Instantaneous Bethe Salpeter Equation and Its Exact Solution

Size: px
Start display at page:

Download "Instantaneous Bethe Salpeter Equation and Its Exact Solution"

Transcription

1 Commun. Theor. hys. Beijing, China pp c International Academic ublishers Vol. 43, No. 1, January 15, 2005 Instantaneous Bethe Salpeter Equation and Its Exact Solution CHANG Chao-Hsi, 1,2 CHEN Jiao-Kai, 2,3 LI Xue-Qian, 1,4 and WANG Guo-Li 4,5 1 CCAST World Laboratory,.O. Box 8730, Beijing , China 2 Institute of Theoretical hysics, the Chinese Academy of Sciences,.O. Box 2735, Beijing , China 3 Graduate School of the Chinese Academy of Sciences, Beijing , China 4 Department of hysics, Nankai University, Tianjin , China 5 Department of hysics, Fujian Normal University, Fuzhou , China Received July 19, 2004 Abstract We present an approach to solve Bethe Salpeter BS equations exactly without any approximation if the kernel of the BS equations exactly is instantaneous, and take positronium as an example to illustrate the general features of the exact solutions. The key step for the approach is from the BS equations to derive a set of coupled and welldetermined integration equations in linear eigenvalue for the components of the BS wave functions equivalently, which may be solvable numerically under a controlled accuracy, even though there is no analytic solution. For positronium, the exact solutions precisely present corrections to those of the corresponding Schrödinger equation in order v 1 v is the relative velocity for eigenfunctions, in order v 2 for eigenvalues, and the mixing between S and D components in J C = 1 states etc., quantitatively. Moreover, we also point out that there is a questionable step in some existent derivations for the instantaneous BS equations if one is pursuing the exact solutions. Finally, we emphasize that one should take the Ov corrections emerging in the exact solutions into account accordingly if one is interested in the relativistic corrections for relevant problems to the bound states. ACS numbers: St, Dr, Ds Key words: instantaneous BS equation, exact solutions, positronium, relativistic corrections Bethe Salpeter BS equation [1 is a very good tool to treat various relativistic bound state systems. For a fermion-antifermion binding system, the BS equation is written as p 1 m 1 χ q p 2 m 2 d 4 k = i 2π 4 V, q, kχ k, 1 where χ q is the BS wave function, is the total momentum, q is relative momentum, and V, q, k is the so-called BS kernel between the electron and positron in the bound state, p 1, p 2 are the momenta of the constituent electron 1 and positron 2, respectively. The total momentum and the relative momentum q are related to the momenta of the fermion-antifermion as follows: p 1 = α 1 q, α 1 = m 1 /m 1 m 2, p 2 = α 2 q, α 2 = m 2 /m 1 m 2. The BS wave function χ q satisfies the normalization condition: d 4 qd 4 q 2π 4 [ Tr χ q [S1 1 p p 1S2 1 p 2δ 4 q q 0 = 2ip 0. 2 V, q, q χ q If the kernel V, q, k of the BS equation has the behavior: V, q, k =0 = V q, k in = 0 frame C.M.S of the concerned bound state, the BS equation is called as instantaneous one, and may be derived to a Schrödinger equation accordingly it was firstly realized by E.E. Salpeter. [2,3 As an example, the BS equation for positronium in the lowest order has the Coulomb kernel as follows: V, q, k =0 = γ 0 V v γ 0 = γ 0 4πα q k 2 γ0. Since in Coulomb gauge, the transverse-photon exchange between electron and positron for the e e bound states is considered as higher order, so with V, q, k as above in the lowest order the BS equation is instantaneous exactly. Thus, when we present the approach to solving an instantaneous BS equation exactly, for convenience and applications, we will take positronium as an example and explore the common features of the solution. The key step for the approach is to derive the instantaneous BS equation to a set of coupled and self-consistent integration equations for the components scalar functions of the BS wave functions without any approximation. The set of equations may not have analytic solutions, but they may be solved numerically under controlled accuracy. Here we will present the interesting features of the exact solutions for the S-wave positronium briefly, while we will put the details and those for -wave ones in Refs. [4 and [5. The approach, which we present, in fact essentially is to follow E.E. Salpeter derivation, but without any approximation. Thus as done in Refs. [2 and [3, first of all we introduce the instantaneous BS wave function dq 0 ϕ q i 2π χ q 0, q, 3 The project supported by National Natural Science Foundation of China under Grant Nos and

2 114 CHANG Chao-Hsi, CHEN Jiao-Kai, LI Xue-Qian, and WANG Guo-Li Vol. 43 then the BS equation 1 is re-written as χ q 0, q = S 1 f pµ 1 η q S2 f pµ 2, 4 where S 1 f p 1 and S 2 f p 2 are the propagators of the fermion and anti-fermion respectively with the definition of the BS-nut d 3 k η q 2π 3 V q, k ϕ k. 5 For general applications, here we keep m 1 m 2 at this moment, although the final application in this paper is to positronium m 1 = m 2. The propagators can be decomposed as with ijs i f Jpµ i = Λ i q Jq 0 α i M ω i iɛ ω i = m 2 i q 2, Λ i q Jq 0 α i M ω i iɛ 6 Λ ± i q = 1 2ω i [γ 0 ω i ± Jm i γ q, where J = 1 for the fermion i = 1 and J = 1 for the anti-fermion i = 2. It is easy to check Λ ± i q Λ i q = γ0, Λ ± i q γ0 Λ i q = 0, Λ ± i q γ0 Λ ± i q = Λ± i q. 7 Based on Eq. 7, Λ ± can be considered as energy projection operators, and they are complete for the projection. For below discussions let us introduce the notations q as ϕ ±± ϕ ±± q Λ ± 1 q γ0 ϕ q γ 0 Λ ± 2 q. 8 Because of the completeness of the projection for Λ ±, we have: ϕ q = ϕ q ϕ q ϕ q ϕ q for the BS wave function ϕ q. As done by E.E. Salpeter to derive the instantaneous BS equation to a corresponding Schrödinger equation, we carry out a contour integration for the time-component q 0 on both sides of Eq. 4, and obtain ϕ q = Λ 1 q η q Λ 2 q Λ 1 q η q Λ 2 q, 9 M ω 1 ω 2 M ω 1 ω 2 M is the eigenvalue and applying the complete set of the projection operators Λ ± i q to Eq. 9 further, we obtain the four equations: M ω 1 ω 2 ϕ q = Λ 1 q η q Λ 2 q, 10 M ω 1 ω 2 ϕ q = Λ 1 q η q Λ 2 q, 11 ϕ q = 0, ϕ q = Now the normalization condition reads: q 2 T dq [ T 2π 2 tr ϕ ϕ ϕ ϕ = M M M M Note that equations 12 do not contain eigenvalue M, so essentially they are constraints on the BS wave functions ϕ q, and because of the completeness of the projectors Λ ±, only the whole set of Eqs are equivalent to Eq. 9. While E.E. Salpeter [2 and the authors of Ref. [3 would like to connect the above coupled equations to the Breit equation, [6,7 so they combined Eqs into one operator equation in C.M.S. of the bound state: Mϕ q γ 0 H 1 q γ 0 ϕ q ϕ q γ 0 H 2 q γ 0 = Λ 1 q η q Λ 2 q Λ 1 q η q Λ 2 q, 14 with the definitions H 1 q m 1 β q α, H 2 q m 2 β q α, β = γ 0, α = β γ. Namely with the definition H 1,2 they considered the equation Eq. 14 as an operator representation of the coupled equations Eqs In fact, exactly to say it is not correct. Equation 14 is not completely equivalent to the coupledequations Eqs Now let us show the un-equivalence as follows. When applying the project operator Λ 1 q γ0 γ 0 Λ 2 q to Eq. 14 we obtain Eq. 10, when applying the project operator Λ 1 q γ0 γ 0 Λ 2 q to Eq. 14 we obtain the Eq. 11, whereas when applying Λ ± 1 q γ0 γ 0 Λ 2 q to Eq. 14, then we obtain the homogeneous equations: [M ω 1 q ω 2 q ϕ q = 0, [M ω 1 q ω 2 q ϕ q = 0 15 with ω 1,2 = m 2 1,2 q 2. The two equations of Eq. 15 not only have the trivial solutions Eq. 12, but also have non-trivial solutions. Therefore, we conclude that equation 14 with the definitions of H 1,2 is not completely equivalent to the BS equation: Eqs Especially, when further approximations on Eq. 14 are made without checking Eq. 12 on the obtained solutions precisely, certain misleading may occur, i.e. the obtained solutions may not be that of the instantaneous BS equation Eq. 9 with η as Eq. 5. The roles of Eqs are important in the present approach. If one really starts with the equation Eq. 14 alone, then it means that one solves the equations Eqs. 10 and 11 and the homogeneous equation Eqs. 15 together. To see the differences, we will solve Eq. 14 with the definitions of H 1,2 and the BS equation: Eqs respectively, and present the results precisely in Ref. [8. The authors of Refs. [2 and [3 etc. thought that, of the coupled equations Eqs , only the so-called positive equation Eq. 10 is important for nonrelativistic binding systems, so they considered it only, and ignored the rests, and then they further assumed that the spin structure of the BS wave function, e.g., for S-wave positronium in c.m.s. = 0, the BS wave function has the formulation precisely ϕ 0 1 S 0 q = [γ 0 1γ 5 f q 16

