Emergence of quantization: the spin of the electron

Size: px
Start display at page:

Download "Emergence of quantization: the spin of the electron"

Transcription

1 Journal of Physics: Conference Series OPEN ACCESS Emergence of quantization: the spin of the electron To cite this article: A M Cetto et al 2014 J. Phys.: Conf. Ser View the article online for upates an enhancements. Relate content - Electron system correlate by the zeropoint fiel: physical explanation for the spin-statistics connection A M Cetto an L e la Peña - Zero-Point Fluctuations an Cosmological Constant Bernhar Haisch an Alfonso Ruea - Quantization as an emergent phenomenon ue to matter-zeropoint fiel interaction A M Cetto, L e la Peña an A Valés- Hernánez Recent citations - Is Einsteinian no-signalling violate in Bell tests? Marian Kupczynski - Electron system correlate by the zeropoint fiel: physical explanation for the spin-statistics connection A M Cetto an L e la Peña - Extene Ehrenfest theorem with raiative corrections L e la Peña et al This content was ownloae from IP aress on 31/10/2018 at 14:44

2 Emergence of quantization: the spin of the electron A M Cetto, L e la Peña an A Valés-Hernánez Instituto e Física, Universia Nacional Autónoma e México, Ap. postal , México DF, Mexico ana, luis, anreavh@fisica.unam.mx Abstract. In previous papers, the quantum behavior of matter has been shown to emerge as a result of its permanent interaction with the ranom zero-point raiation fiel. Funamental results, such as the Schröinger an the Heisenberg formalism, have been erive within this framework. Further, the theory has been shown to provie the basic qe formulas for the raiative corrections, as well as an explanation for entanglement in bipartite systems. This paper aresses the problem of spin from the same perspective. The zero-point fiel is shown to prouce a helicoial motion of the electron, through the torque exerte by the electric fiel moes of a given circular polarization, which results in an intrinsic angular momentum, of value /2. Associate with it, a magnetic moment with a g-factor of 2 is obtaine. This allows us to ientify the spin of the electron as a further emergent property, generate by the action of the ranom zero-point fiel. 1. Introuction In previous work, the quantum behavior of matter has been shown to emerge as a result of its continuous interaction with the ranom zero-point raiation fiel (zpf). This has been, in essence, the program of stochastic electroynamics (se). Funamental quantum results, such as the Schröinger an the Heisenberg formalism, have been recently obtaine within this framework [1]. Contact has been mae with (nonrelativistic) quantum electroynamics, by eriving the main formulas for the raiative corrections, notably the Lamb shift an the atomic lifetimes [1], [2]. Further, the stuy of bipartite systems has shown the zpf to lie at the origin of entanglement an the symmetrization postulate [3]. Another most funamental problem in quantum theory relates to the nature of the spin of the electron: is it something inherent, as is usually consiere, or is it a result of the ynamics, as has been postulate time an again? A theory intene to explain the genesis of quantization shoul be expecte to provie an answer to this query, instea of a priori taking the spin as one more innate property of the particle, like the mass or the electric charge. During the initial perio of se [4] the electron was in fact taken as a spinless particle, the only exception being the analysis by Braffort an Taroni [5] of some effects ue to spin. As of 1981, a number of moels for spin as an acquire property have been propose [6]-[12] (there were of course earlier moels, such as that of Huang [13]). Though base on classical moels, the various se calculations exhibit the zpf as the source of a kin of (nonrelativistic) zitterbewegung that gives rise to an intrinsic angular momentum of the electron, with a mean square value of orer 2 an projections of orer. This paper re-aresses the problem of spin from the perspective offere by present se. Before entering into the subject matter, a brief introuction to recent work on se is provie, Content from this work may be use uner the terms of the Creative Commons Attribution 3.0 licence. Any further istribution of this work must maintain attribution to the author(s) an the title of the work, journal citation an DOI. Publishe uner licence by Lt 1

3 focusing on those results that will be use for the present erivations. It then will be shown that in aition to giving rise to position, momentum an energy fluctuations, the zpf inuces a helicoial motion, as a result of the torque exerte by the ranom Lorentz (electric) force on the particle. The fiel moes of a given circular polarization are shown to give rise to an (intrinsic) spin angular momentum of the electron, of value /2. Aitionally, the corresponing magnetic moment with a g-factor of 2 is erive. The paper ens with some brief aitional remarks on the physical meaning of the results obtaine. 2. Emergence of quantum mechanics 2.1. The original stochastic problem This section contains the basic steps that take us from the original ynamical equation for the particle embee in the ranom zpf, to the Schröinger formulation of quantum mechanics [1]. The system uner stuy is a particle of mass m an charge e typically an electron, subject to an external (bining) potential V in aition to the stationary zpf. The motion of the particle is escribe by mẍ = f(x) + mτ... x + ee(t), (1) where mτ... x, with τ = 2e 2 /3mc 3, represents the reaction force ue to Larmor raiation, an f(x) is the force ue to the potential V. A nonrelativistic escription is assume to be sufficient, so that the magnetic term of the Lorentz force is neglecte. The ranom fiel E(t) is taken in the long-wavelength approximation, anticipating that those fiel moes that become eventually ominant have wavelengths much larger than the characteristic imensions of the motion. The ranom fiel has zero mean value, i.e., E(t) (i) = 0, where ( ) (i) enotes the average over all realizations (i) of the fiel, an a spectral energy ensity corresponing to a mean energy ω/2 per frequency moe, i. e., ρ 0 (ω) = ω2 1 ω3 π 2 c 3 ω = 2 2π 2 c 3. (2) This expression correspons to the autocorrelation function where E i (t)e j (t ) (i) = δ ϕ(t t ), (3) ϕ(t t ) = 4π 3 0 ρ 0 (ω) cos ω(t t )ω. (4) If there is an extra component ue to an external fiel, as coul be a thermal equilibrium raiation or any other excitation of the fiel moes, the corresponing contribution must be ae to ρ 0 (ω) in equation (2) Statistical escription from phase space to configuration space The etaile motion of a single particle epens on the specific realization (i) of the fiel, which is unknown. Therefore a statistical escription is mae, by constructing the equation of evolution for the particle phase-space probability ensity Q(x, p, t), taking the zpf as given an starting from the ynamical equations obtaine from (1), mẋ = p, ṗ = f(x) + mτ... x + ee(t). (5) Through a stanar projection proceure [14], the generalize Fokker-Planck equation (gfpe) Q t + 1 p i Q + f i Q + mτ... x i Q = e 2 ˆDi Q (6) m x i p i p i p i 2

