Effective mass of nonrelativistic quantum electrodynamics
|
|
- Βάαλ Γιάνναρης
- 7 χρόνια πριν
- Προβολές:
Transcript
1 Effective mass of nonrelativistic quantum electrodynamics Fumio Hiroshima and K. R. Ito ecember 6, 5 Abstract The effective mass m eff of the nonrelativistic quantum electrodynamics with spin / is investigated. Let m eff /m = + a (Λ/me + a (Λ/me 4 + O(e 6, where m denotes the bare mass. a (Λ/m log(λ/m as Λ is well known. Also a (Λ/m Λ/m is established for a spinless case. It is shown that a (Λ/m (Λ/m in the case including spin /. Introduction. Quantum electrodynamics In this review we study an translation-invariant Hamiltonian minimally coupled to a quantized radiation field in the nonrelativistic quantum electrodynamics. Before going to discuss our problem, we informally derive our Hamiltonian from physical point of view. The conventional quantum electrodynamics is investigated through the Lagrangian density: L QE (x = ψ(x(iγ µ µ mψ(x 4 F µν(xf µν (x eψ(xγ µ ψ(xa µ (x, where x = (x, x R R 3, γ µ, µ =,,, 3, denotes 4 4 gamma matrices, ψ the spinor given by ψ = (ψ, ψ, ψ, ψ 3 T and ψ = ( ψ, ψ, ψ, ψ 3 γ, A µ (x a radiation field with F µν := µ A ν ν A µ, and m, e are the mass and the charge of an electron, respectively. The effective mass m eff is given through two point function R 4 (Ψ, T [ψ(xψ(]ψe i(x p x p dx and the effective charge through the two point function R 4 (Ψ, T [A µ (xa ν (]Ψe i(x p x p dx, where Ψ denotes a ground state of the Hamiltonian derived from L QE and T the time ordered product. In the perturbative quantum electrodynamics, Feynman diagrammatically, the e and e 4 terms of the effective mass is computed from the self-energy of electron, e.g., Figure : Electron self-energy Faculty of Mathematics, Kyushu University, Fukuoka 8-858, Japan. epartment of Math. and Phys., Setsunan University, , Osaka, Japan
2 and the effective charge from the self-energy of photon, e.g., Figure : Photon self-energy One can interpret the photon self-energy diagram as the emission of the pairs of virtual electrons and positrons. All these argument is successive from the physical point of view, but perturbative and implicit divergences are included.. Informal derivation of nonrelativistic quantum electrodynamics In this note we want to discuss the quantum electrodynamics nonperturbatically, but we assume that ( an electron is in low energy, ( we take the Coulomb gauge, (3 we introduce a form factor of an electron. ( implies that no emission of pairs of virtual electrons and positrons, i.e., there is no loop such as in Fig., then in our model the effective charge equals to the bare charge and the number of electrons is fixed. From ( the theory is not relatively covariant. From (3 it follows that the density of the electron charge is smoothly localised around the position of the electron and the ultraviolet divergence does not exist. Taking into account of (-(3, we modify the quantum electrodynamics as follows. Let E(t, x and B(t, x, (t, x R R 3, be an electric field and a magnetic field respectively, and q(t the position of an electron at time t R. The Maxwell equation with form factor is given by Ḃ = E, B =, Ė = B e( q(t q(t, E = e( q(t. Here Ẋ = dx/dt. Let (J(t, x, ρ(t, x = (e(x q(t q(t, e(x q(t. Then the Lagrangian density of the nonrelativistic quantum electrodynamics under consideration is given by L NRQE (t, x = m q(t + (E(t, x B(t, x + J(t, x A(t, x ρ(t, xφ(t, x, where A and φ are a vector potential and a scalar potential related to E and B such as E = Ȧ φ, B = A. Let L NRQE = L NRQE (t, xdx. Then the conjugate momenta are given p(t := L NRQE q = m q(t + e A(t, x(x q(tdx, Π(t, x := δl NRQE δȧ = Ȧ(t, x.