3 No. 1 Instantaneous Bethe Salpeter Equation and Its Exact Solution 115 for J C = 0 1 S 0 ; and ϕ 1 3 S 1,λ q = [ γ 0 1 A λ f q, A λ ɛ λ γ ɛ λ γ ɛ λ γ, = 0, γ = γ 3 17 for J C = 1 3 S 1. Here 0 is introduced for the zeroth component of γ-matrices in spherical harmonics coordinate to avoid confusions in notation. With the spin structure, making the non-relativistic expansion for ω 1,2 m 1,2 1 q 2 /2m 1,2 and to change the eigenvalue from E to ε M m 1 m 2 as well, they finally turned the equation Eq. 10 for the binding systems exactly to a Schrödinger equation accordingly. To pursue the exact solutions of the instantaneous BS equation 4, we should return to Eqs as a whole without any approximation. Although it is the case for a fermion and anti-fermion system for positronium m 1 = m 2 as an example to illustrate the approach, the approach we present here is also applicable in the cases m 1 m 2, where there is no charge parity quantum number C. [9 In = 0 frame C.M.S., the most general formulation of the BS wave function for the bound states positronium with the quantum numbers J C = 0 1 S 0 may be written as where ϕ1 S 0 q = γ 0 γ 5 ϕ 1 q γ 5 ϕ 2 q 4π q γ5 3 2m Θϕ 3 q 4π 3 γ0 γ 5 q 2m Θϕ 4 q, 18 Θ [Y 1 1 γ Y 11 γ Y 10 γ, γ = γ 3, γ γ1 iγ 2 2, γ = γ1 iγ 2 2, and Y lm Y lm θ q, φ q are spherical harmonics. First of all, to apply Eq. 12 to Eq. 18, we obtain the constraints for the components of the wave functions precisely: ϕ 1 q = 1 2 ϕ 4 q, ϕ 3 q = utting the constraints Eq. 19 into Eq. 18 of the states 0, the components ϕ 3, ϕ 4 are replaced, then the wave function contains two independent components ϕ 1, ϕ 2 only, ϕ1 S 0 q = γ 0 γ 5 ϕ 1 q γ 5 ϕ 2 q 4π 3 γ0 γ 5 q m Θϕ 1 q. 20 By straightforward calculations including to integrate out the relative angles, equations 10 and 11 for positronium, finally, are turned into the coupled radius equations M 2mf 1 2mf 1 2mf 2 = α s π m k ω q d k Q 0 f 2, M 2mf 2 2 ω2 m f 1 2mf 2 = α s m k π ω q d k Q 0 q k m 2 Q 1 f 1 21 with the normalization for the BS wave function q 2 d q 4ω 2π 2 m f 1f 2 = M. 22 Here q 2 Q n Q k 2 n 2 q k n = 0, 1,... are the n-th the Legendre functions of the second kind. Here to shorten the notations we have introduced f 1,2 : ϕ 1 q f 1, ϕ 2 q f 2 and ω = ω 1,2 m 1 = m 2. Especially, we note here that equations 21 are coupled and self-consistent equations in respect to two independent scalar functions f 1,2 respectively and there is not any approximation. They are exact they may be solved numerically under controlled accuracy and may be applicable even to extremely relativistic case. To see the general features for positronium and to reach to the accuracy α 2, we further solve the coupled equations Eq. 21 numerically: to expand them and f 1,2 on the bases of the exact solution of the Schrödinger equation, then to diagonalize the obtained matrix equations on the bases. The corresponding eigenfunctions are expanded as f j i q = nl i,nl R nl q, 23 where j denotes the j-th eigenvalue and eigenfunction, R nl q n and l are the principal and angular quantum numbers: nl = 1S, 2S, 2, 3S, 3,... denotes the Schrödinger radius solution in momentum representation for the positronium their precise expression can be found in Ref. [10. The final results the values of the fine structure constant α and the electron mass are taken so accurate as given by DG, [11 the eigenvalues M j 2m E j, E 1 = [85 ; E 2 = [71 ; E 3 = [18 ; Note that the two digital numbers in the squared brackets in Eq. 24 mean that only the last two digital numbers should be replaced when the solution of the instantaneous BS equation change into that of the Schrödinger equation accordingly. The resultant eigenfunctions corresponding to the eigenvalues are listed in Table 1.