4 is obtaine, with the iffusion operator ˆD(t) efine by means of the expression ˆD i (t)q = ˆP E i Ĝ p j E j an the projection operator ˆP an the evolution operator Ĝ given by k=0 ˆP A = A (i), ĜA(x, p, t) = [ eĝ ] 2k (1 p ˆP )E l Q, (7) l t e ˆL(t t ) A(x, p, t )t, (8) where ˆL is ˆL = 1 p i + (f i + mτ... x i ). (9) m x i p i The operator e ˆL(t t ) in equation (8) makes x(t ), p(t ) (t < t) evolve towars x(t), p(t) as final conitions, following a eterministic path. Right after particle an fiel start to interact, the system is far from equilibrium. In this initial regime the main effect of the zpf on the particle is ue to the high-frequency moes, which prouce violent accelerations an ranomize the motion. Eventually, however (after a transient perio which is estimate to be of the orer of /mc s for an electron), the interplay between the electric fiel force an raiation reaction is expecte to rive the system close to equilibrium. In this new (time-reversible) regime the Markovian approximation applies, an the gfpe (6) reuces to a true Fokker-Planck equation, Q t + 1 p i Q + (f i + mτ... x i ) Q = m x i p i D pp Q + D px Q, (10) p i p j p i x j with the iffusion coefficients given to lowest orer in e 2 by D pp = e2 t t ϕ(t t ) p t j p, D px = e2 i t ϕ(t t ) x j p. (11) i A statistical escription in configuration space is mae in terms of a hierarchy of equations, obtaine by multiplying (10) successively by p k i (k = 1, 2,..., where p i stans for the ifferent components of the momentum p ) an integrating over momentum space (assuming the integran to vanish in the limits). In the time-reversible regime, the raiative terms become small an ten to balance each other in the mean, so any aitional effect they may have on the ynamics becomes negligible. When the raiationless approximation is mae (i. e., to zero orer in e 2 ), the first two equations of the hierarchy can be recast in the form of a Schröinger-like equation for a complex function ψ(x, t), 2η2 m 2 ψ + V ψ = 2iη ψ t, (12) an the corresponing complex conjugates, with ψ ψ = 3 pq(x, p, t) = ρ(x, t), an η a free parameter. The value of this parameter is etermine by the energy-balance conition that must hol in the equilibrium regime (see below). 3

5 2.3. Some important relations for average values Equation (6) (or its Markovian version, (10)) contains a wealth of statistical information about the ynamics of the system, part of which is lost in the transition to the reuce, raiationless escription in configuration space. To recover some of this information we take the (phasespace) average of a generic function G(x, p) that has no explicit time epenence. Equation (6) multiplie from the left by G an integrate over the entire phase space gives thus t G = ẋ i G x i + f i G p i + mτ... x i G p i e 2 G p i ˆDi. (13) In particular, for any G = ξ(x, p) representing a classical ( raiationless ) integral of the motion, we have... ξ ξ ξ = mτ x i e 2 ˆDi. (14) t p i p i In the Markovian limit mentione above, this equation takes the form... ξ ξ = mτ x i + t p i D pp 2 ξ p i p j + D px 2 ξ p i x j, (15) with the iffusion coefficients given by (11). For instance, for the particle Hamiltonian (efine without the raiative terms, i. e., to zero orer in e 2 ), H = 1 2m p2 + V (x), (16) equation (15) gives H = τ... x p + 1 t m trdpp. (17) This equation gives the contributions of the issipative an iffusive terms to the energy balance. Stationarity is reache when the terms cancel each other, which shoul occur when both fiel an particle are in their groun state, i.e., τ... x p 0 = 1 m trdpp 0. (18) Notice that for the calculation of these terms (to the lowest orer of approximation) one must use the solutions of the Schröingerlike equation (12), since the system is alreay in the timereversible regime. This means, in particular, that in equations (11) the following replacements must be mae: p j p 1 x j i 2iη [ˆx i, ˆp j ], p 1 i 2iη [ˆx i, ˆx j ]. (19) Explicit calculation gives that for the energy-balance conition (18) to be satisfie, the parameter η must have precisely the value η = /2 [1]. This is, then, the point of entry of Planck s constant into the Schröinger equation, obtaine from (12), 2 2m 2 ψ + V ψ = i ψ t. (20) The time-reversible an raiationless regime, in which the mechanical system is correctly escribe by this equation, is therefore calle the quantum regime. Notice that, from this perspective, provies a irect measure of the intensity of the fluctuations impresse by the zpf upon the (quantum) particle. 4

