolkata, India. shirsendu st@yahoo.co.in So far we have treated the testing of one-sided

Διαβάστε περισσότερα

C.S. 430 Assignment 6, Sample Solutions

C.S. 430 Assignment 6, Sample Solutions C.S. 430 Assignment 6, Sample Solutions Paul Liu November 15, 2007 Note that these are sample solutions only; in many cases there were many acceptable answers. 1 Reynolds Problem 10.1 1.1 Normal-order

Διαβάστε περισσότερα

Second Order Partial Differential Equations

Second Order Partial Differential Equations Chapter 7 Second Order Partial Differential Equations 7.1 Introduction A second order linear PDE in two independent variables (x, y Ω can be written as A(x, y u x + B(x, y u xy + C(x, y u u u + D(x, y

Διαβάστε περισσότερα

Higher spin gauge theories and their CFT duals

Higher spin gauge theories and their CFT duals Higher spin gauge theories and their CFT duals E-mail: hikida@phys-h.keio.ac.jp 2 AdS Vasiliev AdS/CFT 4 Vasiliev 3 O(N) 3 Vasiliev 2 W N 1 AdS/CFT g µν Vasiliev AdS [1] AdS/CFT anti-de Sitter (AdS) (CFT)

Διαβάστε περισσότερα

ΚΥΠΡΙΑΚΗ ΕΤΑΙΡΕΙΑ ΠΛΗΡΟΦΟΡΙΚΗΣ CYPRUS COMPUTER SOCIETY ΠΑΓΚΥΠΡΙΟΣ ΜΑΘΗΤΙΚΟΣ ΔΙΑΓΩΝΙΣΜΟΣ ΠΛΗΡΟΦΟΡΙΚΗΣ 6/5/2006

ΚΥΠΡΙΑΚΗ ΕΤΑΙΡΕΙΑ ΠΛΗΡΟΦΟΡΙΚΗΣ CYPRUS COMPUTER SOCIETY ΠΑΓΚΥΠΡΙΟΣ ΜΑΘΗΤΙΚΟΣ ΔΙΑΓΩΝΙΣΜΟΣ ΠΛΗΡΟΦΟΡΙΚΗΣ 6/5/2006 Οδηγίες: Να απαντηθούν όλες οι ερωτήσεις. Ολοι οι αριθμοί που αναφέρονται σε όλα τα ερωτήματα είναι μικρότεροι το 1000 εκτός αν ορίζεται διαφορετικά στη διατύπωση του προβλήματος. Διάρκεια: 3,5 ώρες Καλή

Διαβάστε περισσότερα

Cosmological Space-Times

Cosmological Space-Times Cosmological Space-Times Lecture notes compiled by Geoff Bicknell based primarily on: Sean Carroll: An Introduction to General Relativity plus additional material 1 Metric of special relativity ds 2 =

Διαβάστε περισσότερα

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013 Notes on Average Scattering imes and Hall Factors Jesse Maassen and Mar Lundstrom Purdue University November 5, 13 I. Introduction 1 II. Solution of the BE 1 III. Exercises: Woring out average scattering

Διαβάστε περισσότερα

Tutorial problem set 6,

Tutorial problem set 6, GENERAL RELATIVITY Tutorial problem set 6, 01.11.2013. SOLUTIONS PROBLEM 1 Killing vectors. a Show that the commutator of two Killing vectors is a Killing vector. Show that a linear combination with constant

Διαβάστε περισσότερα

Notes on the Open Economy

Notes on the Open Economy Notes on the Open Econom Ben J. Heijdra Universit of Groningen April 24 Introduction In this note we stud the two-countr model of Table.4 in more detail. restated here for convenience. The model is Table.4.

Διαβάστε περισσότερα

THE ENERGY-MOMENTUM TENSOR IN CLASSICAL FIELD THEORY

THE ENERGY-MOMENTUM TENSOR IN CLASSICAL FIELD THEORY THE ENERGY-MOMENTUM TENSOR IN CLASSICAL FIELD THEORY Walter Wyss Department of Physics University of Colorado Boulder, CO 80309 (Received 14 July 2005) My friend, Asim Barut, was always interested in classical

Διαβάστε περισσότερα

The kinetic and potential energies as T = 1 2. (m i η2 i k(η i+1 η i ) 2 ). (3) The Hooke s law F = Y ξ, (6) with a discrete analog

The kinetic and potential energies as T = 1 2. (m i η2 i k(η i+1 η i ) 2 ). (3) The Hooke s law F = Y ξ, (6) with a discrete analog Lecture 12: Introduction to Analytical Mechanics of Continuous Systems Lagrangian Density for Continuous Systems The kinetic and potential energies as T = 1 2 i η2 i (1 and V = 1 2 i+1 η i 2, i (2 where