4 116 CHANG Chao-Hsi, CHEN Jiao-Kai, LI Xue-Qian, and WANG Guo-Li Vol. 43 Table 1 NL WF i,1s The expansion coefficients i,nl for the J C = 0 states. i,2s i,3s i,4s E 1 f S 0 f E 2 f S 0 f E 3 f S 0 f In fact, according to Table 1 and up to the order v accuracy, the eigenfunctions for J C = 0 1 S 0 states can be approximately simplified to write as { } 4π ϕ1 S 0 q γ 0 q 1 Θγ0 fγ 5 Ov 2, 25 3 m i.e. f 1 q f 2 q f = R nl=0 q. The solutions for the 1 positronium states are more interesting than those of 0. Similar to the case of 0 states for the general form of the wave functions from Eq. 18 four components to Eq. 20 two components, now having the constraints Eq. 12 applied, the general form of the BS wave functions for 1 states are reduced from a general form eight components to the following form four components, π π ϕ 1,λ q = 2 3 C λ A λ f D λγ 5 A λ γ 0 f 2 where f i ϕ i q i = 1, 2, 3, 4, A λ is the same as in Eq. 17 and C λ B λ f 3 B λ 6ɛ λ γ Y ɛ λ γ ɛ λ γ Y 2 1 ɛ λ γ ɛ λ γ 2ɛ λ γ Y 20 3 ɛ λ γ ɛ λ γ Y 21 6ɛ λ γ Y 22, 5 3 D λγ 5 B λ γ 0 f 4, 26 C λ q [ ɛ λ m Y 1 1 ɛ λ Y 11 ɛ λ Y 10, D λ q [ ɛ λ m γ ɛ λ γ Y 11 ɛ λ γ ɛ λ γ Y 1 1 ɛ λ γ ɛ λ γ Y 10. From Eq. 26, one may see clearly that f 3,4 correspond to D-wave components, while f 1,2 to S-wave ones and the formulism Eq. 26 is suitable to describe the S D component mixing in 1 states. From Eqs. 10 and 11 and to carry out the angular integration, finally we obtain the coupled radius equations: M 2mf 1 = q 2 π m f 4 2mf 1 2m2 4ω 2 f 2 α k [ 3m π q d 5 k 9π M 2mf 2 = q 2 π m f 3 2 2m 2 ω 2 f 1 2mf 2 α k 1 k [ 3 m π q d 3 M 2mf 3 = 2mf 3 2 2m 2 ω 2 f 4 4 π 3 m 3 q 2 5 m f 2 α k [ q π q d k k 3mω Q 1 m ω Q 2 M 2mf 4 = 1 2m 2 4ω 2 3 m f 3 2mf 4 4 π 3 q 2 5 m f 1 α π q k 2 mω Q q 1f 4 k 3 mω Q 1 m ω Q 0 f 2, 5 q k 1 π mω Q q 1f 3 k 3 mω Q 1 m ω Q 0 f 1, f 4 2 π 3 q k 5 mω Q 1f 2, k m k [ q d ω Q 2 2 q k 3 mω Q 1 f 3 2 π 3 q k 5 mω Q 1f The normalization condition of the BS wave functions now becomes q 2 d q 6ω 2π 2 mπ f 3f 4 f 3 f 2 f 1 f 4 3f 1 f 2 = 2M. 28 To be self-consistent, the four coupled equations for f 1,2,3,4 Eq. 27 are the request to describe the S D wave mixing. With the same method as the case for 0, we solve the set of coupled equations Eq. 27 numerically and obtain the results for eigenvalues M j 2m = E j as follows: E 1 3 S 1 = [85 ; E 2 3 S 1 = [12 ;

5 No. 1 Instantaneous Bethe Salpeter Equation and Its Exact Solution 117 E 3 3 S 1 = [18 ; E 4 3 D 1 = [18 ; The two digital numbers in the squared brackets in Eq. 29 have the same meaning as those in Eq. 24, i.e., they are the last two digital numbers which are different from those eigenvalues of the Schrödinger equation. The coefficients i,nl for the eigenfunctions are listed in Table 2. According to Table 2, for J C = 1 3 S 1 states with the approximation to α 2 v 2, we can simplify f 1 q f 2 q f = R nl=0 q and f 3 q f 4 q 0 Dwave components vanish, i.e. [ π q ϕ3 S 1,λ q 2 3 m C λ A λ 2 π 3 q m D λγ 5 A λ γ 0 f. 30 While for J C = 1 3 D 1 states with the approximation to α 2 v 2, we can simplify f 1 q f 2 q 0 S-wave components vanish and f 3 q f 4 q f = R nl=2 q, i.e. [ 5 ϕ3 D q q 1,λ 2 3 m C λ B λ 5 q 3 m D λγ 5 B λ γ 0 f. 31 We may see that the exact solution obtained here for the wave function contains the order v = q /m corrections to the approximate ones obtained by E.E. Salpeter approach as described above, namely, we obtain the correction terms explicitly proportional to v in Eqs. 25, 30 and 31. An interesting fact is that the S D wave mixing for 1 states due to the instantaneous interaction is fixed by the exact solution. To compare the eigenvalues Eq. 24 for 0 and Eq. 29 for 1 with those of the Schrödinger solution the degenerate ones without any splitting, we may also see that the hyperfine splitting purely from the instantaneous interaction for spin singlet and triplet states is in order of α 2 v α, and there is a remarkable splitting between n[ 3 S 1 and n[ 3 D 1 n 3 for 1 states E S 1 E3 Sch for Schrödinger equation E D 1 and E α 2 due to the fact that the BS equation Eq. 4 is relativistic. We should emphasize several points for the approach to solving instantaneous equations exactly: i The set of Eqs. 10, 11, and Eq. 12 are treated equally ; ii We had better to solve the derived equations, such as Eq. 21 for 0 and Eq. 27 for 1 etc. [5 directly, i.e. to keep the equations with linear eigenvalue originally, but not to solve them by changing them to the equations with quadratic even higher eigenvalues etc.; iii To obtain the clean S-D wave mixing in the states 1 etc., we had better to de-composite the BS wave function to the equations for scalar components in polar coordinate. In the literature, when solving an instantaneous BS equation, in many cases to Eq. 12 less attention was payed, the gauge invariance for radiative transitions was broken quite often. [4 Note that the exact precise equations derived from an instantaneous BS equation with a different kernel may be different from those for positronium as described above, but the present approach may be applicable and exact solutions can be obtained accordingly. NL WF 1S Table 2 The expansion coefficients i,nl for the J C = 1 states. 2S 3S f E 1 f S 1 f f f E 2 f S 1 f f f E 3 f S 1 f f f E 4 f D 1 f f D 4S 4D

6 118 CHANG Chao-Hsi, CHEN Jiao-Kai, LI Xue-Qian, and WANG Guo-Li Vol. 43 In summary, for the positronium example with Coulomb instantaneous interaction being considered, the values and the spin structure of the BS wave functions, the relativistic corrections to the eigenvalues energy level and the possible mixing, such as that between S and D components in J C = 1 states etc. are determined by solving the instantaneous BS equation exactly. The general feature on the quantities is that the corrections to the eigenvalues energy level of the Schrödinger equation are of the order α 2 v 2 v is the relative velocity between electron and positron and those to the wave functions spin structure are of the order Ov. Although based on the specific system of positronium, the general features should not be changed much for the other systems which may be described by an instantaneous BS equation. Since the wave functions contain relativistic corrections in order Ov, thus if the relevant calculations declare that the relativistic effects are taken into account, the relativistic corrections from the wave functions should be considered carefully. For the effective theories, such as NRQED [12 and NRQCD, [13 the relativistic effects from the wave functions may be involved either at matching the underlined theory to the effective one or into the non-perturbative matrix elements properly, but we should note here that in the literature many calculations under the framework of the effective theories when matching the underlined theory to the effective one, the spin projectors, where the relative motions between the two composite elements fermion and anti-fermion were ignored, i.e., equations 16 and 17 were adopted. If the corrections even in order v 1 from the wave functions are taken into account, the spin projectors for the matching should take those as Eqs. 25, 30 and 31. Since we have not involved the contributions from transverse photon exchange and the annihilation of electronpositron as high order ones yet, so at present stage for positronium we do not compare the exact solutions of the instantaneous BS equation with experimental data. We will present the comparisons soon elsewhere when the mentioned contributions are taken into account. Acknowledgments The author C.H. Chang would like to thank Stephen L. Adler for valuable discussions and to thank Xiang-Dong Ji for very useful discussions. The authors would like to thank Tso-Hsiu Ho and Cheng-Rui Ching for valuable suggestion and encouragement. References [1 E.E. Salpeter and H.A. Bethe, hys. Rev [2 E.E. Salpeter, hys. Rev [3 C. Itzykson and J. Zuber, Quantum Field Theory, McGraw-Hill Inc., rinted in the United State of America. [4 Chao-Hsi Chang, Jiao-Kai Chen, and Guo-Li Wang, hepth/ [5 Chao-Hsi Chang, Jiao-Kai Chen, Xue-Qian Li, and Guo- Li Wang, Exact Solutions of Instantaneous Bethe Salpeter Equation for S-Wave and -Wave ositronium in Coulomb Gauge, in preparation. [6 G. Breit, hys. Rev [7 G. Breit and G.E. Brown, hys. Rev ; G.E. Brown and D.G. Ravenhall, roc. Roy. Soc. London A [8 Chao-Hsi Chang and Jiao-Kai Chen The Instantaneous Bethe Salpeter Equation and Its Analog: the Breit Like Equation, nucl-th/ [9 Chao-Hsi Chang, Jiao-Kai Chen, Xue-Qian Li, and Guo- Li Wang, The Exact Solution of the Instantanious BS Equation for µ e or µ e System, in preparation. [10 H.A. Bethe and E.E. Salpeter, Quantum Mechanics of One- and Two-Electron Atoms, Springer-Verlag, OHG, Berlin Göttingen Heidelberg, Gemerny [11 article Data Group, hys. Rev. D [12 W.E. Caswell and G.. Lepage, hys. Lett [13 Geoffrey T. Bodwin, Eric Braaten, and G. eter Lepage, hys. Rev. D ; Erratum, ibid. D