6 Let us now go back to equation (15), an apply it to the angular momentum L, which is a classical constant of the motion for any central-force problem. By taking ξ =L =x i p j x j p i (i j), we get... L = mτ x x D A, (21) t where D A is the antisymmetric tensor with components D px Dpx ji. This equation tells us that for the angular momentum to be conserve, the raiative terms must cancel each other, mτ x... x = D A. (22) Finally, for the square of the angular momentum L 2, equation (14) gives L 2... = mτ t x i L 2 p i + so that for L 2 to be conserve, we must have... L 2 mτ x i = p i D pp D pp 2 L 2 p i p j 2 L 2 p i p j + D px D px 2 L 2 p i x j These latter results, first propose in [9], will be use in section L 2 p i x j, (23). (24) 2.4.Linear response of the particle in the stationary regime A close analysis of the stationary states attaine by the particle in the time-reversible regime escribe above, has prove particularly revealing of some general properties of quantum systems. For such analysis a more straightforwar approach, complementary to the previous one, has been evelope [1], starting again from the same equation of motion (1), an assuming that any stationary solution of it (characterize by the inex α) can be written as an expansion of the form x α (t) = x αβ a αβ e iωαβt, (25) β an similarly for any ynamical variable, A α (t) = β Ã αβ a αβ e iω αβt, (26) where a αβ stans for the ranom amplitue of the zpf moe of frequency ω αβ, E α (t) = β Ẽ αβ a αβ e iω αβt. (27) In these equations the coefficients x αβ, Ã αβ are in principle functions of the amplitues a αβ, an hence stochastic variables. By introucing these expansions into equation (1), the system is foun to respon resonantly to certain fiel moes (αβ); the rest of the zpf (to be neglecte in the expansions) represents just a backgroun noise. The values of the corresponing ω αβ (calle relevant frequencies), as well as of the coefficients x αβ, epen on the specific problem. By imposing the conition of ergoicity on the stationary solutions, the { x αβ } turn out to be inepenent of the {a αβ }, which means, accoring to (25), that the response of the system to the respective fiel moes is linear in the fiel variables. Further, those moes controlling the stationary states are foun to satisfy certain properties, which can be summarize in terms of the chain rule for the ranom fiel coefficients, a αβ a β β a β β a β (n 1) β = a αβ, whence 5

7 a αβ = e iϕ αβ with ϕ αβ = φ α φ β a ranom phase. Similarly for the corresponing relevant frequencies, the relation ω αβ + ω β β ω β (n 1) β = ω αβ applies, which means that ω αβ is of the form ω αβ = Ω α Ω β. (28) As a result of these properties, the coefficients in the above expansions satisfy a matrix algebra; thus, for instance, if ˆx is the matrix with elements x αβ, we have (x n ) α = β ( x n ) αβ a αβ e iω αβt, (29) with ( x n ) αβ given by the element αβ of the corresponing matrix prouct, ( x n ) αβ = (ˆx n ) αβ. It is clear that the time-epenence of x α (t) can be transferre to every single factor x αβ, so that the evolving matrix ˆx(t) has as elements the coefficients x αβ e iω αβt. This allows to write the equation satisfie by the stationary solutions in the form m 2ˆx(t) t 2 = ˆf(t) + mτ 3ˆx(t) t 3 + eê(t). (30) In the raiationless approximation, the last two terms are neglecte an one is left with m 2ˆx(t) t 2 = ˆf(t). (31) With these results one may construct the law of evolution for the matrix Â(t) associate with the (generic) ynamical variable A; the outcome is i Â(t) t = [Â(t), ˆΩ], (32) with the matrix elements of ˆΩ given by Ω αβ = Ω α δ αβ. Notice that, as with the previous erivation presente in section 2.2, the raiationless approximation has elete any explicit trace of the zpf. No stochastic variable is containe in equations (30)-(32); instea, they are expresse in terms of operators. In section 2.3, the missing value of the paramerter η in equation (12) was obtaine by imposing the energy-balance conition; this le unequivocally to the Schröinger equation (20). In the present case, it is again the scale of the solution what is missing in equation (32). The loss is repaire by, first, fining that the canonical commutator [ˆx, ˆp], with ˆp = m ˆx(t) t = im [ ˆx(t), ˆΩ ], (33) has the universal form [ˆx, ˆp] = CI, with C constant, an, secon, fining the value of C. This is reaily achieve by applying the above equations to the harmonic oscillator of natural frequency ω 0 in its groun state, when it is in equilibrium with the zpf moe of the same frequency. One thus obtains C = i, whence [ˆx, ˆp] = i I. (34) The value of the commutator represents therefore a irect measure of the intensity of the fluctuations impresse upon the particle by the zpf, just as was conclue in section 2.3. Finally, from the above results it can be reaily seen that the relevant frequencies are given by ω αβ = Ω α Ω β = 1 (E α E β ), (35) where E α is the eigenvalue of the Hamiltonian in state α, an the final form of equation (32) is therefore i Â(t) = [Â(t), Ĥ], (36) t i. e., the Heisenberg equation for the operator Â(t). 6