Διαβάστε περισσότερα

Homework 8 Model Solution Section

Homework 8 Model Solution Section MATH 004 Homework Solution Homework 8 Model Solution Section 14.5 14.6. 14.5. Use the Chain Rule to find dz where z cosx + 4y), x 5t 4, y 1 t. dz dx + dy y sinx + 4y)0t + 4) sinx + 4y) 1t ) 0t + 4t ) sinx

Διαβάστε περισσότερα

Main source: "Discrete-time systems and computer control" by Α. ΣΚΟΔΡΑΣ ΨΗΦΙΑΚΟΣ ΕΛΕΓΧΟΣ ΔΙΑΛΕΞΗ 4 ΔΙΑΦΑΝΕΙΑ 1

Main source: Discrete-time systems and computer control by Α. ΣΚΟΔΡΑΣ ΨΗΦΙΑΚΟΣ ΕΛΕΓΧΟΣ ΔΙΑΛΕΞΗ 4 ΔΙΑΦΑΝΕΙΑ 1 Main source: "Discrete-time systems and computer control" by Α. ΣΚΟΔΡΑΣ ΨΗΦΙΑΚΟΣ ΕΛΕΓΧΟΣ ΔΙΑΛΕΞΗ 4 ΔΙΑΦΑΝΕΙΑ 1 A Brief History of Sampling Research 1915 - Edmund Taylor Whittaker (1873-1956) devised a

Διαβάστε περισσότερα

Relativistic particle dynamics and deformed symmetry

Relativistic particle dynamics and deformed symmetry Relativistic particle dynamics and deformed Poincare symmetry Department for Theoretical Physics, Ivan Franko Lviv National University XXXIII Max Born Symposium, Wroclaw Outline Lorentz-covariant deformed

Διαβάστε περισσότερα

Απόκριση σε Μοναδιαία Ωστική Δύναμη (Unit Impulse) Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο. Απόστολος Σ.

Απόκριση σε Μοναδιαία Ωστική Δύναμη (Unit Impulse) Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο. Απόστολος Σ. Απόκριση σε Δυνάμεις Αυθαίρετα Μεταβαλλόμενες με το Χρόνο The time integral of a force is referred to as impulse, is determined by and is obtained from: Newton s 2 nd Law of motion states that the action

Διαβάστε περισσότερα

Section 8.3 Trigonometric Equations

Section 8.3 Trigonometric Equations 99 Section 8. Trigonometric Equations Objective 1: Solve Equations Involving One Trigonometric Function. In this section and the next, we will exple how to solving equations involving trigonometric functions.

Διαβάστε περισσότερα

Written Examination. Antennas and Propagation (AA ) April 26, 2017.

Written Examination. Antennas and Propagation (AA ) April 26, 2017. Written Examination Antennas and Propagation (AA. 6-7) April 6, 7. Problem ( points) Let us consider a wire antenna as in Fig. characterized by a z-oriented linear filamentary current I(z) = I cos(kz)ẑ

Διαβάστε περισσότερα

ECE Spring Prof. David R. Jackson ECE Dept. Notes 2

ECE Spring Prof. David R. Jackson ECE Dept. Notes 2 ECE 634 Spring 6 Prof. David R. Jackson ECE Dept. Notes Fields in a Source-Free Region Example: Radiation from an aperture y PEC E t x Aperture Assume the following choice of vector potentials: A F = =

Διαβάστε περισσότερα

Other Test Constructions: Likelihood Ratio & Bayes Tests

Other Test Constructions: Likelihood Ratio & Bayes Tests Other Test Constructions: Likelihood Ratio & Bayes Tests Side-Note: So far we have seen a few approaches for creating tests such as Neyman-Pearson Lemma ( most powerful tests of H 0 : θ = θ 0 vs H 1 :

Διαβάστε περισσότερα

Finite Field Problems: Solutions

Finite Field Problems: Solutions Finite Field Problems: Solutions 1. Let f = x 2 +1 Z 11 [x] and let F = Z 11 [x]/(f), a field. Let Solution: F =11 2 = 121, so F = 121 1 = 120. The possible orders are the divisors of 120. Solution: The

Διαβάστε περισσότερα

CRASH COURSE IN PRECALCULUS

CRASH COURSE IN PRECALCULUS CRASH COURSE IN PRECALCULUS Shiah-Sen Wang The graphs are prepared by Chien-Lun Lai Based on : Precalculus: Mathematics for Calculus by J. Stuwart, L. Redin & S. Watson, 6th edition, 01, Brooks/Cole Chapter