Helium fine structure Ingvar Lindgren (mod )

Helium fine structure Ingvar Lindgren (mod ) Helium fine structure Ingvar Lindgren 2004.09.20 (mod. 2005.01.23) The leading contributions to the helium fine structure beyond the first-order relativistic contribution were first derived by Araki [1]

More information

ψ s a ˆn a s b ˆn b ψ Hint: Because the state is spherically symmetric the answer can depend only on the angle between the two directions.

ψ s a ˆn a s b ˆn b ψ Hint: Because the state is spherically symmetric the answer can depend only on the angle between the two directions. 1. Quantum Mechanics (Fall 2004) Two spin-half particles are in a state with total spin zero. Let ˆn a and ˆn b be unit vectors in two arbitrary directions. Calculate the expectation value of the product

More information

Heavy Hybrids Mesons in NRQCD: Fine and Hyperfine Structure

Heavy Hybrids Mesons in NRQCD: Fine and Hyperfine Structure Heavy Hybrids Mesons in NRQCD: Fine and Hyperfine Structure Author: Pere Solé Campreciós. Advisor: oan Soto Facultat de Física, Universitat de Barcelona, Diagonal 645, 828 Barcelona, Spain*. Abstract:

More information

The 3 dimensional Schrödinger Equation

The 3 dimensional Schrödinger Equation Chapter 6 The 3 dimensional Schrödinger Equation 6.1 Angular Momentum To study how angular momentum is represented in quantum mechanics we start by reviewing the classical vector of orbital angular momentum

More information

Optical Lattices. Chapter Polarization

Optical Lattices. Chapter Polarization Chapter Optical Lattices Abstract In this chapter we give details of the atomic physics that underlies the Bose- Hubbard model used to describe ultracold atoms in optical lattices. We show how the AC-Stark

More information

Quantum Mechanics Solutions

Quantum Mechanics Solutions Quantum Mechanics Solutions (a (i f A and B are Hermitian, since (AB = B A = BA, operator AB is Hermitian if and only if A and B commute So, we know that [A,B] = 0, which means that the Hilbert space H

More information

A Realization of Yangian and Its Applications to the Bi-spin System in an External Magnetic Field

A Realization of Yangian and Its Applications to the Bi-spin System in an External Magnetic Field Commun. Theor. Phys. Beijing, China) 39 003) pp. 1 5 c International Academic Publishers Vol. 39, No. 1, January 15, 003 A Realization of Yangian and Its Applications to the Bi-spin System in an External

More information

Space-Time Symmetries

Space-Time Symmetries Space-Time Symmetries Outline Translation and rotation Parity Charge Conjugation Positronium T violation J. Brau Physics 661, Space-Time Symmetries 1 Conservation Rules Interaction Conserved quantity strong

More information

arxiv:hep-ph/ v1 18 Mar 2006

arxiv:hep-ph/ v1 18 Mar 2006 Radiative decays of B c mesons in a Bethe-Salpeter model arxiv:hep-ph/0603139v1 18 Mar 2006 A. Abd El-Hady a,1, J. R. Spence b and J. P. Vary b a) Physics Department, King Khalid University, Abha 9004,

More information

Addition of Angular Momenta

Addition of Angular Momenta Addition of Angular Momenta What we have so far considered to be an exact solution for the many electron problem, should really be called exact non-relativistic solution. A relativistic treatment is needed

More information

Goal: find Lorentz-violating corrections to the spectrum of hydrogen including nonminimal effects

Goal: find Lorentz-violating corrections to the spectrum of hydrogen including nonminimal effects Goal: find Lorentz-violating corrections to the spectrum of hydrogen including nonminimal effects Method: Rayleigh-Schrödinger Perturbation Theory Step 1: Find the eigenvectors ψ n and eigenvalues ε n

More information

The general solution of Schrödinger equation in three dimensions (if V does not depend on time) are solutions of time-independent Schrödinger equation

The general solution of Schrödinger equation in three dimensions (if V does not depend on time) are solutions of time-independent Schrödinger equation Lecture 17 Page 1 Lecture 17 L17.P1 Review Schrödinger equation The general solution of Schrödinger equation in three dimensions (if V does not depend on time) is where functions are solutions of time-independent

More information

Chem 442 Review for Exam 2. Exact separation of the Hamiltonian of a hydrogenic atom into center-of-mass (3D) and relative (3D) components.

Chem 442 Review for Exam 2. Exact separation of the Hamiltonian of a hydrogenic atom into center-of-mass (3D) and relative (3D) components. Chem 44 Review for Exam Hydrogenic atoms: The Coulomb energy between two point charges Ze and e: V r Ze r Exact separation of the Hamiltonian of a hydrogenic atom into center-of-mass (3D) and relative

More information

6.1 Nondegenerate Perturbation Theory

6.1 Nondegenerate Perturbation Theory 6.1 Nondegenerate Perturbation Theory Analytic solutions to the Schrödinger equation have not been found for many interesting systems. Fortunately, it is often possible to find expressions which are analytic

More information

Introduction to Modern Quantum Field Theory

Introduction to Modern Quantum Field Theory Department of Mathematics University of Texas at Arlington Arlington, TX USA Febuary, 2016 Recall Einstein s famous equation, E 2 = (Mc 2 ) 2 + (c p) 2, where c is the speed of light, M is the classical

More information

arxiv: v2 [hep-th] 6 Jul 2009

arxiv: v2 [hep-th] 6 Jul 2009 HIP-9-/TH Dirac Equation in Noncommutative Space for Hydrogen Atom arxiv:9.86v [hep-th] 6 Jul 9 T. C. Adorno, M. C. Baldiotti, M. Chaichian, D. M. Gitman and A. Tureanu Instituto de Física, Universidade

More information

129 Lecture Notes More on Dirac Equation

129 Lecture Notes More on Dirac Equation 19 Lecture Notes More on Dirac Equation 1 Ultra-relativistic Limit We have solved the Diraction in the Lecture Notes on Relativistic Quantum Mechanics, and saw that the upper lower two components are large

More information

Molecules in Magnetic Fields

Molecules in Magnetic Fields Molecules in Magnetic Fields Trygve Helgaker Hylleraas Centre, Department of Chemistry, University of Oslo, Norway and Centre for Advanced Study at the Norwegian Academy of Science and Letters, Oslo, Norway

More information

Transition Matrix Elements for Pion Photoproduction

Transition Matrix Elements for Pion Photoproduction Transition Matrix Elements for Pion Photoproduction Mohamed E. Kelabi 1 Abstract We have obtained the transition matrix elements for pion photoproduction by considering the number of gamma matrices involved.