3 Then the Hamiltonian is given through the Legendre transformation as H NRQE = p(t q(t + Ȧ(t, xπ(t, xdx L NRQE = ( p(t e A(t, x(x q(tdx + V (q + {Ȧ(t, x + ( A(t, x } dx m where V is a smeared external potential given by V (q := (q y(q y e 4π y y dydy. In the next subsection we quantize H NRQE with spin / and total momentum p R 3, which is denoted by H(p and is called the Pauli-Fierz Hamiltonian, in the rigorous way from mathematical point of view..3 Non-relativistic quantum electrodynamics [ ] Let F be the boson Fock space given by F n s L (R 3 {, }, where n s denotes the n-fold symmetric tensor product with sl (R 3 {, } C. The Fock vacuum Ω F is defined by Ω {,,,..}. Let a(f be the creation operator and a (f the annihilation operator on F defined by n= (a (fψ (n+ n + S n+ (f Ψ (n, f L (R 3 {, }, and a(f = [a ( f], where S n denotes the symmetrizer. The scalar product on K is denoted by (f, g K which is linear in g and anti-linear in f. a and a satisfy canonical commutation relations: j=, [a(f, a (g] = ( f, g L (R 3 {,}, [a(f, a(g] =, [a (f, a (g] =. We write as a (k, jf(k, jdk for a (f with a formal kernel a (k, j. Let T be a selfadjoint operator on L (R 3. We define Γ(e itt a (f a (f n Ω a (e itt f a (e itt f n Ω. Thus Γ(e itt turns out to be a strongly continuous one-parameter unitary group in t, which implies that there exists a self-adjoint operator dγ(t on F such that Γ(e itt = e itdγ(t for t R. We define a Hilbert space H by H C F. The Pauli-Fierz Hamiltonian with total momentum p = (p, p, p 3 R 3 is given by a symmetric operator on H: H(p 3 σ m µ (p µ µ ea ˆµ + H f, µ= where m > and e R denote the mass and the charge( of an electron, respectively, ( i σ (σ, σ, σ 3 the Pauli-matrices given by σ, σ, i 3
4 ( σ 3, and the free Hamiltonian H f, the momentum operator and quantum radiation field A ˆµ are given by H f dγ(ω, µ dγ(k µ, A ˆµ ˆ(k e µ (k, j(a (k, j + a(k, jdk, µ =,, 3. ω(k j=, Here e(k, j, j =,, denotes polarization vectors such that e(k, j =, e(k, e(k, =, k e(k, j = and e(k, e(k, = k/ k. We omit the tensor notation in what follows. Then H(p = m (p ea ˆ + H f e m σb ˆ, p R 3, where B ˆµ denotes the quantum magnetic field given by B ˆµ i j=, ˆ(k ω(k (k e(k, j µ (a (k, j a(k, jdk. Note that [A ˆµ, B ˆν ] = for µ, ν =,, 3. The spectrum of H(p is stuided in e.g., [, ] and see references in [5]. Mass renormalization. Main theorems Let where T m (e, p (p ea ˆm + H f e σb ˆ m, p R 3,, k < κ/m, ˆ m (k ˆ(mk = / (π 3, κ/m k Λ/m,, k > Λ/m. ( It is established in [4] that T m (e, p is self-adjoint on ( (H f for arbitrary Λ >, m >, p R 3, e R. Since A ˆ = ma ˆm, B ˆ = mb ˆm, H f = mhf and = mpf, where X = Y denotes the unitary equivalence, we have H m (e, p = mt m (e, ( p /mn z, where n z = (,,. Let :X : be the Wick product of X. We define H(e, ɛ :T m (e, ɛn z :, ɛ R. Set E(e, ɛ inf σ(h(e, ɛ. It is established in [5] that there exist constants e > and ɛ > such that for (e, ɛ a {(e, ɛ R e < e, ɛ < ɛ }, ( the dimension of Ker(H(e, ɛ E(e, ɛ is two, ( E(e, ɛ is an analytic function of e and ɛ on a, (3 there exists a strongly analytic ground state of H(e, ɛ. The effective mass m eff is defined by m m eff = ɛ E(e, ɛ ɛ=. 4
5 From this it immediately follows that effective mass m eff is an analytic function of e on {e R 3 e < e } with some e >. Set m m eff = a n (Λ/me n. n= The effective mass is investigated in e.g., [3, 5, 6, 8]. It is known and easily derived that a (Λ/m = 8 3π Our next issue is to study a (Λ/m. 4π ( Λ/m κ/m r + dr + Λ/m κ/m r (r + 3 dr. a (Λ/m Theorem. There exist positive constants c < c such that c lim Λ (Λ/m c.. Expansions We set A A ˆm and B B ˆm. Let us define H, E and g by H H(e, = H + eh I + e H II, E E(e, = n= e n n! E (n, g g (e, = n= e n n! (n, where H H f +, H I H ( I + H ( I, H ( I = A, H ( I σb, and H II : AA := A + A + + A + A + A A. Here we put A + j=, ˆm (k e(k, ja (k, jdk, A ω(k We can see that E ( = E (n+ =, n =,,, 3,..., and j=, ˆm (k ω(k e(k, ja(k, jdk. ( E ( = ( (, H ( I ( H = ( (, σb ( σb H ( H. ( Note that E ( (Λ/m as Λ. Moreover ( ( = Ω, ( = ( σb H (, ( = ( H II H ( + ( A ( H H + {( σb ( H H (3 = 3 H ( H II H ( σb σb ( σb ( E } ( (, ( + 3 H ( A H ( H II ( 5
6 +6 ( A ( A ( σb H H H ( +6 ( A {( σb ( σb ( E } ( H H H ( +3 ( σb ( H II H ( + 6 ( σb ( A ( σb H H H H +6 ( σb {( σb ( σb ( E } ( H H H (. ( Although formula m m eff = 3 3 µ= (( + ea µ g, (H E ( + ea µ g H ( g, g H (3 is well known, it is not useful for our task, since expansion of (H E in e leads us to a complicated operator domain argument. Then, instead of (3, it is established in [6] that g s g (e, ɛ/ ɛ ɛ= satisfies that ( + ea 3 g ((H E with g = (H E ( + ea 3 g and H m = ( g, ( + ea 3 g. (4 m eff ( g, g H Using (4 in [5] it is proven that the effective mass is expanded as or where m m eff = 3 c (Λ/me 3 c (Λ/me 4 + O(e 6, (5 m eff m = + ( ( 3 c (Λ/me + 3 c (Λ/m + c (Λ/m e 4 + O(e 6, (6 3 Here 3 c (Λ/m (Ψ µ, H Ψ µ H, µ= 3 c (Λ/m µ= Ψ µ n { (Ψ µ, H Ψ µ H (Ψ µ, H Ψ µ H( (, ( H + R(Ψ µ, H Ψ µ H +(Ψ µ, H Ψ µ H + R(Ψ µ 3, H Ψ µ H (n! A µ (n + n! µ (n, n =,, 3, µ =,, 3, and H H, H H + H 3, H H 4 + H 5 + H 6 + H 7 + H 8, where we put H =, H = ( A, H 3 = ( σb, H H H H H }. (7 6