Διαβάστε περισσότερα

3.4 SUM AND DIFFERENCE FORMULAS. NOTE: cos(α+β) cos α + cos β cos(α-β) cos α -cos β

3.4 SUM AND DIFFERENCE FORMULAS. NOTE: cos(α+β) cos α + cos β cos(α-β) cos α -cos β 3.4 SUM AND DIFFERENCE FORMULAS Page Theorem cos(αβ cos α cos β -sin α cos(α-β cos α cos β sin α NOTE: cos(αβ cos α cos β cos(α-β cos α -cos β Proof of cos(α-β cos α cos β sin α Let s use a unit circle

Διαβάστε περισσότερα

Homework 3 Solutions

Homework 3 Solutions Homework 3 s Free graviton Hamiltonian Show that the free graviton action we discussed in class (before making it gauge- and Lorentzinvariant), S 0 = α d 4 x µ h ij µ h ij, () yields the correct free Hamiltonian

Διαβάστε περισσότερα

the total number of electrons passing through the lamp.

the total number of electrons passing through the lamp. 1. A 12 V 36 W lamp is lit to normal brightness using a 12 V car battery of negligible internal resistance. The lamp is switched on for one hour (3600 s). For the time of 1 hour, calculate (i) the energy

Διαβάστε περισσότερα

상대론적고에너지중이온충돌에서 제트입자와관련된제동복사 박가영 인하대학교 윤진희교수님, 권민정교수님

상대론적고에너지중이온충돌에서 제트입자와관련된제동복사 박가영 인하대학교 윤진희교수님, 권민정교수님 상대론적고에너지중이온충돌에서 제트입자와관련된제동복사 박가영 인하대학교 윤진희교수님, 권민정교수님 Motivation Bremsstrahlung is a major rocess losing energies while jet articles get through the medium. BUT it should be quite different from low energy

Διαβάστε περισσότερα

Matrices and Determinants

Matrices and Determinants Matrices and Determinants SUBJECTIVE PROBLEMS: Q 1. For what value of k do the following system of equations possess a non-trivial (i.e., not all zero) solution over the set of rationals Q? x + ky + 3z

Διαβάστε περισσότερα

Partial Differential Equations in Biology The boundary element method. March 26, 2013

Partial Differential Equations in Biology The boundary element method. March 26, 2013 The boundary element method March 26, 203 Introduction and notation The problem: u = f in D R d u = ϕ in Γ D u n = g on Γ N, where D = Γ D Γ N, Γ D Γ N = (possibly, Γ D = [Neumann problem] or Γ N = [Dirichlet

Διαβάστε περισσότερα

Example Sheet 3 Solutions

Example Sheet 3 Solutions Example Sheet 3 Solutions. i Regular Sturm-Liouville. ii Singular Sturm-Liouville mixed boundary conditions. iii Not Sturm-Liouville ODE is not in Sturm-Liouville form. iv Regular Sturm-Liouville note

Διαβάστε περισσότερα

ST5224: Advanced Statistical Theory II

ST5224: Advanced Statistical Theory II ST5224: Advanced Statistical Theory II 2014/2015: Semester II Tutorial 7 1. Let X be a sample from a population P and consider testing hypotheses H 0 : P = P 0 versus H 1 : P = P 1, where P j is a known

Διαβάστε περισσότερα

SPONTANEOUS GENERATION OF GEOMETRY IN 4D

SPONTANEOUS GENERATION OF GEOMETRY IN 4D SPONTANEOUS GENERATION OF GEOMETRY IN 4D Dani Puigdomènch Dual year Russia-Spain: Particle Physics, Nuclear Physics and Astroparticle Physics 10/11/11 Based on arxiv: 1004.3664 and wor on progress. by

Διαβάστε περισσότερα

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS CHAPTER 5 SOLVING EQUATIONS BY ITERATIVE METHODS EXERCISE 104 Page 8 1. Find the positive root of the equation x + 3x 5 = 0, correct to 3 significant figures, using the method of bisection. Let f(x) =

Διαβάστε περισσότερα

Problem Set 9 Solutions. θ + 1. θ 2 + cotθ ( ) sinθ e iφ is an eigenfunction of the ˆ L 2 operator. / θ 2. φ 2. sin 2 θ φ 2. ( ) = e iφ. = e iφ cosθ.

