Effective mass of nonrelativistic quantum electrodynamics

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

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

2 Composition. Invertible Mappings

Ordinal Arithmetic: Addition, Multiplication, Exponentiation and Limit

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

Space-Time Symmetries

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

Math221: HW# 1 solutions

Example Sheet 3 Solutions

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

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.

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

derivation of the Laplacian from rectangular to spherical coordinates

4.6 Autoregressive Moving Average Model ARMA(1,1)

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

Jesse Maassen and Mark Lundstrom Purdue University November 25, 2013

C.S. 430 Assignment 6, Sample Solutions

Congruence Classes of Invertible Matrices of Order 3 over F 2

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

Symmetric Stress-Energy Tensor

Areas and Lengths in Polar Coordinates

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

Other Test Constructions: Likelihood Ratio & Bayes Tests

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)

EE512: Error Control Coding

Reminders: linear functions

Statistical Inference I Locally most powerful tests

Problem Set 3: Solutions

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

Parametrized Surfaces

Fourier Series. MATH 211, Calculus II. J. Robert Buchanan. Spring Department of Mathematics

Areas and Lengths in Polar Coordinates

Solution Series 9. i=1 x i and i=1 x i.

Second Order Partial Differential Equations

Section 8.3 Trigonometric Equations

Fractional Colorings and Zykov Products of graphs

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

A Note on Intuitionistic Fuzzy. Equivalence Relation

Srednicki Chapter 55

Matrices and Determinants

Commutative Monoids in Intuitionistic Fuzzy Sets

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

ST5224: Advanced Statistical Theory II

Solutions to Exercise Sheet 5

6.3 Forecasting ARMA processes

Uniform Convergence of Fourier Series Michael Taylor

DiracDelta. Notations. Primary definition. Specific values. General characteristics. Traditional name. Traditional notation

Derivation of Optical-Bloch Equations

8.324 Relativistic Quantum Field Theory II

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)

b. Use the parametrization from (a) to compute the area of S a as S a ds. Be sure to substitute for ds!

Non analyticity of the ground state energy of the Hamiltonian for Hydrogen atom in nonrelativistic QED

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.

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

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

Relativistic particle dynamics and deformed symmetry

g-selberg integrals MV Conjecture An A 2 Selberg integral Summary Long Live the King Ole Warnaar Department of Mathematics Long Live the King

Finite Field Problems: Solutions

ORDINAL ARITHMETIC JULIAN J. SCHLÖDER

Higher Derivative Gravity Theories

Homework 3 Solutions

5. Choice under Uncertainty

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

On the Galois Group of Linear Difference-Differential Equations

Chapter 3: Ordinal Numbers

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

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

Lecture 2. Soundness and completeness of propositional logic

General 2 2 PT -Symmetric Matrices and Jordan Blocks 1

The semiclassical Garding inequality

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

CHAPTER 25 SOLVING EQUATIONS BY ITERATIVE METHODS

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

1 String with massive end-points

12. Radon-Nikodym Theorem

Lecture 13 - Root Space Decomposition II

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

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

Concrete Mathematics Exercises from 30 September 2016

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

SCHOOL OF MATHEMATICAL SCIENCES G11LMA Linear Mathematics Examination Solutions

Inverse trigonometric functions & General Solution of Trigonometric Equations

DESIGN OF MACHINERY SOLUTION MANUAL h in h 4 0.

Mean-Variance Analysis

Arithmetical applications of lagrangian interpolation. Tanguy Rivoal. Institut Fourier CNRS and Université de Grenoble 1

Optimal Parameter in Hermitian and Skew-Hermitian Splitting Method for Certain Two-by-Two Block Matrices

6. MAXIMUM LIKELIHOOD ESTIMATION

Practice Exam 2. Conceptual Questions. 1. State a Basic identity and then verify it. (a) Identity: Solution: One identity is csc(θ) = 1

SOLUTIONS TO MATH38181 EXTREME VALUES AND FINANCIAL RISK EXAM

DIRECT PRODUCT AND WREATH PRODUCT OF TRANSFORMATION SEMIGROUPS

Homomorphism in Intuitionistic Fuzzy Automata

On a four-dimensional hyperbolic manifold with finite volume

CHAPTER 101 FOURIER SERIES FOR PERIODIC FUNCTIONS OF PERIOD

Lecture 34 Bootstrap confidence intervals

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

상대론적고에너지중이온충돌에서 제트입자와관련된제동복사 박가영 인하대학교 윤진희교수님, 권민정교수님

Tridiagonal matrices. Gérard MEURANT. October, 2008

Section 9.2 Polar Equations and Graphs

Section 7.6 Double and Half Angle Formulas

The Simply Typed Lambda Calculus

Transcript:

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, 57-858, Osaka, Japan

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.

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

( 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

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 ( 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

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= } 6 6 6 ( 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. 3-7. 7

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 4 3 + 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 5 4 5 + Λ/m ( (Φ µ 6, H Φ µ 6 4 5 [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

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

.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.

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

(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

(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

(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

(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

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

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

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 4 9... (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

. 3. 4. 5. 6. (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

7. 8. 9.. (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

. (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

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

3. 3. 33. 34. 35. 36. (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

37. 38. (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

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

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, 59 98. [3] C. Hainzl and R. Seiringer, Mass renormalization and energy level shift in non-relativistic QE, Adv. Theor. Math. Phys. 6 (, 847-87. [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, ( 57 69. [8] H. Spohn, Effective mass of the polaron: A functional integral approach, Ann. Phys. 75 (987, 78 38. 6