7 H 4 = ( H II, H 5 = ( A ( A, H H H H H H 6 = ( σb ( A, H 7 = H 6 = ( A ( σb H H H H H H 8 = {( σb ( σb ( E } (. H H H, H From above expressions of (, (, (3, it follows that for µ =,, 3, Ψ µ Φµ + Φµ, 6 Ψµ Φ µ i, Ψµ 3 6 Φ µ i, i= i=7 where Φ µ = A+ µ ( Φ µ = P f µ σb + H ( Φ µ 3 = A µ σb + H ( Φ µ 4 = P f µ A + A + H ( Φ µ 5 = P f µ ( A σb + H H ( Φ µ 6 = 4 P f µ σb + σb + H H ( Φ µ 7 = A µ A + A + H ( Φ µ 8 = A µ ( A σb + H H ( Φ µ 9 = 4 A µ σb + σb + H H ( Φ µ = 4 P f µ :AA: σb + H H ( Φ µ = P f µ ( A A + A + H H ( Φ µ = P f µ ( A ( A σb + H H H ( Φ µ 3 = 4 P f µ ( A σb + σb + H H H ( Φ µ 4 = 4 P f µ σb A + A + H H ( Φ µ 5 = 4 P f µ σb ( A σb + H H H ( Φ µ 6 = 8 P f µ σb σb + σb + H H H ( Substituting H,..., H 8 and Φ µ,..., Φµ 6 into (7, we see that { 3 8 c (Λ/m = ( Φ µ i, H l Φ µ i H + ( Φ µ i, H Φ µ i H µ= i= l=4 i= i= i= } ( Φ µ i, (H + H 3 Φ µ i H + ( Φ µ i, H Φ µ i 6 H +( Φ µ i, H Φ µ i H. (8 i=3 i= i=3 i=3 i=7 i= From (8 it follows that c (Λ/m is decomposed into 76 terms. Fortunately it is, however, enough to consider terms containing even number of σb s, since the terms with odd number of σb vanishes by a symmetry. See Fig
8 No. Term σb H Order ( (Φ µ, H Φ µ ( (, ( H [log(λ/m] ( (Φ µ, H Φ µ ( (, ( H 3 [log(λ/m] Figure 3: ( i= Φ µ i, H i= Φ µ i H No. Term σb H Order (3 (Φ µ 3, H Φ µ 3 3 [log(λ/m] (4 (Φ µ 5, H Φ µ 3 4 [log(λ/m] (5 (Φ µ 3, H Φ µ 5 4 [log(λ/m] (6 (Φ µ 4, H Φ µ Λ/m (7 (Φ µ 6, H Φ µ 4 4 Λ/m (8 (Φ µ 4, H Φ µ 6 4 Λ/m (9 (Φ µ 5, H Φ µ Λ/m ( (Φ µ 6, H Φ µ [log(λ/m] Figure 4: ( 6 i=3 Φ µ i, H 6i=3 Φ µ i H No. Term σb H Order ( (Φ µ, H 4Φ µ [log(λ/m] ( (Φ µ, H 4Φ µ 4 [log(λ/m] (3 (Φ µ, H 5Φ µ 3 log(λ/m (4 (Φ µ, H 5Φ µ 4 5 [log(λ/m] (5 (Φ µ, H 6Φ µ 4 [log(λ/m] (6 (Φ µ, H 6Φ µ 4 [log(λ/m] (7 (Φ µ, H 7Φ µ 4 [log(λ/m] (8 (Φ µ, H 7Φ µ 4 [log(λ/m] (9 (Φ µ, H 8Φ µ 3 [log(λ/m] ( (Φ µ, H 8Φ µ 4 5 [log(λ/m] Figure 5: ( i= Φ µ i, 8 l=4 H l i= Φ µ i H 8
9 No. Term σb H Order ( (Φ µ 4, H Φ µ 3 log(λ/m ( (Φ µ 6, H Φ µ 4 [log(λ/m] (3 (Φ µ 3, H Φ µ 4 [log(λ/m] (4 (Φ µ 5, H Φ µ 4 5 Λ/m (5 (Φ µ 3, H 3Φ µ 4 [log(λ/m] (6 (Φ µ 5, H 3Φ µ 4 [log(λ/m] (7 (Φ µ 4, H 3Φ µ 4 Λ/m (8 (Φ µ 6, H 3Φ µ 4 5 Λ/m Figure 6: ( 6 i=3 Φ µ i, (H + H 3 ( i= Φ µ i H No. Term σb H Order (9 (Φ µ 7, H Φ µ [log(λ/m] (3 (Φ µ 9, H Φ µ 3 [log(λ/m] (3 (Φ µ, H Φ µ 3 = (3 (Φ µ 3, H Φ µ 4 = (33 (Φ µ 5, H Φ µ 4 = (34 (Φ µ 8, H Φ µ 4 [log(λ/m] (35 (Φ µ, H Φ µ 4 Λ/m (36 (Φ µ, H Φ µ 4 5 [log(λ/m] (37 (Φ µ 4, H Φ µ 4 [log(λ/m] (38 (Φ µ 6, H Φ µ 4 5 (Λ/m Figure 7: ( 6 i=7 Φµ i, H i= Φ µ i H 9
10 .3 Feynman diagrams spin = σb + = σ(k, f = σ (k e(k, j, polarization = A µ = e µ (k, j, propagator( = (π 3 ω(k, propagator( = = H ω(k i + k i /, E i propagator(3 = = H ω(k + ω(k + k + k /, E propagator(4 = ( = ( H ω(k + k /, ( A + = k e(p, j, µ = k µ.. Figure 8: Items of diagrams The 38 terms in Fig. 3-7 can be represented by Feynman diagrams. The items of diagrams are in Fig. 8. Example. We compute (Φ µ 5, H Φ µ 5 as an example. Since (Φ µ 5, H Φ µ 5 = 4 (P f µ ( A + σb + H H (, H µ ( A + σb + H H (, its diagram is given as in Fig. 9. Figure 9: (Φ µ 5, H Φ µ 5.
11 Then (Φ µ 5, H Φ µ 5 = d 3 k d 3 k 4 4(π 6 ω ω σ (k e (k + k µ (k + k µ E E E E d 3 k d 3 k k + k = 4(π 6 ω ω E 3 ( σ σ (k e (k e E ( (k + k e σ + (k + k e σ E E + σ σ (k e (k e E E Here and in what follows we set e = e(k, j, e = ( e(k, j (, σ = σ(k, j, σ = σ(k, j and X denotes the expectation value of X: X = (, X C. The diagrams consists of three kinds of diagrams; AA type, Aσ type and σσ type. particular AA type corresponds to the spinless model discussed in [6]. In (Φ µ 4, H Φ µ 4 = O( Λ/m (Φ µ, H 4Φ µ = O([log(Λ/m] (Φ µ, H 5Φ µ = O(log Λ/m (Φ µ 4, H Φ µ = O(log Λ/m (Φ µ 7, H Φ µ = O([log(Λ/m] (Φ µ, H Φ µ = Figure : AA type Feynman diagrams
12 (Φ µ 3, H Φ µ 3 = O([log(Λ/m] (Φ µ 5, H Φ µ 3 = O([log(Λ/m] (Φ µ 3, H Φ µ 5 = O([log(Λ/m] (Φ µ 5, H Φ µ 5 = O( Λ/m (Φ µ, H 4Φ µ = O([log(Λ/m] (Φ µ, H 5Φ µ = O([log(Λ/m] (Φ µ, H 7Φ µ = O([log(Λ/m] (Φ µ, H 7Φ µ = O([log(Λ/m] (Φ µ, H 8Φ µ = O([log(Λ/m] Figure : Aσ type Feynman diagrams