Problem Set 9 Solutions. θ + 1. θ 2 + cotθ ( ) sinθ e iφ is an eigenfunction of the ˆ L 2 operator. / θ 2. φ 2. sin 2 θ φ 2. ( ) = e iφ. = e iφ cosθ. Chemistry 362 Dr Jean M Standard Problem Set 9 Solutions The ˆ L 2 operator is defined as Verify that the angular wavefunction Y θ,φ) Also verify that the eigenvalue is given by 2! 2 & L ˆ 2! 2 2 θ 2 +

Διαβάστε περισσότερα

Areas and Lengths in Polar Coordinates

Areas and Lengths in Polar Coordinates Kiryl Tsishchanka Areas and Lengths in Polar Coordinates In this section we develop the formula for the area of a region whose boundary is given by a polar equation. We need to use the formula for the

Διαβάστε περισσότερα

Symmetry. March 31, 2013

Symmetry. March 31, 2013 Symmetry March 3, 203 The Lie Derivative With or without the covariant derivative, which requires a connection on all of spacetime, there is another sort of derivation called the Lie derivative, which

Διαβάστε περισσότερα

ΚΥΠΡΙΑΚΗ ΕΤΑΙΡΕΙΑ ΠΛΗΡΟΦΟΡΙΚΗΣ CYPRUS COMPUTER SOCIETY ΠΑΓΚΥΠΡΙΟΣ ΜΑΘΗΤΙΚΟΣ ΔΙΑΓΩΝΙΣΜΟΣ ΠΛΗΡΟΦΟΡΙΚΗΣ 19/5/2007

ΚΥΠΡΙΑΚΗ ΕΤΑΙΡΕΙΑ ΠΛΗΡΟΦΟΡΙΚΗΣ CYPRUS COMPUTER SOCIETY ΠΑΓΚΥΠΡΙΟΣ ΜΑΘΗΤΙΚΟΣ ΔΙΑΓΩΝΙΣΜΟΣ ΠΛΗΡΟΦΟΡΙΚΗΣ 19/5/2007 Οδηγίες: Να απαντηθούν όλες οι ερωτήσεις. Αν κάπου κάνετε κάποιες υποθέσεις να αναφερθούν στη σχετική ερώτηση. Όλα τα αρχεία που αναφέρονται στα προβλήματα βρίσκονται στον ίδιο φάκελο με το εκτελέσιμο

Διαβάστε περισσότερα

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit Ting Zhang Stanford May 11, 2001 Stanford, 5/11/2001 1 Outline Ordinal Classification Ordinal Addition Ordinal Multiplication Ordinal

Διαβάστε περισσότερα

Lecture 15 - Root System Axiomatics

Lecture 15 - Root System Axiomatics Lecture 15 - Root System Axiomatics Nov 1, 01 In this lecture we examine root systems from an axiomatic point of view. 1 Reflections If v R n, then it determines a hyperplane, denoted P v, through the

Διαβάστε περισσότερα

Reminders: linear functions

Reminders: linear functions Reminders: linear functions Let U and V be vector spaces over the same field F. Definition A function f : U V is linear if for every u 1, u 2 U, f (u 1 + u 2 ) = f (u 1 ) + f (u 2 ), and for every u U

Διαβάστε περισσότερα

Dr. D. Dinev, Department of Structural Mechanics, UACEG

Dr. D. Dinev, Department of Structural Mechanics, UACEG Lecture 4 Material behavior: Constitutive equations Field of the game Print version Lecture on Theory of lasticity and Plasticity of Dr. D. Dinev, Department of Structural Mechanics, UACG 4.1 Contents

Διαβάστε περισσότερα

On a four-dimensional hyperbolic manifold with finite volume

On a four-dimensional hyperbolic manifold with finite volume BULETINUL ACADEMIEI DE ŞTIINŢE A REPUBLICII MOLDOVA. MATEMATICA Numbers 2(72) 3(73), 2013, Pages 80 89 ISSN 1024 7696 On a four-dimensional hyperbolic manifold with finite volume I.S.Gutsul Abstract. In

Διαβάστε περισσότερα

The Simply Typed Lambda Calculus

The Simply Typed Lambda Calculus Type Inference Instead of writing type annotations, can we use an algorithm to infer what the type annotations should be? That depends on the type system. For simple type systems the answer is yes, and

Διαβάστε περισσότερα

A Short Introduction to Tensors

A Short Introduction to Tensors May 2, 2007 Tensors: Scalars and Vectors Any physical quantity, e.g. the velocity of a particle, is determined by a set of numerical values - its components - which depend on the coordinate system. Studying

Διαβάστε περισσότερα

Approximation of distance between locations on earth given by latitude and longitude