More information

charges q r p = q 2mc 2mc L (1.4) ptles µ e = g e

charges q r p = q 2mc 2mc L (1.4) ptles µ e = g e APAS 5110. Atomic and Molecular Processes. Fall 2013. 1. Magnetic Moment Classically, the magnetic moment µ of a system of charges q at positions r moving with velocities v is µ = 1 qr v. (1.1) 2c charges

More information

Lecture 7 From Dirac equation to Feynman diagramms. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2

Lecture 7 From Dirac equation to Feynman diagramms. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 Lecture 7 From Dirac equation to Feynman diagramms SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 Dirac equation* The Dirac equation - the wave-equation for free relativistic fermions

More information

(relativistic effects kinetic energy & spin-orbit coupling) 3. Hyperfine structure: ) (spin-spin coupling of e & p + magnetic moments) 4.

(relativistic effects kinetic energy & spin-orbit coupling) 3. Hyperfine structure: ) (spin-spin coupling of e & p + magnetic moments) 4. 4 Time-ind. Perturbation Theory II We said we solved the Hydrogen atom exactly, but we lied. There are a number of physical effects our solution of the Hamiltonian H = p /m e /r left out. We already said

More information

PoS(Confinement X)133

PoS(Confinement X)133 Endpoint Logarithms in e + e J/ψ + η c Geoffrey T. Bodwin HEP Division, Argonne National Laboratory E-mail: gtb@hep.anl.gov Department of Physics, Korea University E-mail: neville@korea.ac.kr Jungil Lee

More information

On the relativistic L S coupling

On the relativistic L S coupling Eur. J. Phys. 9 (998) 553 56. Printed in the UK PII: S043-0807(98)93698-4 On the relativistic L S coupling P Alberto, M Fiolhais and M Oliveira Departamento de Física, Universidade de Coimbra, P-3000 Coimbra,

More information

PHY 407 QUANTUM MECHANICS Fall 05 Problem set 1 Due Sep

PHY 407 QUANTUM MECHANICS Fall 05 Problem set 1 Due Sep Problem set 1 Due Sep 15 2005 1. Let V be the set of all complex valued functions of a real variable θ, that are periodic with period 2π. That is u(θ + 2π) = u(θ), for all u V. (1) (i) Show that this V

More information

a = ( a σ )( b σ ) = a b + iσ ( a b) mω 2! x + i 1 2! x i 1 2m!ω p, a = mω 2m!ω p Physics 624, Quantum II -- Final Exam

a = ( a σ )( b σ ) = a b + iσ ( a b) mω 2! x + i 1 2! x i 1 2m!ω p, a = mω 2m!ω p Physics 624, Quantum II -- Final Exam Physics 624, Quantum II -- Final Exam Please show all your work on the separate sheets provided (and be sure to include your name). You are graded on your work on those pages, with partial credit where

More information

arxiv:gr-qc/ v2 6 Apr 1999

arxiv:gr-qc/ v2 6 Apr 1999 1 Notations I am using the same notations as in [3] and [2]. 2 Temporal gauge - various approaches arxiv:gr-qc/9801081v2 6 Apr 1999 Obviously the temporal gauge q i = a i = const or in QED: A 0 = a R (1)

More information

PHYSICS DEPARTMENT, PRINCETON UNIVERSITY PHYSICS 505 FINAL EXAMINATION. January 18, 2013, 1:30 4:30pm, A06 Jadwin Hall SOLUTIONS

PHYSICS DEPARTMENT, PRINCETON UNIVERSITY PHYSICS 505 FINAL EXAMINATION. January 18, 2013, 1:30 4:30pm, A06 Jadwin Hall SOLUTIONS PHYSICS DEPARTMENT, PRINCETON UNIVERSITY PHYSICS 55 FINAL EXAMINATION January 18, 13, 1:3 4:3pm, A6 Jadwin Hall SOLUTIONS This exam contains five problems Work any three of the five problems All problems

More information

ψ(t) = U(t) ψ(0). (6.1.1)

ψ(t) = U(t) ψ(0). (6.1.1) Chapter 6 Symmetries 6.1 Quantum dynamics The state, or ket, vector ψ of a physical system completely characterizes the system at a given instant. The corresponding bra vector ψ is the Hermitian conjugate

More information

Plane wave solutions of the Dirac equation

Plane wave solutions of the Dirac equation Lecture #3 Spherical spinors Hydrogen-like systems again (Relativistic version) irac energy levels Chapter, pages 48-53, Lectures on Atomic Physics Chapter 5, pages 696-76, Bransden & Joachain,, Quantum

More information

Problem 1: Spin 1 2. particles (10 points)

Problem 1: Spin 1 2. particles (10 points) Problem 1: Spin 1 particles 1 points 1 Consider a system made up of spin 1/ particles. If one measures the spin of the particles, one can only measure spin up or spin down. The general spin state of a

More information

Lecture 10. The Dirac equation. WS2010/11: Introduction to Nuclear and Particle Physics

Lecture 10. The Dirac equation. WS2010/11: Introduction to Nuclear and Particle Physics Lecture 10 The Dirac equation WS2010/11: Introduction to Nuclear and Particle Physics The Dirac equation The Dirac equation is a relativistic quantum mechanical wave equation formulated by British physicist

More information

Potential energy, from Coulomb's law. Potential is spherically symmetric. Therefore, solutions must have form

Potential energy, from Coulomb's law. Potential is spherically symmetric. Therefore, solutions must have form Lecture 6 Page 1 Atoms L6.P1 Review of hydrogen atom Heavy proton (put at the origin), charge e and much lighter electron, charge -e. Potential energy, from Coulomb's law Potential is spherically symmetric.

More information

Attempts at relativistic QM

Attempts at relativistic QM Attempts at relativistic QM based on S-1 A proper description of particle physics should incorporate both quantum mechanics and special relativity. However historically combining quantum mechanics and

More information

Lecture 10. Central potential

Lecture 10. Central potential Lecture 10 Central potential 89 90 LECTURE 10. CENTRAL POTENTIAL 10.1 Introduction We are now ready to study a generic class of three-dimensional physical systems. They are the systems that have a central

More information

( ). Expanding the square and keeping in mind that

( ). Expanding the square and keeping in mind that One-electron atom in a Magnetic Field When the atom is in a magnetic field the magnetic moment of the electron due to its orbital motion and its spin interacts with the field and the Schrodinger Hamiltonian

More information

Figure 1. (a) (b) (c)

Figure 1. (a) (b) (c) arxiv:hep-ph/9407339 v 15 Jan 1997 (a) (b) (c) Figure 1 arxiv:hep-ph/9407339 v 15 Jan 1997 H S Figure arxiv:hep-ph/9407339 v 15 Jan 1997 P/ + p - P/ + p (a) (b) Figure 3 arxiv:hep-ph/9407339 v 15 Jan 1997