13 (Φ µ 6, H Φ µ = O([log(Λ/m] (Φ µ 3, H Φ µ = O([log(Λ/m] (Φ µ 5, H Φ µ = O( Λ/m (Φ µ 3, H 3Φ µ = O([log(Λ/m] (Φ µ 5, H 3Φ µ = O([log(Λ/m] (Φ µ 4, H 3Φ µ = O( Λ/m (Φ µ 9, H Φ µ = O([log(Λ/m] (Φ µ 3, H Φ µ = (Φ µ 5, H Φ µ = Figure : Aσ type Feynman diagrams 3
14 (Φ µ 8, H Φ µ = O([log(Λ/m] (Φ µ, H Φ µ = O( Λ/m (Φ µ, H Φ µ = O([log(Λ/m] (Φ µ 4, H Φ µ = O([log(Λ/m] (Φ µ 6, H Φ µ 4 = O( Λ/m (Φ µ 4, H Φ µ 6 = O( Λ/m (Φ µ, H 6Φ µ = O([log(Λ/m] (Φ µ, H 6Φ µ = O([log(Λ/m] (Φ µ, H Φ µ = O([log(Λ/m] Figure 3: Aσ type Feynman diagrams 4
15 (Φ µ 6, H Φ µ 6 = O([log(Λ/m] (Φ µ, H Φ µ = O([log(Λ/m] (Φ µ 6, H 3Φ µ = O(Λ/m (Φ µ 6, H Φ µ = O((Λ/m (Φ µ, H 8Φ µ = O([log(Λ/m] Figure 4: σσ type Feynman diagrams.4 Proof of Theorem. We shall prove Theorem.. Note that the following formulas are useful. Lemma.3 It follows that e i e i =, i =,, (9 (e e (e e = + (ˆk ˆk, ( (k e (k e = k ( (ˆk ˆk, ( (k e (e e (e k = (k, k ( (ˆk ˆk, ( σ i σ i = k i, i =,, (3 R σ σ (e k (k e = k k ((ˆk ˆk, (4 5
16 Proof: Note that R σ σ (e e = k k (ˆk ˆk, (5 σ σ σ σ = 4 k k, (6 R σ σ σ σ = k k ( (ˆk ˆk. (7 e µ (k, je ν (k, j = (δ µν k µk ν k, (k e(k, j µe ν (k, j = ɛ µνα k α, R σ µ σ ν = δ µν. Here ɛ αβγ denotes the antisymmetric tensor with ɛ 3 = +. In what follows, the summation over repeated index is understood. We see that ( e i e i = e µ (k i, je µ (k i, j =, i =,, ( (e e (e e = e µ (k, je µ (k, j e ν (k, je ν (k, j = (δ µν k µk ν k (δ µν k µk ν k = (3 + (ˆk ˆk k k = + (ˆk ˆk, (3 (k e (k e = k µ e µ (k, jk ν e ν (k, j = k µ k ν (δ µν k µk ν k = k ( (ˆk ˆk, (4 (k e (e e (e k = k µ e µ (k, je λ (k, je λ (k, j k ν e ν (k, j = k µ (δ µλ k µk λ k k ν(δ λν k λk ν k = (k, k ( (ˆk ˆk, (5 R σ σ = R σ µ σ ν (k e(k, j µ (k e(k, j ν = δ µν (k e(k, j µ (k e(k, j ν = (k e(k, j µ (k e(k, j µ = k ( e(k, + e(k, = k, (6 R σ σ (e k (k e = R σ µ σ ν (k e(k, j µ (k e(k, j ν e α (k, jk α e β (k, j k β = (k e(k, j µ (k e(k, j µ e α (k, jk α e β (k, j k β = ( ɛ µαγ k γ ( ɛ µβδ k δ k α k β = k k = k k ( (ˆk ˆk, (7 R σ σ (e e = R σ µ σ ν (k e(k, j µ (k e(k, j ν e α (k, je α (k, j = ( ɛ µαβ k β ( ɛ µαγ k γ = (k k, (8 σ σ σ σ = σ σ µ σ ν σ (k e(k, j µ (k e(k, j ν = σ σ (k e(k, j µ (k e(k, j µ = (k e(k, j (k e(k, j = k k = 4 k k, (9 R σ σ σ σ = σ σ σ σ + (k e(k, j µ (k e(k, j µ R σ σ = 4 k k + (k e(k, j µ (k e(k, j µ (k e(k, j ν (k e(k, j ν = 4 k k + (δ µν k µk ν k (δ µν k µk ν k = 4 k k + k k ( + (ˆk ˆk = k k ( (ˆk ˆk. Using the diagrams presented in Fig.-4 and (9-(7, we can easily expressed 38 terms as integrals on = {(k, k R 3 R 3 κ/m k Λ/m, κ/m k Λ/m}. 6
17 Note that imaginary part of σ a σ b does not contribute integrals. We show the results:. (Φ µ, H Φ µ ( (, ( = 4 (A+ µ (, A + µ H ( ( σb + H (, σb + H ( = d 3 k d 3 k 4 4(π 6 e e σ σ ω ω E E E = d 3 k d 3 k 4 k 4 4(π 6 ω ω E E. (Φ µ, H Φ µ ( (, ( = 4 (P f µ σb + H (, H µ σb + H ( ( σb + H (, σb + H ( = d 3 k d 3 k 4 4(π 6 k σ σ σ σ ω ω E E E E E = d 3 k d 3 k 4 k 4 k 4 4(π 6 ω ω E 3 E 3. (Φ µ 3, H Φ µ 3 = 4 (A+ µ = 4 = 4 H σb + (, H A + µ H σb + ( d 3 k d 3 k 4(π 6 ( σ σ (e e + σ σ (e e ω ω E E E E d 3 k d 3 k 4(π 6 ( 4 k + k k (ˆk ˆk ω ω E E E E 4. (Φ µ 5, H Φ µ 3 = 4 (P f µ ( A + σb + H H (, = d 3 k d 3 k 4 4(π 6 ω ω E = d 3 k d 3 k 4 4(π 6 ω ω E H A + µ H σb + ( E ((k e (k e σ σ E + (k e (k e σ σ E ( k 4 ( (ˆk ˆk + k k ( (ˆk ˆk E E E 5. (Φ µ 3, H Φ µ 5 = (Φµ 5, H Φ µ 3 7
18 6. 7. (Φ µ 4, H Φ µ 4 = [6, (3.3] = 4 (P f µ (A + A + H (, H µ (A + A + H ( = d 3 k d 3 k 4 4(π 6 ω ω E 3 k + k (e e (e e + e e = d 3 k d 3 k 4 4(π 6 k + k ( + (ˆk ˆk ω ω E 3 (Φ µ 6, H Φ µ 4 = 8 (P f µ σb + σb + H H (, H µ (A + A + H ( = d 3 k d 3 k 8 4(π 6 ω ω E 3 k + k ( σ σ e e + σ σ e e E E = d 3 k d 3 k 8 4(π 6 k + k k k (ˆk ˆk ( + ω ω E E E 3 8. (Φ µ 4, H Φ µ 6 = (Φµ 6, H Φ µ (Φ µ 5, H Φ µ 5 = 4 (P f µ ( A + σb + H H (, = d 3 k d 3 k 4 4(π 6 ω ω E 3 = d 3 k d 3 k 4 4(π 6 ω ω E 3 H µ ( A + σb + H H ( k + k (k e ((k e σ σ + (k e σ σ E E E k + k ( k 4 ( (ˆk ˆk + k k ( (ˆk ˆk E E E (Φ µ 6, H Φ µ 6 = E = 6 (P f µ σb + σb + H H (, = d 3 k d 3 k 6 4(π 6 ω ω E 3 = d 3 k d 3 k 6 4(π 6 ω ω E 3 H µ σb + σb + H H ( E k + k ( σ σ σ σ E + σ σ σ σ E k + k ( 4 k k + k k ( (ˆk ˆk E E E (Φ µ, H 4Φ µ = [6, (3.34] = (A ν = = d 3 k d 3 k 4(π 6 (e e (e e ω ω E E d 3 k d 3 k 4(π 6 ( + (ˆk ˆk ω ω E E H A + µ (, A ν H A + µ ( 8