Approximation of distance between locations on earth given by latitude and longitude Approximation of distance between locations on earth given by latitude and longitude Jan Behrens 2012-12-31 In this paper we shall provide a method to approximate distances between two points on earth

Διαβάστε περισσότερα

Chapter 6: Systems of Linear Differential. be continuous functions on the interval

Chapter 6: Systems of Linear Differential. be continuous functions on the interval Chapter 6: Systems of Linear Differential Equations Let a (t), a 2 (t),..., a nn (t), b (t), b 2 (t),..., b n (t) be continuous functions on the interval I. The system of n first-order differential equations

Διαβάστε περισσότερα

Η αλληλεπίδραση ανάμεσα στην καθημερινή γλώσσα και την επιστημονική ορολογία: παράδειγμα από το πεδίο της Κοσμολογίας

Η αλληλεπίδραση ανάμεσα στην καθημερινή γλώσσα και την επιστημονική ορολογία: παράδειγμα από το πεδίο της Κοσμολογίας Η αλληλεπίδραση ανάμεσα στην καθημερινή γλώσσα και την επιστημονική ορολογία: παράδειγμα από το πεδίο της Κοσμολογίας ΠΕΡΙΛΗΨΗ Αριστείδης Κοσιονίδης Η κατανόηση των εννοιών ενός επιστημονικού πεδίου απαιτεί

Διαβάστε περισσότερα

Econ 2110: Fall 2008 Suggested Solutions to Problem Set 8 questions or comments to Dan Fetter 1

Econ 2110: Fall 2008 Suggested Solutions to Problem Set 8  questions or comments to Dan Fetter 1 Eon : Fall 8 Suggested Solutions to Problem Set 8 Email questions or omments to Dan Fetter Problem. Let X be a salar with density f(x, θ) (θx + θ) [ x ] with θ. (a) Find the most powerful level α test

Διαβάστε περισσότερα

Tridiagonal matrices. Gérard MEURANT. October, 2008

Tridiagonal matrices. Gérard MEURANT. October, 2008 Tridiagonal matrices Gérard MEURANT October, 2008 1 Similarity 2 Cholesy factorizations 3 Eigenvalues 4 Inverse Similarity Let α 1 ω 1 β 1 α 2 ω 2 T =......... β 2 α 1 ω 1 β 1 α and β i ω i, i = 1,...,

Διαβάστε περισσότερα

Spherical Coordinates

Spherical Coordinates Spherical Coordinates MATH 311, Calculus III J. Robert Buchanan Department of Mathematics Fall 2011 Spherical Coordinates Another means of locating points in three-dimensional space is known as the spherical

Διαβάστε περισσότερα

DERIVATION OF MILES EQUATION FOR AN APPLIED FORCE Revision C

DERIVATION OF MILES EQUATION FOR AN APPLIED FORCE Revision C DERIVATION OF MILES EQUATION FOR AN APPLIED FORCE Revision C By Tom Irvine Email: tomirvine@aol.com August 6, 8 Introduction The obective is to derive a Miles equation which gives the overall response

Διαβάστε περισσότερα

ω ω ω ω ω ω+2 ω ω+2 + ω ω ω ω+2 + ω ω+1 ω ω+2 2 ω ω ω ω ω ω ω ω+1 ω ω2 ω ω2 + ω ω ω2 + ω ω ω ω2 + ω ω+1 ω ω2 + ω ω+1 + ω ω ω ω2 + ω

ω ω ω ω ω ω+2 ω ω+2 + ω ω ω ω+2 + ω ω+1 ω ω+2 2 ω ω ω ω ω ω ω ω+1 ω ω2 ω ω2 + ω ω ω2 + ω ω ω ω2 + ω ω+1 ω ω2 + ω ω+1 + ω ω ω ω2 + ω 0 1 2 3 4 5 6 ω ω + 1 ω + 2 ω + 3 ω + 4 ω2 ω2 + 1 ω2 + 2 ω2 + 3 ω3 ω3 + 1 ω3 + 2 ω4 ω4 + 1 ω5 ω 2 ω 2 + 1 ω 2 + 2 ω 2 + ω ω 2 + ω + 1 ω 2 + ω2 ω 2 2 ω 2 2 + 1 ω 2 2 + ω ω 2 3 ω 3 ω 3 + 1 ω 3 + ω ω 3 +

Διαβάστε περισσότερα

Areas and Lengths in Polar Coordinates

Areas and Lengths in Polar Coordinates Kiryl Tsishchanka Areas and Lengths in Polar Coordinates In this section we develop the formula for the area of a region whose boundary is given by a polar equation. We need to use the formula for the

