Geometry of Nonlinear Supersymmetry in Curved Spacetime and Unity of Nature

Σχετικά έγγραφα
6.1. Dirac Equation. Hamiltonian. Dirac Eq.

Space-Time Symmetries

Higher Derivative Gravity Theories

Symmetric Stress-Energy Tensor

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

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

2 Composition. Invertible Mappings

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

4.6 Autoregressive Moving Average Model ARMA(1,1)

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

EE512: Error Control Coding

derivation of the Laplacian from rectangular to spherical coordinates

Homework 3 Solutions

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

Math221: HW# 1 solutions

Strain gauge and rosettes

Congruence Classes of Invertible Matrices of Order 3 over F 2

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)

Statistical Inference I Locally most powerful tests

C.S. 430 Assignment 6, Sample Solutions

Second Order Partial Differential Equations

Higher spin gauge theories and their CFT duals

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

Cosmological Space-Times

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013

Tutorial problem set 6,

Notes on the Open Economy

THE ENERGY-MOMENTUM TENSOR IN CLASSICAL FIELD THEORY

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

Homework 8 Model Solution Section

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

Relativistic particle dynamics and deformed symmetry

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

Section 8.3 Trigonometric Equations

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

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

Other Test Constructions: Likelihood Ratio & Bayes Tests

Finite Field Problems: Solutions

CRASH COURSE IN PRECALCULUS

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

Homework 3 Solutions

the total number of electrons passing through the lamp.

상대론적고에너지중이온충돌에서 제트입자와관련된제동복사 박가영 인하대학교 윤진희교수님, 권민정교수님

Matrices and Determinants

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

Example Sheet 3 Solutions

ST5224: Advanced Statistical Theory II

SPONTANEOUS GENERATION OF GEOMETRY IN 4D

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS

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.

Areas and Lengths in Polar Coordinates

Symmetry. March 31, 2013

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

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit

Lecture 15 - Root System Axiomatics

Reminders: linear functions

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

On a four-dimensional hyperbolic manifold with finite volume

The Simply Typed Lambda Calculus

A Short Introduction to Tensors

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

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

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

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

Tridiagonal matrices. Gérard MEURANT. October, 2008

Spherical Coordinates

DERIVATION OF MILES EQUATION FOR AN APPLIED FORCE Revision C

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

Areas and Lengths in Polar Coordinates

A Note on Intuitionistic Fuzzy. Equivalence Relation

Riemannian Curvature

Démographie spatiale/spatial Demography

8.324 Relativistic Quantum Field Theory II

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

Orbital angular momentum and the spherical harmonics

1 String with massive end-points

Geodesic Equations for the Wormhole Metric

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

Parametrized Surfaces

Second Order RLC Filters

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

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

Calculating the propagation delay of coaxial cable

[1] P Q. Fig. 3.1

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

5. Choice under Uncertainty

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

DESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0.

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

Concrete Mathematics Exercises from 30 September 2016

Example of the Baum-Welch Algorithm

Assalamu `alaikum wr. wb.

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

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

On the Galois Group of Linear Difference-Differential Equations

Section 9.2 Polar Equations and Graphs

ΠΑΝΕΠΙΣΤΗΜΙΟ ΠΕΙΡΑΙΑ ΤΜΗΜΑ ΝΑΥΤΙΛΙΑΚΩΝ ΣΠΟΥΔΩΝ ΠΡΟΓΡΑΜΜΑ ΜΕΤΑΠΤΥΧΙΑΚΩΝ ΣΠΟΥΔΩΝ ΣΤΗΝ ΝΑΥΤΙΛΙΑ

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions

1 Poincare group and spinors

3+1 Splitting of the Generalized Harmonic Equations

Transcript:

Proceedings of Institute of Mathematics of NAS of Ukraine 00, Vol. 43, Part, 530 539 Geometry of Nonlinear Supersymmetry in Curved Spacetime and Unity of Nature Kazunari SHIMA Laboratory of Physics, Saitama Institute of Technology, Okabe-machi, Saitama 369-093, Japan E-mail: shima@sit.ac.jp 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.

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

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.

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 + 1 + 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 4 + + 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

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 + 1 + 1+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

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

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

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-

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, 33 36. [] Volkov D.V. and Akulov V.P., Is neutrino a Goldstone particle?, Phys. Lett. B, 1973, V.46, 109 110. [3] Shima K., Superon-quintet and graviton model for supersymmetric spacetime and matter, European Phys. J. C, 1999, V.7, 341 345. [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, 37 44. [6] Shima K. and Tsuda M., On gravitational interaction of spin 3/ Nambu Goldstone fermion, Phys. Lett. B, 001, V.51, 67 70.

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, 60 64. [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, 153 177. [9] Roček M., Linearlizing the Volkov Akulov model, Phys. Rev. Lett., 1978, V.41, 451 453; Ivanov E.A. and Kapustnikov A.A., General relationship between linear and nonlinear realization of supersymmetry, J. Phys., 1978, 375 384; Uematsu T. and Zachos C.K., Structure of phenomenological Lagrangians of broken supersymmetry, Nucl. Phys. B, 198, V.01, 54 301; 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, 381 40. [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, 19 35. [13] Shima K. and Tsuda M., in preparation.