More information

Improved Coulomb Potential. Abstract

Improved Coulomb Potential. Abstract THEF-NIJM 8.18 Improved Coulomb Potential G. J. M. Austen and J. J. de Swart Institute for Theoretical Physics, University of Nijmegen, Nijmegen, The Netherlands Abstract An improved Coulomb potential

More information

Multi-Electron Atoms II

Multi-Electron Atoms II Multi-Electron Atoms II LS Coupling The basic idea of LS coupling or Russell-Saunders coupling is to assume that spin-orbit effects are small, and can be neglected to a first approximation. If there is

More information

Maxwell s equations. electric field charge density. current density

Maxwell s equations. electric field charge density. current density Maxwell s equations based on S-54 Our next task is to find a quantum field theory description of spin-1 particles, e.g. photons. Classical electrodynamics is governed by Maxwell s equations: electric field

More information

Approximation Methods in QM

Approximation Methods in QM Chapter 3 Approximation Methods in QM Contents 3.1 Time independent PT (nondegenerate)............... 5 3. Degenerate perturbation theory (PT)................. 59 3.3 Time dependent PT and Fermi s golden

More information

PHYSICS PH.D. COMPREHENSIVE EXAM 2006

PHYSICS PH.D. COMPREHENSIVE EXAM 2006 PHYSICS PH.D. COMPREHENSIVE EXAM 2006 (1) In construction work, a practical means of establishing a vertical reference line is the use of a plumb line a mass hanging in equilibrium from a long vertical

More information

Lecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2

Lecture 6 Scattering theory Partial Wave Analysis. SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 Lecture 6 Scattering theory Partial Wave Analysis SS2011: Introduction to Nuclear and Particle Physics, Part 2 2 1 The Born approximation for the differential cross section is valid if the interaction

More information

Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction

Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction Lecture 5 Coupling of Angular Momenta Isospin Nucleon-Nucleon Interaction WS0/3: Introduction to Nuclear and Particle Physics,, Part I I. Angular Momentum Operator Rotation R(θ): in polar coordinates the

More information

Spectra of Free Diquark in the Bethe Salpeter Approach

Spectra of Free Diquark in the Bethe Salpeter Approach Commun. Theor. hys. (Beijing, China) 46 (2006) pp. 1031 1039 c International Academic ublishers Vol. 46, No. 6, December 15, 2006 Spectra of Free Diquark in the Bethe Salpeter Approach YU Yan-ing, 1 KE

More information

Forbidden Electric Dipole Transitions in the Hydrogen Molecular Ion First Estimates

Forbidden Electric Dipole Transitions in the Hydrogen Molecular Ion First Estimates Bulg. J. Phys. 44 (2017) 76 83 Forbidden Electric Dipole Transitions in the Hydrogen Molecular Ion First Estimates P. Danev Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences,

More information

9 Electron orbits in atoms

9 Electron orbits in atoms Physics 129b Lecture 15 Caltech, 02/22/18 Reference: Wu-Ki-Tung, Group Theory in physics, Chapter 7. 9 Electron orbits in atoms Now let s see how our understanding of the irreps of SO(3) (SU(2)) can help

More information

4-Space Dirac Theory and LENR

4-Space Dirac Theory and LENR J. Condensed Matter Nucl. Sci. 2 (2009) 7 12 Research Article 4-Space Dirac Theory and LENR A. B. Evans Department of Mathematics and Statistics, University of Otago, P.O. Box 56, Dunedin, New Zealand

More information

arxiv:quant-ph/ v1 10 May 1999

arxiv:quant-ph/ v1 10 May 1999 Minimal Length Uncertainty Relation and Hydrogen Atom F. Brau Université de Mons-Hainaut, B-7 Mons, BELGIQUE (February 1, 8) arxiv:quant-ph/99533v1 1 May 1999 Abstract We propose a new approach to calculate

More information

Comparing and Improving Quark Models for the Triply Bottom Baryon Spectrum

Comparing and Improving Quark Models for the Triply Bottom Baryon Spectrum Comparing and Improving Quark Models for the Triply Bottom Baryon Spectrum A thesis submitted in partial fulfillment of the requirements for the degree of Bachelor of Science degree in Physics from the

More information

(a) Write down the total Hamiltonian of this system, including the spin degree of freedom of the electron, but neglecting spin-orbit interactions.

(a) Write down the total Hamiltonian of this system, including the spin degree of freedom of the electron, but neglecting spin-orbit interactions. 1. Quantum Mechanics (Spring 2007) Consider a hydrogen atom in a weak uniform magnetic field B = Bê z. (a) Write down the total Hamiltonian of this system, including the spin degree of freedom of the electron,

More information

Nuclear models: Collective Nuclear Models (part 2)

Nuclear models: Collective Nuclear Models (part 2) Lecture 4 Nuclear models: Collective Nuclear Models (part 2) WS2012/13: Introduction to Nuclear and Particle Physics,, Part I 1 Reminder : cf. Lecture 3 Collective excitations of nuclei The single-particle

More information

Chemistry 3502/4502. Final Exam Part I. May 14, 2005

Chemistry 3502/4502. Final Exam Part I. May 14, 2005 Advocacy chit Chemistry 350/450 Final Exam Part I May 4, 005. For which of the below systems is = where H is the Hamiltonian operator and T is the kinetic-energy operator? (a) The free particle

More information

THE QUANTUM MECHANICAL CURRENT OF THE PAULI EQUATION

THE QUANTUM MECHANICAL CURRENT OF THE PAULI EQUATION THE QUANTUM MECHANICAL CURRENT OF THE PAULI EQUATION Marek Nowakowski Grup de Física Teòrica, Universitat Autònoma de Barcelona, 08193 Bellaterra, Spain Abstract We argue that the process of constructing

More information

Ket space as a vector space over the complex numbers

Ket space as a vector space over the complex numbers Ket space as a vector space over the complex numbers kets ϕ> and complex numbers α with two operations Addition of two kets ϕ 1 >+ ϕ 2 > is also a ket ϕ 3 > Multiplication with complex numbers α ϕ 1 >

More information

11.D.2. Collision Operators

11.D.2. Collision Operators 11.D.. Collision Operators (11.94) can be written as + p t m h+ r +p h+ p = C + h + (11.96) where C + is the Boltzmann collision operator defined by [see (11.86a) for convention of notations] C + g(p)

More information

Evaluation of Triangle Diagrams

Evaluation of Triangle Diagrams Evaluation of Triangle Diagrams R. Abe, T. Fujita, N. Kanda, H. Kato, and H. Tsuda Department of Physics, Faculty of Science and Technology, Nihon University, Tokyo, Japan E-mail: csru11002@g.nihon-u.ac.jp

More information

Angular momentum and spin

Angular momentum and spin Luleå tekniska universitet Avdelningen för Fysik, 007 Hans Weber Angular momentum and spin Angular momentum is a measure of how much rotation there is in particle or in a rigid body. In quantum mechanics

More information

Solutions to exam : 1FA352 Quantum Mechanics 10 hp 1

Solutions to exam : 1FA352 Quantum Mechanics 10 hp 1 Solutions to exam 6--6: FA35 Quantum Mechanics hp Problem (4 p): (a) Define the concept of unitary operator and show that the operator e ipa/ is unitary (p is the momentum operator in one dimension) (b)

More information

Atomic Structure and Processes

Atomic Structure and Processes Chapter 5 Atomic Structure and Processes 5.1 Elementary atomic structure Bohr Orbits correspond to principal quantum number n. Hydrogen atom energy levels where the Rydberg energy is R y = m e ( e E n