Διαβάστε περισσότερα

A Note on Intuitionistic Fuzzy. Equivalence Relation

A Note on Intuitionistic Fuzzy. Equivalence Relation International Mathematical Forum, 5, 2010, no. 67, 3301-3307 A Note on Intuitionistic Fuzzy Equivalence Relation D. K. Basnet Dept. of Mathematics, Assam University Silchar-788011, Assam, India dkbasnet@rediffmail.com

Διαβάστε περισσότερα

Riemannian Curvature

Riemannian Curvature Riemannian Curvature February 6, 013 We now generalize our computation of curvature to arbitrary spaces. 1 Parallel transport around a small closed loop We compute the change in a vector, w, which we parallel

Διαβάστε περισσότερα

Démographie spatiale/spatial Demography

Démographie spatiale/spatial Demography ΠΑΝΕΠΙΣΤΗΜΙΟ ΘΕΣΣΑΛΙΑΣ Démographie spatiale/spatial Demography Session 1: Introduction to spatial demography Basic concepts Michail Agorastakis Department of Planning & Regional Development Άδειες Χρήσης

Διαβάστε περισσότερα

8.324 Relativistic Quantum Field Theory II

8.324 Relativistic Quantum Field Theory II 8.324 Relativistic Quantum Field Theory II MIT OpenCourseWare Lecture Notes Hong Liu, Fall 200 Lecture 2 3: GENERAL ASPECTS OF QUANTUM ELECTRODYNAMICS 3.: RENORMALIZED LAGRANGIAN Consider the Lagrangian

Διαβάστε περισσότερα

forms This gives Remark 1. How to remember the above formulas: Substituting these into the equation we obtain with

forms This gives Remark 1. How to remember the above formulas: Substituting these into the equation we obtain with Week 03: C lassification of S econd- Order L inear Equations In last week s lectures we have illustrated how to obtain the general solutions of first order PDEs using the method of characteristics. We

Διαβάστε περισσότερα

Orbital angular momentum and the spherical harmonics

Orbital angular momentum and the spherical harmonics Orbital angular momentum and the spherical harmonics March 8, 03 Orbital angular momentum We compare our result on representations of rotations with our previous experience of angular momentum, defined

Διαβάστε περισσότερα

1 String with massive end-points

1 String with massive end-points 1 String with massive end-points Πρόβλημα 5.11:Θεωρείστε μια χορδή μήκους, τάσης T, με δύο σημειακά σωματίδια στα άκρα της, το ένα μάζας m, και το άλλο μάζας m. α) Μελετώντας την κίνηση των άκρων βρείτε

Διαβάστε περισσότερα

Geodesic Equations for the Wormhole Metric

Geodesic Equations for the Wormhole Metric Geodesic Equations for the Wormhole Metric Dr R Herman Physics & Physical Oceanography, UNCW February 14, 2018 The Wormhole Metric Morris and Thorne wormhole metric: [M S Morris, K S Thorne, Wormholes

Διαβάστε περισσότερα

k A = [k, k]( )[a 1, a 2 ] = [ka 1,ka 2 ] 4For the division of two intervals of confidence in R +

k A = [k, k]( )[a 1, a 2 ] = [ka 1,ka 2 ] 4For the division of two intervals of confidence in R + Chapter 3. Fuzzy Arithmetic 3- Fuzzy arithmetic: ~Addition(+) and subtraction (-): Let A = [a and B = [b, b in R If x [a and y [b, b than x+y [a +b +b Symbolically,we write A(+)B = [a (+)[b, b = [a +b

Διαβάστε περισσότερα

Parametrized Surfaces

Parametrized Surfaces Parametrized Surfaces Recall from our unit on vector-valued functions at the beginning of the semester that an R 3 -valued function c(t) in one parameter is a mapping of the form c : I R 3 where I is some

Διαβάστε περισσότερα

Second Order RLC Filters

Second Order RLC Filters ECEN 60 Circuits/Electronics Spring 007-0-07 P. Mathys Second Order RLC Filters RLC Lowpass Filter A passive RLC lowpass filter (LPF) circuit is shown in the following schematic. R L C v O (t) Using phasor

Διαβάστε περισσότερα

Appendix to On the stability of a compressible axisymmetric rotating flow in a pipe. By Z. Rusak & J. H. Lee

Appendix to On the stability of a compressible axisymmetric rotating flow in a pipe. By Z. Rusak & J. H. Lee Appendi to On the stability of a compressible aisymmetric rotating flow in a pipe By Z. Rusak & J. H. Lee Journal of Fluid Mechanics, vol. 5 4, pp. 5 4 This material has not been copy-edited or typeset