19 (Φ µ, H 4Φ µ = 8 (P f µ σb + H (, (A + A + + A + A + A A H H µ σb + H ( = 4 (A ν H µ σb + H (, A ν H µ σb + H ( = d 3 k d 3 k 4 4(π 6 σ σ (k k (e e ω ω E E E E = d 3 k d 3 k k k (ˆk ˆk 4 4(π 6 ω ω E E (Φ µ, H 5Φ µ = [6, (3.36] = (A+ µ (, = = H ( A + H ( A + H A + µ ( d 3 k d 3 k 4(π 6 (k e ((k e (e e + (k e (e e ω ω E E E E d 3 k d 3 k 4(π 6 ( k ( (ˆk ˆk + (k k ( (ˆk ˆk ω ω E E E E (Φ µ, H 5Φ µ = 4 ( ( A + H H µ σb + H (, ( A + H µ σb + H ( = d 3 k d 3 k 4 4(π 6 ω ω E E (k e ((k e k σ σ E + (k e (k k σ σ E = d 3 k d 3 k 4 4(π 6 ω ω E E ( k 6 ( (ˆk ˆk E + (k k ( k k ( (ˆk ˆk E (Φ µ, H 6Φ µ = 4 ( σb H H µ σb + H (, ( A + A + µ H ( = d 3 k d 3 k 4 4(π 6 (k e ((k e σ σ + (k e σ σ ω ω E E E E E E = d 3 k d 3 k k k ( (ˆk ˆk 4 4(π 6 ω ω E E E (Φ µ, H 6Φ µ = 4 (σb+ A + µ H (, ( A + H H µ σb + H ( = d 3 k d 3 k 4 4(π 6 ((k e (k e σ σ + (k e (k e σ σ ω ω E E E E E = d 3 k d 3 k k 4 ( (ˆk ˆk 4 4(π 6 ω ω E E E 9
20 (Φ µ, H 7Φ µ = 4 ( ( A + H H µ σb + H (, σb + A + µ H ( = d 3 k d 3 k 4 4(π 6 ((k e (k e σ σ + (k e (k e σ σ ω ω E E E E E E = d 3 k d 3 k k 4 ( (ˆk ˆk 4 4(π 6 ω ω E E E (Φ µ, H 7Φ µ = 4 (σb+ ( A + A + µ H H (, H µ σb + H ( = d 3 k d 3 k 4 4(π 6 σ σ ((k e (k e + (k e (k e ω ω E E E E E = d 3 k d 3 k k k ( (ˆk ˆk 4 4(π 6 ω ω E E E (Φ µ, H 8Φ µ = E = 4 (σb+ H A + µ (, 4 (σb+ (, H σb + ( (A + µ (, E H σb + H A + µ ( A + µ H H ( = d 3 k d 3 k 4 4(π 6 ((e e σ σ + (e e σ σ ω ω E E E E d 3 k d 3 k 4 4(π 6 σ σ (e e ω ω E E E = d 3 k d 3 k 4 4(π 6 ( 4 k + k k (ˆk ˆk d 3 k d 3 k ω ω E E E 4 4(π 6 4 k ω ω E (Φ µ, H 8Φ µ = E 3 = 6 (σb+ H µ σb + H (, σb + H H µ σb + H ( 6 (σb+ (, σb + H ( (σb + (, H H µ H µ σb + H ( = d 3 k d 3 k 6 4(π 6 ω ω E E d 3 k d 3 k 6 4(π 6 k σ σ σ σ ω ω E E E E E = d 3 k d 3 k 6 4(π 6 ω ω E E ( 4 k k 4 E d 3 k d 3 k 6 4(π 6 4 k k 4 ω ω E E 4 E ( σ σ σ σ k E E + (k k σ σ σ σ E E + (k k ( k k ( (ˆk ˆk E
21 . (Φ µ 4, H Φ µ = [6, (3.33] = (P f µ A + A + H (, ( A + A + µ H H ( = d 3 k d 3 k 4(π 6 ω ω E (k e (k e ((e e + (e e E = d 3 k d 3 k 4(π 6 ( (k k ( (ˆk ˆk ω ω E E. (Φ µ 6, H Φ µ = 4 (P f µ σb + σb + H H (, = d 3 k d 3 k 4 4(π 6 ω ω E = d 3 k d 3 k 4 4(π 6 ω ω E H ( A + H A + µ ( E ((k e (k e σ σ E + (k e (k e σ σ E E ( k k ( (ˆk ˆk ( E + E 3. (Φ µ 3, H Φ µ = 4 (A+ µ σb + H (, ( A + H H µ σb + H ( = d 3 k d 3 k 4 4(π 6 ω ω E E ((k e (k e σ σ + (k e (k e σ σ E E = d 3 k d 3 k 4 4(π 6 k 4 ( (ˆk ˆk ω ω E E 3 4. (Φ µ 5, H Φ µ = 4 (P f µ ( A + σb + H H (, = d 3 k d 3 k 4 4(π 6 ω ω E = d 3 k d 3 k 4 4(π 6 ω ω E E ( A + H H µ σb + H ( (k e (k + k k ((k e σ σ + (k e σ σ E E E E k (k + k ( k 4 ( (ˆk ˆk E + k k ( (ˆk ˆk E 5. (Φ µ 3, H 3Φ µ = 4 (A+ µ σb + H (, σb + A + µ H H ( = d 3 k d 3 k 4 4(π 6 ( σ σ (e e + σ σ (e e ω ω E E E E = 4 d 3 k d 3 k 4(π 6 ω ω E ( k k (ˆk ˆk + 4 k E E E
22 6. (Φ µ 5, H 3Φ µ = 4 (P f µ ( A + σb + H H (, = d 3 k d 3 k 4 4(π 6 ω ω E = d 3 k d 3 k 4 4(π 6 ω ω E σb + A + µ H H ( (k e ( σ σ (k e + σ σ (k e E E E ( k k ( (ˆk ˆk + k 4 ( (ˆk ˆk E E E 7. (Φ µ 4, H 3Φ µ = 8 (P f µ A + A + H (, σb H H µ σb + H ( = d 3 k d 3 k 8 4(π 6 ω ω E σ σ (k + k k (e e + e e E E = d 3 k d 3 k 8 4(π 6 4k (k + k k k (ˆk ˆk ω ω E E 8. (Φ µ 6, H 3Φ µ = 6 (P f µ σb + σb + H H (, = d 3 k d 3 k 6 4(π 6 ω ω E = d 3 k d 3 k 6 4(π 6 (k + k k ( 4 k k ω ω σb H H µ σb + H ( (k + k k ( σ σ σ σ + σ σ σ σ E E E E E E E + k k ( (ˆk ˆk E 9. (Φ µ 7, H Φ µ = [6, (3.3] = ( H A + A + (, A + µ = = d 3 k d 3 k 4(π 6 (e e ((e e + (e e ω ω d 3 k d 3 k 4(π 6 ( + (ˆk ˆk ω ω E E H A + µ ( 3. (Φ µ 9, H Φ µ = 4 ( σb + σb + H H (, A + µ A + µ H ( = d 3 k d 3 k 4 4(π 6 (e e ( σ σ + σ σ ω ω E E E E = d 3 k d 3 k 4 4(π 6 k k (ˆk ˆk ( + ω ω E E E E
23 (Φ µ, H Φ µ = [6, RHS of(3.3] = ( A + A + H (, ( A + H µ A + µ H ( = d 3 k d 3 k 4(π 6 (e k (e k (e e + e e = ω ω E E E (Φ µ 3, H Φ µ = 4 (P f µ ( A + σb + σb + H H H (, A + µ H ( = d 3 k d 3 k 4 4(π 6 (e k (k e ( σ σ + σ σ = ω ω E E E E E (Φ µ 5, H Φ µ = 4 (P f µ σb + ( A + σb + H H H (, A + µ H ( d 3 k d 3 k = 4(π 6 (e k ((k e σ σ + (k e σ σ = ω ω E E E E E (Φ µ 8, H Φ µ = 4 ( ( A + σb + H H (, A + µ H µ σb + H ( = d 3 k d 3 k 4 4(π 6 (k e ((k e σ σ + (k e σ σ ω ω E E E E E = d 3 k d 3 k 4 4(π 6 ( k 4 ( (ˆk ˆk + k k ( (ˆk ˆk ω ω E E E E (Φ µ, H Φ µ = 8 (P f µ A + A σb + H H (, H µ σb + H ( = 4 (A µ σb + H (, A µ H ν H ν σb + H ( = d 3 k d 3 k 4 4(π 6 k σ σ (e e ω ω E E E E = d 3 k d 3 k 4 4(π 6 k k 3 (ˆk ˆk ω ω E E 3 (Φ µ, H Φ µ = 4 ( ( A + σb + H H (, ( A + H µ H µ σb + H ( = d 3 k d 3 k 4 4(π 6 (k e k ((k e σ σ + (k e σ σ ω ω E E E E E E = d 3 k d 3 k 4 4(π 6 k ( k 4 ( (ˆk ˆk + k k ( (ˆk ˆk ω ω E E E E 3 3