More information

MOTT-RUTHERFORD SCATTERING AND BEYOND. Abstract. The electron charge is considered to be distributed or extended in

MOTT-RUTHERFORD SCATTERING AND BEYOND. Abstract. The electron charge is considered to be distributed or extended in MOTT-RUTHERFORD SCATTERING AND BEYOND Abstract The electron charge is considered to be distributed or extended in space. The differential of the electron charge is set equal to a function of the electron

More information

Tight-Binding Model of Electronic Structures

Tight-Binding Model of Electronic Structures Tight-Binding Model of Electronic Structures Consider a collection of N atoms. The electronic structure of this system refers to its electronic wave function and the description of how it is related to

More information

Physics 221A Fall 1996 Notes 13 Spins in Magnetic Fields

Physics 221A Fall 1996 Notes 13 Spins in Magnetic Fields Physics 221A Fall 1996 Notes 13 Spins in Magnetic Fields A nice illustration of rotation operator methods which is also important physically is the problem of spins in magnetic fields. The earliest experiments

More information

129 Lecture Notes Relativistic Quantum Mechanics

129 Lecture Notes Relativistic Quantum Mechanics 19 Lecture Notes Relativistic Quantum Mechanics 1 Need for Relativistic Quantum Mechanics The interaction of matter and radiation field based on the Hamitonian H = p e c A m Ze r + d x 1 8π E + B. 1 Coulomb

More information

Nuclear Shell Model. Experimental evidences for the existence of magic numbers;

Nuclear Shell Model. Experimental evidences for the existence of magic numbers; Nuclear Shell Model It has been found that the nuclei with proton number or neutron number equal to certain numbers 2,8,20,28,50,82 and 126 behave in a different manner when compared to other nuclei having

More information

B-spline-based complex-rotation method with spin-dependent interaction

B-spline-based complex-rotation method with spin-dependent interaction B-spline-based complex-rotation method with spin-dependent interaction T. K. Fang 1 and T. N. Chang 2,3 1 Department of Physics, Fu Jen Catholic University, Taipei, Taiwan 242, ROC 2 Department of Physics

More information

The path integral for photons

The path integral for photons The path integral for photons based on S-57 We will discuss the path integral for photons and the photon propagator more carefully using the Lorentz gauge: as in the case of scalar field we Fourier-transform

More information

Part I. Many-Body Systems and Classical Field Theory

Part I. Many-Body Systems and Classical Field Theory Part I. Many-Body Systems and Classical Field Theory 1. Classical and Quantum Mechanics of Particle Systems 3 1.1 Introduction. 3 1.2 Classical Mechanics of Mass Points 4 1.3 Quantum Mechanics: The Harmonic

More information

LS coupling. 2 2 n + H s o + H h f + H B. (1) 2m

LS coupling. 2 2 n + H s o + H h f + H B. (1) 2m LS coupling 1 The big picture We start from the Hamiltonian of an atomic system: H = [ ] 2 2 n Ze2 1 + 1 e 2 1 + H s o + H h f + H B. (1) 2m n e 4πɛ 0 r n 2 4πɛ 0 r nm n,m Here n runs pver the electrons,

More information

LECTURES ON QUANTUM MECHANICS

LECTURES ON QUANTUM MECHANICS LECTURES ON QUANTUM MECHANICS GORDON BAYM Unitsersity of Illinois A II I' Advanced Bock Progrant A Member of the Perseus Books Group CONTENTS Preface v Chapter 1 Photon Polarization 1 Transformation of

More information

2 Canonical quantization

2 Canonical quantization Phys540.nb 7 Canonical quantization.1. Lagrangian mechanics and canonical quantization Q: How do we quantize a general system?.1.1.lagrangian Lagrangian mechanics is a reformulation of classical mechanics.

More information

Lecture 8 Nature of ensemble: Role of symmetry, interactions and other system conditions: Part II

Lecture 8 Nature of ensemble: Role of symmetry, interactions and other system conditions: Part II Lecture 8 Nature of ensemble: Role of symmetry, interactions and other system conditions: Part II We continue our discussion of symmetries and their role in matrix representation in this lecture. An example

More information

QM and Angular Momentum

QM and Angular Momentum Chapter 5 QM and Angular Momentum 5. Angular Momentum Operators In your Introductory Quantum Mechanics (QM) course you learned about the basic properties of low spin systems. Here we want to review that

More information

CHINESE JOURNAL OF PHYSICS VOL. 43, NO. 2 APRIL Ming-Keh Chen

CHINESE JOURNAL OF PHYSICS VOL. 43, NO. 2 APRIL Ming-Keh Chen CHINESE JOURNAL OF PHYSICS VOL. 43, NO. 2 APRIL 2004 Doubly Excited 1,3 P e Resonances in He Between the N=2 and 3 He + Thresholds Ming-Keh Chen Department of Physics, National Chung-Hsing University,

More information

Angular momentum. Quantum mechanics. Orbital angular momentum

Angular momentum. Quantum mechanics. Orbital angular momentum Angular momentum 1 Orbital angular momentum Consider a particle described by the Cartesian coordinates (x, y, z r and their conjugate momenta (p x, p y, p z p. The classical definition of the orbital angular

More information

(Again, this quantity is the correlation function of the two spins.) With z chosen along ˆn 1, this quantity is easily computed (exercise):

(Again, this quantity is the correlation function of the two spins.) With z chosen along ˆn 1, this quantity is easily computed (exercise): Lecture 30 Relevant sections in text: 3.9, 5.1 Bell s theorem (cont.) Assuming suitable hidden variables coupled with an assumption of locality to determine the spin observables with certainty we found

More information

QUANTUM MECHANICS OF ONE- AND TWO-ELECTRON ATOMS

QUANTUM MECHANICS OF ONE- AND TWO-ELECTRON ATOMS QUANTUM MECHANICS OF ONE- AND TWO-ELECTRON ATOMS QUANTUM MECHANICS OF ONE- AND TWO-ELECTRON ATOMS HANS A. BETHE AND EDWIN E. SALPETER Cornell University Ithaca, New York A PLENUM/ROSETTA EDITION Library

More information

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama

Lorentz-covariant spectrum of single-particle states and their field theory Physics 230A, Spring 2007, Hitoshi Murayama Lorentz-covariant spectrum of single-particle states and their field theory Physics 30A, Spring 007, Hitoshi Murayama 1 Poincaré Symmetry In order to understand the number of degrees of freedom we need

More information

arxiv: v2 [hep-ph] 27 Oct 2009

arxiv: v2 [hep-ph] 27 Oct 2009 Symmetry of Dirac Equation and Corresponding Phenomenology Hong-Wei Ke 1, Zuo Li, Jing-Ling Chen 3, Yi-Bing Ding 4 and Xue-Qian Li 1 School of Science, Tianjin University, Tianjin 30007, China School of

More information

Solutions Final exam 633

Solutions Final exam 633 Solutions Final exam 633 S.J. van Enk (Dated: June 9, 2008) (1) [25 points] You have a source that produces pairs of spin-1/2 particles. With probability p they are in the singlet state, ( )/ 2, and with

More information

PHY4604 Introduction to Quantum Mechanics Fall 2004 Final Exam SOLUTIONS December 17, 2004, 7:30 a.m.- 9:30 a.m.