Διαβάστε περισσότερα

Phys624 Quantization of Scalar Fields II Homework 3. Homework 3 Solutions. 3.1: U(1) symmetry for complex scalar

Phys624 Quantization of Scalar Fields II Homework 3. Homework 3 Solutions. 3.1: U(1) symmetry for complex scalar Homework 3 Solutions 3.1: U(1) symmetry for complex scalar 1 3.: Two complex scalars The Lagrangian for two complex scalar fields is given by, L µ φ 1 µ φ 1 m φ 1φ 1 + µ φ µ φ m φ φ (1) This can be written

Διαβάστε περισσότερα

Calculating the propagation delay of coaxial cable

Calculating the propagation delay of coaxial cable Your source for quality GNSS Networking Solutions and Design Services! Page 1 of 5 Calculating the propagation delay of coaxial cable The delay of a cable or velocity factor is determined by the dielectric

Διαβάστε περισσότερα

[1] P Q. Fig. 3.1

[1] P Q. Fig. 3.1 1 (a) Define resistance....... [1] (b) The smallest conductor within a computer processing chip can be represented as a rectangular block that is one atom high, four atoms wide and twenty atoms long. One

Διαβάστε περισσότερα

SCITECH Volume 13, Issue 2 RESEARCH ORGANISATION Published online: March 29, 2018

SCITECH Volume 13, Issue 2 RESEARCH ORGANISATION Published online: March 29, 2018 Journal of rogressive Research in Mathematics(JRM) ISSN: 2395-028 SCITECH Volume 3, Issue 2 RESEARCH ORGANISATION ublished online: March 29, 208 Journal of rogressive Research in Mathematics www.scitecresearch.com/journals

Διαβάστε περισσότερα

5. Choice under Uncertainty

5. Choice under Uncertainty 5. Choice under Uncertainty Daisuke Oyama Microeconomics I May 23, 2018 Formulations von Neumann-Morgenstern (1944/1947) X: Set of prizes Π: Set of probability distributions on X : Preference relation

Διαβάστε περισσότερα

Right Rear Door. Let's now finish the door hinge saga with the right rear door

Right Rear Door. Let's now finish the door hinge saga with the right rear door Right Rear Door Let's now finish the door hinge saga with the right rear door You may have been already guessed my steps, so there is not much to describe in detail. Old upper one file:///c /Documents

Διαβάστε περισσότερα

DESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0.

DESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0. DESIGN OF MACHINERY SOLUTION MANUAL -7-1! PROBLEM -7 Statement: Design a double-dwell cam to move a follower from to 25 6, dwell for 12, fall 25 and dwell for the remader The total cycle must take 4 sec

Διαβάστε περισσότερα

Section 1: Listening and responding. Presenter: Niki Farfara MGTAV VCE Seminar 7 August 2016

Section 1: Listening and responding. Presenter: Niki Farfara MGTAV VCE Seminar 7 August 2016 Section 1: Listening and responding Presenter: Niki Farfara MGTAV VCE Seminar 7 August 2016 Section 1: Listening and responding Section 1: Listening and Responding/ Aκουστική εξέταση Στο πρώτο μέρος της

Διαβάστε περισσότερα

Concrete Mathematics Exercises from 30 September 2016

Concrete Mathematics Exercises from 30 September 2016 Concrete Mathematics Exercises from 30 September 2016 Silvio Capobianco Exercise 1.7 Let H(n) = J(n + 1) J(n). Equation (1.8) tells us that H(2n) = 2, and H(2n+1) = J(2n+2) J(2n+1) = (2J(n+1) 1) (2J(n)+1)

Διαβάστε περισσότερα

Example of the Baum-Welch Algorithm

Example of the Baum-Welch Algorithm Example of the Baum-Welch Algorithm Larry Moss Q520, Spring 2008 1 Our corpus c We start with a very simple corpus. We take the set Y of unanalyzed words to be {ABBA, BAB}, and c to be given by c(abba)

Διαβάστε περισσότερα

Assalamu `alaikum wr. wb.