8 3. Revealing the spin of the electron To isclose the rotational effect of the zpf on the particle, let us briefly go back to the original (stochastic) equation of motion (1) an rewrite it as ṗ = f + mτ... x + ee(t), (37) where p = mẋ. We shall consier that there is no external torque; the (central) force can then be written as f = g(r)x, r = x. By taking the vector prouct of this equation with x we get... L = x ṗ = mτx x + ex E, (38) t which gives the instantaneous change of the angular-momentum ue to the torque exerte by both raiation reaction an the ranom zpf. The average of this expression over the fiel realizations is t L(i) = mτ(x... x) (i) + e(x E) (i). (39) Since in the quantum regime the ynamical variables satisfy the conition of ergoicity, accoring to our iscussion in section 2.4, this equation is equivalent to (21). Equation (39), however, has the avantage of allowing us to irectly ientify the last term as the effective torque exerte by the Lorentz force of the zpf on the particle. For the angular momentum to be conserve, we must have (compare with equation (22)) mτ(x... x) (i) = e(x E) (i). (40) Let us assume that the system is in its groun state, so that there is no orbital angular momentum. Making the usual substitution ṗ f (which is vali to zero orer in τ e 2 ) an writing f as g(r)x, we get explicitly τg(r)l (i) 0 = me (x E) (i) 0. (41) Since only the fluctuating component of x can contribute to the average (x E) (i) (because E(t) is purely ranom), it is clear that all the angular momentum thus generate is ue to the ranom motion aroun the mean trajectory followe by the particle; thus, it is inepenent of the system of coorinates, an has an internal nature, usualy taken as intrinsic The electron s intrinsic angular momentum The above iscussion suggests looking for a proceure that can bring to the surface the intrinsic angular momentum acquire by the electron through its interaction with the zpf. For this purpose we recall the experimental observation that the interaction of the electron with the raiation fiel takes place via the circular polarize moes of the fiel (or moes of a certain helicity). This is known to be the case for the photonic fiel, which, from the perspective of se, is the excite state of the raiation fiel, aitional to the zero-point component. Now, it is natural to assume that the moes of the fiel in its groun state, i. e., of the zpf, interact in a similar way with the electron. To analyze the effect of such interaction, we shoul therefore consier the zpf as compose of moes of both right- an left-hane circular polarization. When the ensemble of fiel moes is consiere in its entirety, as is usually one, any such effect is conceale; yet by focusing on one of the two subensembles of a given polarization, the effective rotation inuce on the corresponing particles shoul be isclose. Let us therefore consier a situation in which the particle is in a stationary state, uner the action of the backgroun fiel of a given circular polarization with respect to an axis k. To start 7

9 with, we shall consier the particle in its groun state, so as to ensure that there is no orbital angular momentum. We therefore take L 0 = 0 (ˆx i ˆp j ˆx j ˆp i ) 0 (42) an analyze separately the contributions arising from each of the two circular polarizations, characterize by the (circularly polarize) vectors ɛ k± = 1 2 (ɛ ki ± iɛ kj ), (43) with ɛ ki, ɛ kj unit Cartesian vectors orthogonal to the axis k. Since accoring to the results reporte in section 2.4, the response of the particle to the fiel is linear, to escribe its motion uner the action of a circular fiel moe one shoul write the variable x in cylinrical coorinates, i. e. x = x + ɛ k+ + x ɛ k + x kˆk, with x ± = 1 2 (x i ix j ), x i = 1 2 ( x + + x ), x j = i 1 2 ( x + x ). (44a) (44b) Taking into account that x ± n0 = ( x 0n), equation (42) becomes explicitly L 0 = m n ( ω n0 x + 0n x n0 ) ( x 0n x+ n0 = m ω n0 x + 2 0n x 2) 0n. (45) In the groun state, L 0 = 0; hence the two sums on the right-han sie contribute with equal magnitue an opposite sign to the k-component of the total angular momentum, as shoul be the case for a nonpolarize vacuum. Taken separately, these contributions are L + 0 = m ω n0 x + 2 0n, L 0 = m ω n0 x 2 0n. (46) n n n Since, on the other han, the mean value of the commutator (34) gives the sum rule m n ω n0 x ± 0n 2 = 2, (47) the size of each separate contribution to (45) is just /2. In orer to istinguish these contributions from the (orbital) component of the angular momentum we write S ± instea of L ± 0 ; thus L 0 = S + + S, with S ± = ± 2. (48) Direct calculation of the square of the angular momentum, using (24), is more cumbersome. As a simple expeient, let us carry out this calculation for the isotropic harmonic oscillator in its groun state. The (raiationless) approximation ṗ i = f i allows us to write in this case m... x i = ω0 2p i. Further, since L 2 = x 2 p 2 (x p) 2, we have p i L 2 p i = 2L 2, 2 L 2 p i p i = 4x 2, With these results equation (24) transforms into 2 L 2 x i p i = 0. L 2 0 = mc3 D pp e 2 ω0 2 x 2 0, (49) 8