24 (Φ µ 4, H Φ µ = 8 ( A + A + H (, σb + H µ H µ σb + H ( = d 3 k d 3 k 8 4(π 6 k σ σ (e e + e e ω ω E E E E = d 3 k d 3 k 4 k k 3 (ˆk ˆk 8 4(π 6 ω ω E E 3 (Φ µ 6, H Φ µ = E 4 = 6 ( σb + σb + H H (, σb + H µ H µ σb + H ( = d 3 k d 3 k 6 4(π 6 k ( σ σ σ σ + σ σ σ σ ω ω E E E E E E = d 3 k d 3 k 6 4(π 6 k ( k k ( (ˆk ˆk + 4 k k ω ω E E E E 3 As is seen above, integrands in each terms are functions of k, k, (ˆk ˆk. Changing variables k, k, (ˆk ˆk to r, r, X = cos θ, θ < π, respectively, it is seen that We see that F (Λ/m = d d(λ/m F (Λ/m = = π (π 6 d 3 k d 3 k 4(π 6 f( k, k, (ˆk ˆk ω ω dx Λ/m κ/m Λ/m dr dr r r f(r, r, X. κ/m π Λ/m (π 6 dx drr(λ/m[f(λ/m, r, X + f(r, Λ/m, X]. (8 κ/m To see the asymptotic behavior of F (Λ/m, we estimate the right hand side of (8. Then we can see that (Φ µ i lim, H jφ µ k <, µ =,, 3, Λ Λ/m where (i, j, k (, 8,, (, 8,, (6,,. In the case of (i, j, k = (, 8,, (, 8,, each term is divided into two integrals. Although each integral diverges as (Λ/m as Λ, cancelation happens. See Fig. 5 and 6. Then the terms (i, j, k = (, 8,, (, 8, diverge as [log(λ/m]. Finally we can directly see that the term (Φ µ 6, H Φ µ diverges as (Λ/m. Then the proof is complete. 4
25 Remark.4 Informally we can see that the diagram behaves as (Λ/m. Figure 5: (Φ µ, H 8Φ µ Figure 6: (Φ µ, H 8Φ µ Figure 7: (Φ µ 6, H Φ µ Terms (Φ µ, H 8Φ µ, (Φµ, H 8Φ µ and (Φµ 6, H Φ µ include diagram. Although, as is seen in Fig. 5, 6 and 7, (Φ µ, H 8Φ µ and (Φµ, H 8Φ µ have counter terms, (Φµ 6, H Φ µ does not. 5
26 Acknowledgements. We thank Tetsuya Hattori and Takashi Hara for helpful comments. K. R. I. thanks Grant-in-Aid for Science Research (C 554 from MEXT and F. H. thanks Grant-in-Aid for Science Research (C 5549 from MEXT. References [] T. Chen, Operator-theoretic infrared renormalization and construction of dressed -particle states in non-relativistic QE, mp-arc -3, preprint,. [] J. Fröhlich, Existence of dressed one electron states in a class of persistent models, Fortschritte der Physik (974, [3] C. Hainzl and R. Seiringer, Mass renormalization and energy level shift in non-relativistic QE, Adv. Theor. Math. Phys. 6 (, [4] F. Hiroshima, Fiber Hamiltonians in nonrelativistic quantum electrodynamics, in preparation. [5] F. Hiroshima and K. R. Ito, Mass renormalization in non-relativistic quantum electrodynamics with spin /, mp-arc 4-46, preprint 4. [6] F. Hiroshima and H. Spohn, Mass renormalization in nonrelativistic QE, J. Math. Phys. 46 (5 43. [7] E. Lieb and M. Loss, A bound on binding energies and mass renormalization in models of quantum electrodynamics, J. Stat. Phys. 8, ( [8] H. Spohn, Effective mass of the polaron: A functional integral approach, Ann. Phys. 75 (987,
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
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
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,
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
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
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
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
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
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
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
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 +
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
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
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
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
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
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
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
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
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
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
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
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 :
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
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
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
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
Problem Set 3: Solutions
CMPSCI 69GG Applied Information Theory Fall 006 Problem Set 3: Solutions. [Cover and Thomas 7.] a Define the following notation, C I p xx; Y max X; Y C I p xx; Ỹ max I X; Ỹ We would like to show that C