PHY4604 Introduction to Quantum Mechanics Fall 2004 Final Exam SOLUTIONS December 17, 2004, 7:30 a.m.- 9:30 a.m. PHY464 Introduction to Quantum Mechanics Fall 4 Final Eam SOLUTIONS December 7, 4, 7:3 a.m.- 9:3 a.m. No other materials allowed. If you can t do one part of a problem, solve subsequent parts in terms

More information

Preliminary Quantum Questions

Preliminary Quantum Questions Preliminary Quantum Questions Thomas Ouldridge October 01 1. Certain quantities that appear in the theory of hydrogen have wider application in atomic physics: the Bohr radius a 0, the Rydberg constant

More information

χ cj Decays into B B in Quark-Pair Creation Model

χ cj Decays into B B in Quark-Pair Creation Model Commun. Theor. Phys. (Beijing, China) 41 (4) pp. 5 56 c International Academic Publishers Vol. 41, No., February 15, 4 χ cj Decays into B B in Quark-Pair Creation Model PING Rong-Gang 1, and JIANG Huan-Qing

More information

Atomic and molecular physics Revision lecture

Atomic and molecular physics Revision lecture Atomic and molecular physics Revision lecture Answer all questions Angular momentum J`2 ` J z j,m = j j+1 j,m j,m =m j,m Allowed values of mgo from j to +jin integer steps If there is no external field,

More information

Quantum Physics III (8.06) Spring 2007 FINAL EXAMINATION Monday May 21, 9:00 am You have 3 hours.

Quantum Physics III (8.06) Spring 2007 FINAL EXAMINATION Monday May 21, 9:00 am You have 3 hours. Quantum Physics III (8.06) Spring 2007 FINAL EXAMINATION Monday May 21, 9:00 am You have 3 hours. There are 10 problems, totalling 180 points. Do all problems. Answer all problems in the white books provided.

More information

Two and Three-Dimensional Systems

Two and Three-Dimensional Systems 0 Two and Three-Dimensional Systems Separation of variables; degeneracy theorem; group of invariance of the two-dimensional isotropic oscillator. 0. Consider the Hamiltonian of a two-dimensional anisotropic

More information

Magentic Energy Diagram for A Single Electron Spin and Two Coupled Electron Spins. Zero Field.

Magentic Energy Diagram for A Single Electron Spin and Two Coupled Electron Spins. Zero Field. 7. Examples of Magnetic Energy Diagrams. There are several very important cases of electron spin magnetic energy diagrams to examine in detail, because they appear repeatedly in many photochemical systems.

More information

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω. Wednesday March 30 ± ǁ

. α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω. Wednesday March 30 ± ǁ . α β γ δ ε ζ η θ ι κ λ μ Aμ ν(x) ξ ο π ρ ς σ τ υ φ χ ψ ω. Α Β Γ Δ Ε Ζ Η Θ Ι Κ Λ Μ Ν Ξ Ο Π Ρ Σ Τ Υ Φ Χ Ψ Ω Wednesday March 30 ± ǁ 1 Chapter 5. Photons: Covariant Theory 5.1. The classical fields 5.2. Covariant

More information

Recent Progress on Charmonium Decays at BESIII

Recent Progress on Charmonium Decays at BESIII Recent Progress on Charmonium Decays at BESIII Xiao-Rui Lu (on behalf of the BESIII Collaboration) Physics Department Graduate University of Chinese Academy of Sciences Beijing, 0049, China xiaorui@gucas.ac.cn

More information

Electric Dipole Paradox: Question, Answer, and Interpretation

Electric Dipole Paradox: Question, Answer, and Interpretation Electric Dipole Paradox: Question, Answer, and Interpretation Frank Wilczek January 16, 2014 Abstract Non-vanishing electric dipole moments for the electron, neutron, or other entities are classic signals

More information

Dr Victoria Martin, Spring Semester 2013

Dr Victoria Martin, Spring Semester 2013 Particle Physics Dr Victoria Martin, Spring Semester 2013 Lecture 3: Feynman Diagrams, Decays and Scattering Feynman Diagrams continued Decays, Scattering and Fermi s Golden Rule Anti-matter? 1 Notation

More information

M04M.1 Particles on a Line

M04M.1 Particles on a Line Part I Mechanics M04M.1 Particles on a Line M04M.1 Particles on a Line Two elastic spherical particles with masses m and M (m M) are constrained to move along a straight line with an elastically reflecting

More information

Symmetry Properties of Superconductors

Symmetry Properties of Superconductors Australian Journal of Basic and Applied Sciences, 6(3): 81-86, 2012 ISSN 1991-8178 Symmetry Properties of Superconductors Ekpekpo, A. Department of Physics, Delta State University, Abraka, Nigeria. Abstract:

More information

Relativistic Calculations for Be-like Iron

Relativistic Calculations for Be-like Iron Commun. Theor. Phys. (Beijing, China) 50 (2008) pp. 468 472 Chinese Physical Society Vol. 50, No. 2, August 15, 2008 Relativistic Calculations for Be-like Iron YANG Jian-Hui, 1 LI Ping, 2, ZHANG Jian-Ping,

More information

MATTER THEORY OF EXPANDED MAXWELL EQUATIONS

MATTER THEORY OF EXPANDED MAXWELL EQUATIONS MATTER THEORY OF EXPANDED MAXWELL EQUATIONS WU SHENG-PING Abstract. This article try to unified the four basic forces by Maxwell equations, the only experimental theory. Self-consistent Maxwell equation

More information

Total Angular Momentum for Hydrogen

Total Angular Momentum for Hydrogen Physics 4 Lecture 7 Total Angular Momentum for Hydrogen Lecture 7 Physics 4 Quantum Mechanics I Friday, April th, 008 We have the Hydrogen Hamiltonian for central potential φ(r), we can write: H r = p

More information

Non-Hermitian CP-Symmetric Dirac Hamiltonians with Real Energy Eigenvalues

Non-Hermitian CP-Symmetric Dirac Hamiltonians with Real Energy Eigenvalues Non-Hermitian CP-Symmetric irac Hamiltonians with Real Energy Eigenvalues.. lhaidari Saudi Center for Theoretical Physics, Jeddah 438, Saudi rabia bstract: We present a large class of non-hermitian non-pt-symmetric

More information

Central density. Consider nuclear charge density. Frois & Papanicolas, Ann. Rev. Nucl. Part. Sci. 37, 133 (1987) QMPT 540

Central density. Consider nuclear charge density. Frois & Papanicolas, Ann. Rev. Nucl. Part. Sci. 37, 133 (1987) QMPT 540 Central density Consider nuclear charge density Frois & Papanicolas, Ann. Rev. Nucl. Part. Sci. 37, 133 (1987) Central density (A/Z* charge density) about the same for nuclei heavier than 16 O, corresponding

More information

UNIVERSITY OF MARYLAND Department of Physics College Park, Maryland. PHYSICS Ph.D. QUALIFYING EXAMINATION PART II

UNIVERSITY OF MARYLAND Department of Physics College Park, Maryland. PHYSICS Ph.D. QUALIFYING EXAMINATION PART II UNIVERSITY OF MARYLAND Department of Physics College Park, Maryland PHYSICS Ph.D. QUALIFYING EXAMINATION PART II January 22, 2016 9:00 a.m. 1:00 p.m. Do any four problems. Each problem is worth 25 points.

More information

Preons from holography

Preons from holography arxiv:0801.3670v1 [physics.gen-ph] 23 Jan 2008 Preons from holography T. R. Mongan 84 Marin Avenue Sausalito, CA 94965 USA (415) - 332-1506 tmongan@gmail.com January, 2008 Abstract Our universe is apparently

More information