10 with D pp given by equation (11). Now in the case of the harmonic oscillator, using equations (2), (4) an (19) we obtain a constant value for the iffusion coefficient, D pp = e2 ω 3 0 c 3, (50) whence using x 2 0 = 3ˆx 2 0 = 3 /(2mω 0 ), equation (49) becomes finally L 2 0 = m ω 0 x 2 0 = (51) This result was obtaine for the first time by Marshall in 1965 [15], an taken as an aitional contribution to the orbital angular momentum ue to the zpf. In [9] the same result was obtaine, but interprete as an intrinsic (spin) angular momentum of ouble the correct value. However, in line with the present approach, we separate again the full ensemble into two subensembles corresponing to the ifferent circular polarizations, thus obtaining L 2 0 = L L 2 0, (52) with each partial contribution to the mean square angular momentum given by L = L 2 0 = (53) Using the notation introuce above (see equation (48)), which ientifies this as an intrinsic angular momentum, we write S 2 + = S 2 = (54) The fact that this result oes not epen on the oscillator s frequency ω 0, suggests that it hols in the general case, an for the free particle in particular. Therefore, we conclue that when the transformation (44) possesses physical meaning, so that the ecompositions L 0 = L L 0 an L = L L 2 make sense, equations (48) an (54) 0 tell us that there exists an angular momentum that oes not correspon to an orbital motion of the particle an can therefore be consiere as intrinsic. For an electron, which (as state above) interacts with the raiation fiel via its circular polarize moes, the transformation (44) is inee physically meaningful, an the angular momentum thus inuce can therefore be ientifie with its spin General erivation of the spin angular momentum In the preceing section we have isclose the existence of the spin angular momentum for an electron in its groun state. Let us now exten our analysis to the general case, incluing excite states with orbital angular momentum. Accoring to the above iscussion, we shoul separate the contributions to the angular momentum arising from the two circular polarizations of the fiel. Denoting with the inex n (or k) the set of quantum numbers that characterize a state of the particle, incluing the orbital angular momentum an its projection along the z-axis, we have (for simplicity in the writing we use x i = x, x j = y, an x k = z) ˆLz n = n ˆL z n = k (x nkp ykn y nk p xkn ) = = im k ω kn (x nk y kn y nk x kn ). (55) 9

11 Uner the same proceure that le to (45), equation (55) transforms into ˆLz = m ( ω kn x + 2 n k nk x 2) nk. (56) This expression can be rewritten as with O z σ n given by (σ = ±) O ˆLz n = O z + n + O z n, (57) z σ n = σm k ω kn x σ nk 2. (58) Using again the sum rule m k ω kn x nk 2 = m k ω kn y nk 2 = 1 2, one obtains from (58) = m ( ω kn x + 2 k nk + x 2) nk = O z + n O z n, (59) which combine with (57) gives O z σ n = 1 2 ˆLz + σ 1 n 2. (60) This quantity O z σ n contains, for every polarization state σ, both the corresponing part of the orbital angular momentum, an the spin associate with that state. To construct the operator associate with the vector S introuce in section 3.1, we observe that the mean value ˆL z n oes not epen on σ, whereas the term σ /2 oes not epen on n. This inicates that the operator ˆL z an the operator to be associate with σ /2 (which we shall call ˆΣ z ) belong to ifferent Hilbert spaces. In orer to express O z σ n as the average of an operator, we must therefore exten the Hilbert space to inclue the ichotomous variable σ in aition to the quantum inex n. The result is the prouct space H = H n H 2, with H 2 a biimensional vector space spanne by an orthonormal basis having as elements the vectors { σ} = { +, }. In terms of nσ = n σ, equation (60) rewrites as with ˆΣ z an operator that has σ as eigenvector, Expressing ˆΣ z in terms of the Pauli matrices gives O z σ n = 1 2 nσ ˆL z nσ nσ ˆΣ z nσ, (61) nσ ˆΣ z nσ = σ ˆΣ z σ = σ. (62) ˆΣ z = a 0 I + a z ˆσ z + a +ˆσ + + a ˆσ, (63) where a ± = (a x ia y ) / 2, an ˆσ + = 2 +, ˆσ = 2 + are laer operators. Conition (62) impose on ˆΣ z gives a 0 = 0, a z = 1. Further, since we are here consiering the variables (x +, x, z), the polarization vectors (43) fix ẑ as the preferre axis, whence a ± = 0, ˆΣ z = ˆσ z, an equation (61) becomes ( O z σ n = nσ 1 ˆL ) 2 + Ŝ ẑ nσ, (64) with Ŝ the vector operator efine as Ŝ z = 1 2 ˆΣ z, i.e., Ŝ = 1 2 ˆσ. (65) 10

12 The ientification of the operator Ŝ with the spin of the electron is thus justifie. The inepenence of ˆL z n from σ an of ˆΣ z from n, inicates that uner the present conitions, the fluctuations associate with the spin are not correlate with those that characterize the kinematics of the particle in the configuration space: L an S constitute inepenent ynamical variables. Of course the spaces of the spin an the orbital angular momentum may become connecte by the presence of magnetic fiels. It shoul be stresse that even if ˆL an Ŝ are combine uner one expression for the angular motions, e. g. equation (64), the spin is not an orbital angular momentum. Inee, there are funamental ifferences between ˆL an Ŝ. In particular, the mean value of ˆL z, say, can be freely etermine by ajusting external parameters, an may acquire a whole spectrum of values. However, only the sign of the projection Ŝz can be subject to external ajustment; its absolute value is etermine by the funamental commutator, which in its turn is fixe by the zpf. It is because of the universal value of the commutator that the spin of the electron is the same for all electrons uner all circumstances, which reinforces its intrinsic nature. The connection of the commutator [ˆx, ˆp x ] = i with the spin of the electron eserves a further comment. As pointe out in previous sections, Planck s constant is a irect measure of the size of the fluctuations, both those of the zpf an those impresse by it on the particle. Specifically, since the commutator implies that the fluctuations of x an p x have a minimum value ajuste to the rule σxσ 2 p 2 min x = 2 /4 (σx, 2 σp 2 x are variances), one may write the numerical relation ± Ŝz ± = /2 = σ x σ px min, which emphasizes the fact that the value of the electron spin is etermine by the irreucible fluctuations of the phase-space variables x, p x aroun the instantaneous position of the particle The spin gyromagnetic factor It was iscovere experimentally that the g-factor associate with the spin magnetic moment of the electron has an approximate value g S = 2, whereas for the orbital magnetic moment the g-factor is g L = 1. This characteristic value of g S is incorporate into nonrelativistic quantum theory by han, usually without further elaboration. The issue is normally resolve by resorting to the Dirac equation, which preicts g S = 2. Given that the present theory prouces the electron spin, it seems appropriate to investigate the value preicte by it for g S. For this purpose consier the electron acte on, in aition to the external force f(x), by a static uniform magnetic fiel B = Bẑ. The contribution of the orbital angular momentum L to the Hamiltonian is given by Ĥ = ˆµ B = µ z B, (66) where ˆµ = (g L µ 0 ˆL)/ is the magnetic moment ue to ˆL, µ 0 = e /(2mc) is the Bohr magneton (with e = e ), an g L = 1. Therefore the mean energy is E = µ 0 BˆL z. (67) Consier now a situation in which the spin projection along ẑ has a well-efine value, say Ŝz = + /2. This means that one shoul consier only the subensemble that correspons to σ = +. Resorting to equation (60) to write the corresponing contribution to L z as (ˆL z + )/2, the component of E of interest is E + = µ 0B ( 1 2 ˆL z + 2 ) = µ 0B ( ) ˆL z + Ŝz. (68) An analogous result hols for the subensemble with σ =, for which Ŝz = /2, E = µ ( 0B 1 2 ˆL z ) = µ ( ) 0B ˆL z + Ŝz. (69) 11