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
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
Fourier Series. MATH 211, Calculus II. J. Robert Buchanan. Spring Department of Mathematics
Fourier Series MATH 211, Calculus II J. Robert Buchanan Department of Mathematics Spring 2018 Introduction Not all functions can be represented by Taylor series. f (k) (c) A Taylor series f (x) = (x c)
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
Solution Series 9. i=1 x i and i=1 x i.
Lecturer: Prof. Dr. Mete SONER Coordinator: Yilin WANG Solution Series 9 Q1. Let α, β >, the p.d.f. of a beta distribution with parameters α and β is { Γ(α+β) Γ(α)Γ(β) f(x α, β) xα 1 (1 x) β 1 for < x
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
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.
Fractional Colorings and Zykov Products of graphs
Fractional Colorings and Zykov Products of graphs Who? Nichole Schimanski When? July 27, 2011 Graphs A graph, G, consists of a vertex set, V (G), and an edge set, E(G). V (G) is any finite set E(G) is
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
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
Srednicki Chapter 55
Srednicki Chapter 55 QFT Problems & Solutions A. George August 3, 03 Srednicki 55.. Use equations 55.3-55.0 and A i, A j ] = Π i, Π j ] = 0 (at equal times) to verify equations 55.-55.3. This is our third
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
Commutative Monoids in Intuitionistic Fuzzy Sets
Commutative Monoids in Intuitionistic Fuzzy Sets S K Mala #1, Dr. MM Shanmugapriya *2 1 PhD Scholar in Mathematics, Karpagam University, Coimbatore, Tamilnadu- 641021 Assistant Professor of Mathematics,
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
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
Solutions to Exercise Sheet 5
Solutions to Eercise Sheet 5 jacques@ucsd.edu. Let X and Y be random variables with joint pdf f(, y) = 3y( + y) where and y. Determine each of the following probabilities. Solutions. a. P (X ). b. P (X
6.3 Forecasting ARMA processes
122 CHAPTER 6. ARMA MODELS 6.3 Forecasting ARMA processes The purpose of forecasting is to predict future values of a TS based on the data collected to the present. In this section we will discuss a linear
Uniform Convergence of Fourier Series Michael Taylor
Uniform Convergence of Fourier Series Michael Taylor Given f L 1 T 1 ), we consider the partial sums of the Fourier series of f: N 1) S N fθ) = ˆfk)e ikθ. k= N A calculation gives the Dirichlet formula
DiracDelta. Notations. Primary definition. Specific values. General characteristics. Traditional name. Traditional notation
DiracDelta Notations Traditional name Dirac delta function Traditional notation x Mathematica StandardForm notation DiracDeltax Primary definition 4.03.02.000.0 x Π lim ε ; x ε0 x 2 2 ε Specific values
Derivation of Optical-Bloch Equations
Appendix C Derivation of Optical-Bloch Equations In this appendix the optical-bloch equations that give the populations and coherences for an idealized three-level Λ system, Fig. 3. on page 47, will be
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
2. Let H 1 and H 2 be Hilbert spaces and let T : H 1 H 2 be a bounded linear operator. Prove that [T (H 1 )] = N (T ). (6p)
Uppsala Universitet Matematiska Institutionen Andreas Strömbergsson Prov i matematik Funktionalanalys Kurs: F3B, F4Sy, NVP 2005-03-08 Skrivtid: 9 14 Tillåtna hjälpmedel: Manuella skrivdon, Kreyszigs bok
b. Use the parametrization from (a) to compute the area of S a as S a ds. Be sure to substitute for ds!
MTH U341 urface Integrals, tokes theorem, the divergence theorem To be turned in Wed., Dec. 1. 1. Let be the sphere of radius a, x 2 + y 2 + z 2 a 2. a. Use spherical coordinates (with ρ a) to parametrize.
Non analyticity of the ground state energy of the Hamiltonian for Hydrogen atom in nonrelativistic QED
Non analyticity of the ground state energy of the Hamiltonian for Hydrogen atom in nonrelativistic QED Jean-Marie Barbaroux, Semjon Vugalter To cite this version: Jean-Marie Barbaroux, Semjon Vugalter.
Math 446 Homework 3 Solutions. (1). (i): Reverse triangle inequality for metrics: Let (X, d) be a metric space and let x, y, z X.