Assalamu `alaikum wr. wb. LUMP SUM Assalamu `alaikum wr. wb. LUMP SUM Wassalamu alaikum wr. wb. Assalamu `alaikum wr. wb. LUMP SUM Wassalamu alaikum wr. wb. LUMP SUM Lump sum lump sum lump sum. lump sum fixed price lump sum lump

Διαβάστε περισσότερα

department listing department name αχχουντσ ϕανε βαλικτ δδσϕηασδδη σδηφγ ασκϕηλκ τεχηνιχαλ αλαν ϕουν διξ τεχηνιχαλ ϕοην µαριανι

department listing department name αχχουντσ ϕανε βαλικτ δδσϕηασδδη σδηφγ ασκϕηλκ τεχηνιχαλ αλαν ϕουν διξ τεχηνιχαλ ϕοην µαριανι She selects the option. Jenny starts with the al listing. This has employees listed within She drills down through the employee. The inferred ER sttricture relates this to the redcords in the databasee

Διαβάστε περισσότερα

w o = R 1 p. (1) R = p =. = 1

w o = R 1 p. (1) R = p =. = 1 Πανεπιστήµιο Κρήτης - Τµήµα Επιστήµης Υπολογιστών ΗΥ-570: Στατιστική Επεξεργασία Σήµατος 205 ιδάσκων : Α. Μουχτάρης Τριτη Σειρά Ασκήσεων Λύσεις Ασκηση 3. 5.2 (a) From the Wiener-Hopf equation we have:

Διαβάστε περισσότερα

On the Galois Group of Linear Difference-Differential Equations

On the Galois Group of Linear Difference-Differential Equations On the Galois Group of Linear Difference-Differential Equations Ruyong Feng KLMM, Chinese Academy of Sciences, China Ruyong Feng (KLMM, CAS) Galois Group 1 / 19 Contents 1 Basic Notations and Concepts

Διαβάστε περισσότερα

Section 9.2 Polar Equations and Graphs

Section 9.2 Polar Equations and Graphs 180 Section 9. Polar Equations and Graphs In this section, we will be graphing polar equations on a polar grid. In the first few examples, we will write the polar equation in rectangular form to help identify

Διαβάστε περισσότερα

ΠΑΝΕΠΙΣΤΗΜΙΟ ΠΕΙΡΑΙΑ ΤΜΗΜΑ ΝΑΥΤΙΛΙΑΚΩΝ ΣΠΟΥΔΩΝ ΠΡΟΓΡΑΜΜΑ ΜΕΤΑΠΤΥΧΙΑΚΩΝ ΣΠΟΥΔΩΝ ΣΤΗΝ ΝΑΥΤΙΛΙΑ

ΠΑΝΕΠΙΣΤΗΜΙΟ ΠΕΙΡΑΙΑ ΤΜΗΜΑ ΝΑΥΤΙΛΙΑΚΩΝ ΣΠΟΥΔΩΝ ΠΡΟΓΡΑΜΜΑ ΜΕΤΑΠΤΥΧΙΑΚΩΝ ΣΠΟΥΔΩΝ ΣΤΗΝ ΝΑΥΤΙΛΙΑ ΠΑΝΕΠΙΣΤΗΜΙΟ ΠΕΙΡΑΙΑ ΤΜΗΜΑ ΝΑΥΤΙΛΙΑΚΩΝ ΣΠΟΥΔΩΝ ΠΡΟΓΡΑΜΜΑ ΜΕΤΑΠΤΥΧΙΑΚΩΝ ΣΠΟΥΔΩΝ ΣΤΗΝ ΝΑΥΤΙΛΙΑ ΝΟΜΙΚΟ ΚΑΙ ΘΕΣΜΙΚΟ ΦΟΡΟΛΟΓΙΚΟ ΠΛΑΙΣΙΟ ΚΤΗΣΗΣ ΚΑΙ ΕΚΜΕΤΑΛΛΕΥΣΗΣ ΠΛΟΙΟΥ ΔΙΠΛΩΜΑΤΙΚΗ ΕΡΓΑΣΙΑ που υποβλήθηκε στο

Διαβάστε περισσότερα

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions SCHOOL OF MATHEMATICAL SCIENCES GLMA Linear Mathematics 00- Examination Solutions. (a) i. ( + 5i)( i) = (6 + 5) + (5 )i = + i. Real part is, imaginary part is. (b) ii. + 5i i ( + 5i)( + i) = ( i)( + i)

Διαβάστε περισσότερα

1 Poincare group and spinors

1 Poincare group and spinors Introduction on Supersymmetry Di Xu 1 Poincare group and spinors A Poincare transformation P is a proper Lorentz transformation Λ followed by a translation a. The generators of the Poincare group are the

Διαβάστε περισσότερα

3+1 Splitting of the Generalized Harmonic Equations

3+1 Splitting of the Generalized Harmonic Equations 3+1 Splitting of the Generalized Harmonic Equations David Brown North Carolina State University EGM June 2011 Numerical Relativity Interpret general relativity as an initial value problem: Split spacetime

Διαβάστε περισσότερα