13 The corresponing Hamiltonian escribing the total magnetic interaction of the electron follows from the sum of these contributions; it is therefore Ĥ LS = µ 0B (ˆLz + 2Ŝz). (70) This contains the correct g-factor of 2 for the spin of the electron, in the raiationless approximation. It is clear from the erivation that this value is etermine by the two egrees of freeom associate with the polarization of the zpf. Notice that the result (70) gives a precise meaning to the operator appearing in equation (64). Inee, from this latter equation we can write Ô = (ˆL + 2Ŝ)/2, whence Ĥ LS = µ 0 B (ˆL + 2Ŝ ) = ˆµ B, (71) with ˆµ = 2µ 0 Ô, which irectly relates Ô with the total magnetic-moment operator of the atomic electron. 4. Final remarks The present results give strong support to the representation of the electron spin as an acquire angular momentum. They reaffirm the image, suggeste in previous se work, of spin as a helicoial motion aroun the local mean path followe by the particle, prouce by the highfrequency (circular polarize) moes of the fluctuating vacuum. If, accoring to the results presente, a charge particle acquires spin 1/2, the question arises as to whether a similar effect shouln t be expecte to appear in the case of scalar bosons. A possible answer to this question is that the spin 1/2 is acquire by elementary particles, such as the electron, whereas composite particles may acquire it or not, epening on their internal structure. This suggests that bosons are in general composite structures, with an even number of elements (if of fermion type). Acknowlegments This work was supporte by DGAPA-UNAM through project PAPIIT IN References [1] A. M. Cetto, L. e la Peña an A. Valés-Hernánez, J. Phys. JPCS 361 (2012) an references therein; L. e la Peña, A. M. Cetto an A. Valés-Hernánez, Int. J. Moern Phys. A (to be publishe). [2] A. M. Cetto an L. e la Peña, Phys. Scripta T151 (2002) ; A. M. Cetto, L. e la Peña an A. Valés-Hernánez, Rev. Mex. Fis. 59 (2013) 433; arxiv: (quant-ph), 26 Jan [3] A. Valés-Hernánez, Investigación el origen el enreamiento cuántico ese la perspectiva e la electroinámica estocástica lineal, Ph. D. thesis, UNAM (Mexico, 2010); A. Valés-Hernánez, L. e la Peña an A. M. Cetto, Foun. Physics 41 (2011) 843. [4] L. e la Peña an A. M. Cetto, The Quantum Dice (Kluwer, Dorrecht, 1996) an references therein. [5] P. Braffort an A. Taroni, C. R. Aca. Sc. Paris 264 (1967) [6] S. M. Moore an J. A. Ramírez, Lett. Nuovo Cim. 33 (1982) 87; S. M. Moore, Lett. Nuovo Cim. 40 (1984) 385. [7] G. Cavalleri, Lett. Nuovo Cim. 43 (1985) 285. [8] A. Ruea, Foun. Phys. Lett. 6 (1993) 139. [9] A. Jáuregui an L. e la Peña, Phys. Lett. A, 86 (1981) 280; L. e la Peña an A. Jáuregui, Foun. Phys. 12 (1982) 441. [10] A. Barranco, S. A. Brunini an H. M. Franca, Phys. Rev. A 39 (1989), [11] D. Hestenes, Foun. Phys. 15 (1985) 63. [12] K. Muralihar, Apeyron 18 (2011) 146. [13] K. Huang, Am. J. Phys. 20 (1952) 479. [14] U. Frisch, in Probabilistic Methos in Applie Mathematics, vol. I, A. T. Barucha-Rei, e. (Acaemic Press, NY, 1968); see also L. e la Peña an A. M. Cetto, J. Math. Phys. 18 (1977) [15] T. W. Marshall, Nuovo Cim. 38 (1965)

Schrödinger s equation.