Math 446 Homework 3 Solutions. (1). (i): Reverse triangle inequalit for metrics: Let (X, d) be a metric space and let x,, z X. Prove that d(x, z) d(, z) d(x, ). (ii): Reverse triangle inequalit for norms:
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:
= {{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
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
g-selberg integrals MV Conjecture An A 2 Selberg integral Summary Long Live the King Ole Warnaar Department of Mathematics Long Live the King
Ole Warnaar Department of Mathematics g-selberg integrals The Selberg integral corresponds to the following k-dimensional generalisation of the beta integral: D Here and k t α 1 i (1 t i ) β 1 1 i
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
ORDINAL ARITHMETIC JULIAN J. SCHLÖDER
ORDINAL ARITHMETIC JULIAN J. SCHLÖDER Abstract. We define ordinal arithmetic and show laws of Left- Monotonicity, Associativity, Distributivity, some minor related properties and the Cantor Normal Form.
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)
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
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
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
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
Chapter 3: Ordinal Numbers
Chapter 3: Ordinal Numbers There are two kinds of number.. Ordinal numbers (0th), st, 2nd, 3rd, 4th, 5th,..., ω, ω +,... ω2, ω2+,... ω 2... answers to the question What position is... in a sequence? What
Nowhere-zero flows Let be a digraph, Abelian group. A Γ-circulation in is a mapping : such that, where, and : tail in X, head in
Nowhere-zero flows Let be a digraph, Abelian group. A Γ-circulation in is a mapping : such that, where, and : tail in X, head in : tail in X, head in A nowhere-zero Γ-flow is a Γ-circulation such that
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 = =
Lecture 2. Soundness and completeness of propositional logic
Lecture 2 Soundness and completeness of propositional logic February 9, 2004 1 Overview Review of natural deduction. Soundness and completeness. Semantics of propositional formulas. Soundness proof. Completeness
General 2 2 PT -Symmetric Matrices and Jordan Blocks 1
General 2 2 PT -Symmetric Matrices and Jordan Blocks 1 Qing-hai Wang National University of Singapore Quantum Physics with Non-Hermitian Operators Max-Planck-Institut für Physik komplexer Systeme Dresden,
The semiclassical Garding inequality
The semiclassical Garding inequality We give a proof of the semiclassical Garding inequality (Theorem 4.1 using as the only black box the Calderon-Vaillancourt Theorem. 1 Anti-Wick quantization For (q,
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
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) =
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
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
12. Radon-Nikodym Theorem
Tutorial 12: Radon-Nikodym Theorem 1 12. Radon-Nikodym Theorem In the following, (Ω, F) is an arbitrary measurable space. Definition 96 Let μ and ν be two (possibly complex) measures on (Ω, F). We say
Lecture 13 - Root Space Decomposition II
Lecture 13 - Root Space Decomposition II October 18, 2012 1 Review First let us recall the situation. Let g be a simple algebra, with maximal toral subalgebra h (which we are calling a CSA, or Cartan Subalgebra).
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
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
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)
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
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)
Inverse trigonometric functions & General Solution of Trigonometric Equations. ------------------ ----------------------------- -----------------
Inverse trigonometric functions & General Solution of Trigonometric Equations. 1. Sin ( ) = a) b) c) d) Ans b. Solution : Method 1. Ans a: 17 > 1 a) is rejected. w.k.t Sin ( sin ) = d is rejected. If sin
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
Mean-Variance Analysis
Mean-Variance Analysis Jan Schneider McCombs School of Business University of Texas at Austin Jan Schneider Mean-Variance Analysis Beta Representation of the Risk Premium risk premium E t [Rt t+τ ] R1
Arithmetical applications of lagrangian interpolation. Tanguy Rivoal. Institut Fourier CNRS and Université de Grenoble 1
Arithmetical applications of lagrangian interpolation Tanguy Rivoal Institut Fourier CNRS and Université de Grenoble Conference Diophantine and Analytic Problems in Number Theory, The 00th anniversary
Optimal Parameter in Hermitian and Skew-Hermitian Splitting Method for Certain Two-by-Two Block Matrices
Optimal Parameter in Hermitian and Skew-Hermitian Splitting Method for Certain Two-by-Two Block Matrices Chi-Kwong Li Department of Mathematics The College of William and Mary Williamsburg, Virginia 23187-8795
6. MAXIMUM LIKELIHOOD ESTIMATION
6 MAXIMUM LIKELIHOOD ESIMAION [1] Maximum Likelihood Estimator (1) Cases in which θ (unknown parameter) is scalar Notational Clarification: From now on, we denote the true value of θ as θ o hen, view θ
Practice Exam 2. Conceptual Questions. 1. State a Basic identity and then verify it. (a) Identity: Solution: One identity is csc(θ) = 1
Conceptual Questions. State a Basic identity and then verify it. a) Identity: Solution: One identity is cscθ) = sinθ) Practice Exam b) Verification: Solution: Given the point of intersection x, y) of the
SOLUTIONS TO MATH38181 EXTREME VALUES AND FINANCIAL RISK EXAM
SOLUTIONS TO MATH38181 EXTREME VALUES AND FINANCIAL RISK EXAM Solutions to Question 1 a) The cumulative distribution function of T conditional on N n is Pr T t N n) Pr max X 1,..., X N ) t N n) Pr max
DIRECT PRODUCT AND WREATH PRODUCT OF TRANSFORMATION SEMIGROUPS
GANIT J. Bangladesh Math. oc. IN 606-694) 0) -7 DIRECT PRODUCT AND WREATH PRODUCT OF TRANFORMATION EMIGROUP ubrata Majumdar, * Kalyan Kumar Dey and Mohd. Altab Hossain Department of Mathematics University
Homomorphism in Intuitionistic Fuzzy Automata
International Journal of Fuzzy Mathematics Systems. ISSN 2248-9940 Volume 3, Number 1 (2013), pp. 39-45 Research India Publications http://www.ripublication.com/ijfms.htm Homomorphism in Intuitionistic
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
CHAPTER 101 FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD
CHAPTER FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD EXERCISE 36 Page 66. Determine the Fourier series for the periodic function: f(x), when x +, when x which is periodic outside this rge of period.
Lecture 34 Bootstrap confidence intervals
Lecture 34 Bootstrap confidence intervals Confidence Intervals θ: an unknown parameter of interest We want to find limits θ and θ such that Gt = P nˆθ θ t If G 1 1 α is known, then P θ θ = P θ θ = 1 α
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
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
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,...,
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
Section 7.6 Double and Half Angle Formulas
09 Section 7. Double and Half Angle Fmulas To derive the double-angles fmulas, we will use the sum of two angles fmulas that we developed in the last section. We will let α θ and β θ: cos(θ) cos(θ + θ)
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