Schrödinger s equation. Physics 342 Lecture 5 Schröinger s Equation Lecture 5 Physics 342 Quantum Mechanics I Wenesay, February 3r, 2010 Toay we iscuss Schröinger s equation an show that it supports the basic interpretation of

More information

ensembles When working with density operators, we can use this connection to define a generalized Bloch vector: v x Tr x, v y Tr y

ensembles When working with density operators, we can use this connection to define a generalized Bloch vector: v x Tr x, v y Tr y Ph195a lecture notes, 1/3/01 Density operators for spin- 1 ensembles So far in our iscussion of spin- 1 systems, we have restricte our attention to the case of pure states an Hamiltonian evolution. Toay

More information

4. Important theorems in quantum mechanics

4. Important theorems in quantum mechanics TFY4215 Kjemisk fysikk og kvantemekanikk - Tillegg 4 1 TILLEGG 4 4. Important theorems in quantum mechanics Before attacking three-imensional potentials in the next chapter, we shall in chapter 4 of this

More information

Chapter 6: Energy-Momentum Tensors

Chapter 6: Energy-Momentum Tensors 49 Chapter 6: Energy-Momentum Tensors This chapter outlines the general theory of energy an momentum conservation in terms of energy-momentum tensors, then applies these ieas to the case of Bohm's moel.

More information

PHYS 414 Problem Set 2: Turtles all the way down

PHYS 414 Problem Set 2: Turtles all the way down PHYS 414 Problem Set 2: Turtles all the way own This problem set explores the common structure of ynamical theories in statistical physics as you pass from one length an time scale to another. Brownian

More information

Lecture 2 Lagrangian formulation of classical mechanics Mechanics

Lecture 2 Lagrangian formulation of classical mechanics Mechanics Lecture Lagrangian formulation of classical mechanics 70.00 Mechanics Principle of stationary action MATH-GA To specify a motion uniquely in classical mechanics, it suffices to give, at some time t 0,

More information

Conservation Laws. Chapter Conservation of Energy

Conservation Laws. Chapter Conservation of Energy 20 Chapter 3 Conservation Laws In orer to check the physical consistency of the above set of equations governing Maxwell-Lorentz electroynamics [(2.10) an (2.12) or (1.65) an (1.68)], we examine the action

More information

Quantum mechanical approaches to the virial

Quantum mechanical approaches to the virial Quantum mechanical approaches to the virial S.LeBohec Department of Physics an Astronomy, University of Utah, Salt Lae City, UT 84112, USA Date: June 30 th 2015 In this note, we approach the virial from

More information

1 Heisenberg Representation

1 Heisenberg Representation 1 Heisenberg Representation What we have been ealing with so far is calle the Schröinger representation. In this representation, operators are constants an all the time epenence is carrie by the states.

More information

arxiv: v1 [physics.class-ph] 20 Dec 2017

arxiv: v1 [physics.class-ph] 20 Dec 2017 arxiv:1712.07328v1 [physics.class-ph] 20 Dec 2017 Demystifying the constancy of the Ermakov-Lewis invariant for a time epenent oscillator T. Pamanabhan IUCAA, Post Bag 4, Ganeshkhin, Pune - 411 007, Inia.

More information

Ana María Cetto, Luis de la Peña and Andrea Valdés Hernández

Ana María Cetto, Luis de la Peña and Andrea Valdés Hernández Ana María Cetto, Luis de la Peña and Andrea Valdés Hernández Instituto de Física, UNAM EmQM13, Vienna, 3-6 October 2013 1 Planck's law as a consequence of the zero-point field Equilibrium radiation field

More information

Solution to the exam in TFY4230 STATISTICAL PHYSICS Wednesday december 1, 2010

Solution to the exam in TFY4230 STATISTICAL PHYSICS Wednesday december 1, 2010 NTNU Page of 6 Institutt for fysikk Fakultet for fysikk, informatikk og matematikk This solution consists of 6 pages. Solution to the exam in TFY423 STATISTICAL PHYSICS Wenesay ecember, 2 Problem. Particles

More information

The Ehrenfest Theorems

The Ehrenfest Theorems The Ehrenfest Theorems Robert Gilmore Classical Preliminaries A classical system with n egrees of freeom is escribe by n secon orer orinary ifferential equations on the configuration space (n inepenent

More information

The Principle of Least Action

The Principle of Least Action Chapter 7. The Principle of Least Action 7.1 Force Methos vs. Energy Methos We have so far stuie two istinct ways of analyzing physics problems: force methos, basically consisting of the application of

More information

Introduction to the Vlasov-Poisson system

Introduction to the Vlasov-Poisson system Introuction to the Vlasov-Poisson system Simone Calogero 1 The Vlasov equation Consier a particle with mass m > 0. Let x(t) R 3 enote the position of the particle at time t R an v(t) = ẋ(t) = x(t)/t its

More information

Chapter 2 Lagrangian Modeling

Chapter 2 Lagrangian Modeling Chapter 2 Lagrangian Moeling The basic laws of physics are use to moel every system whether it is electrical, mechanical, hyraulic, or any other energy omain. In mechanics, Newton s laws of motion provie

More information

Quantum Mechanics in Three Dimensions

Quantum Mechanics in Three Dimensions Physics 342 Lecture 20 Quantum Mechanics in Three Dimensions Lecture 20 Physics 342 Quantum Mechanics I Monay, March 24th, 2008 We begin our spherical solutions with the simplest possible case zero potential.

More information

Physics 5153 Classical Mechanics. The Virial Theorem and The Poisson Bracket-1

Physics 5153 Classical Mechanics. The Virial Theorem and The Poisson Bracket-1 Physics 5153 Classical Mechanics The Virial Theorem an The Poisson Bracket 1 Introuction In this lecture we will consier two applications of the Hamiltonian. The first, the Virial Theorem, applies to systems

More information

'HVLJQ &RQVLGHUDWLRQ LQ 0DWHULDO 6HOHFWLRQ 'HVLJQ 6HQVLWLYLW\,1752'8&7,21

'HVLJQ &RQVLGHUDWLRQ LQ 0DWHULDO 6HOHFWLRQ 'HVLJQ 6HQVLWLYLW\,1752'8&7,21 Large amping in a structural material may be either esirable or unesirable, epening on the engineering application at han. For example, amping is a esirable property to the esigner concerne with limiting

More information

1 dx. where is a large constant, i.e., 1, (7.6) and Px is of the order of unity. Indeed, if px is given by (7.5), the inequality (7.

1 dx. where is a large constant, i.e., 1, (7.6) and Px is of the order of unity. Indeed, if px is given by (7.5), the inequality (7. Lectures Nine an Ten The WKB Approximation The WKB metho is a powerful tool to obtain solutions for many physical problems It is generally applicable to problems of wave propagation in which the frequency

More information

Survey Sampling. 1 Design-based Inference. Kosuke Imai Department of Politics, Princeton University. February 19, 2013

Survey Sampling. 1 Design-based Inference. Kosuke Imai Department of Politics, Princeton University. February 19, 2013 Survey Sampling Kosuke Imai Department of Politics, Princeton University February 19, 2013 Survey sampling is one of the most commonly use ata collection methos for social scientists. We begin by escribing

More information

Free rotation of a rigid body 1 D. E. Soper 2 University of Oregon Physics 611, Theoretical Mechanics 5 November 2012

Free rotation of a rigid body 1 D. E. Soper 2 University of Oregon Physics 611, Theoretical Mechanics 5 November 2012 Free rotation of a rigi boy 1 D. E. Soper 2 University of Oregon Physics 611, Theoretical Mechanics 5 November 2012 1 Introuction In this section, we escribe the motion of a rigi boy that is free to rotate

More information

THE VAN KAMPEN EXPANSION FOR LINKED DUFFING LINEAR OSCILLATORS EXCITED BY COLORED NOISE

THE VAN KAMPEN EXPANSION FOR LINKED DUFFING LINEAR OSCILLATORS EXCITED BY COLORED NOISE Journal of Soun an Vibration (1996) 191(3), 397 414 THE VAN KAMPEN EXPANSION FOR LINKED DUFFING LINEAR OSCILLATORS EXCITED BY COLORED NOISE E. M. WEINSTEIN Galaxy Scientific Corporation, 2500 English Creek

More information

Separation of Variables

Separation of Variables Physics 342 Lecture 1 Separation of Variables Lecture 1 Physics 342 Quantum Mechanics I Monay, January 25th, 2010 There are three basic mathematical tools we nee, an then we can begin working on the physical

More information

Physics 115C Homework 4

Physics 115C Homework 4 Physics 115C Homework 4 Problem 1 a In the Heisenberg picture, the ynamical equation is the Heisenberg equation of motion: for any operator Q H, we have Q H = 1 t i [Q H,H]+ Q H t where the partial erivative

More information

6 General properties of an autonomous system of two first order ODE

6 General properties of an autonomous system of two first order ODE 6 General properties of an autonomous system of two first orer ODE Here we embark on stuying the autonomous system of two first orer ifferential equations of the form ẋ 1 = f 1 (, x 2 ), ẋ 2 = f 2 (, x

More information

Semiclassical analysis of long-wavelength multiphoton processes: The Rydberg atom

Semiclassical analysis of long-wavelength multiphoton processes: The Rydberg atom PHYSICAL REVIEW A 69, 063409 (2004) Semiclassical analysis of long-wavelength multiphoton processes: The Ryberg atom Luz V. Vela-Arevalo* an Ronal F. Fox Center for Nonlinear Sciences an School of Physics,

More information

QUANTUMMECHANICAL BEHAVIOUR IN A DETERMINISTIC MODEL. G. t Hooft

QUANTUMMECHANICAL BEHAVIOUR IN A DETERMINISTIC MODEL. G. t Hooft QUANTUMMECHANICAL BEHAVIOUR IN A DETERMINISTIC MODEL G. t Hooft Institute for Theoretical Physics University of Utrecht, P.O.Box 80 006 3508 TA Utrecht, the Netherlans e-mail: g.thooft@fys.ruu.nl THU-96/39

More information

Chapter 4. Electrostatics of Macroscopic Media

Chapter 4. Electrostatics of Macroscopic Media Chapter 4. Electrostatics of Macroscopic Meia 4.1 Multipole Expansion Approximate potentials at large istances 3 x' x' (x') x x' x x Fig 4.1 We consier the potential in the far-fiel region (see Fig. 4.1

More information

Table of Common Derivatives By David Abraham

Table of Common Derivatives By David Abraham Prouct an Quotient Rules: Table of Common Derivatives By Davi Abraham [ f ( g( ] = [ f ( ] g( + f ( [ g( ] f ( = g( [ f ( ] g( g( f ( [ g( ] Trigonometric Functions: sin( = cos( cos( = sin( tan( = sec

More information

A simple model for the small-strain behaviour of soils

A simple model for the small-strain behaviour of soils A simple moel for the small-strain behaviour of soils José Jorge Naer Department of Structural an Geotechnical ngineering, Polytechnic School, University of São Paulo 05508-900, São Paulo, Brazil, e-mail:

More information

involve: 1. Treatment of a decaying particle. 2. Superposition of states with different masses.

involve: 1. Treatment of a decaying particle. 2. Superposition of states with different masses. Physics 195a Course Notes The K 0 : An Interesting Example of a Two-State System 021029 F. Porter 1 Introuction An example of a two-state system is consiere. involve: 1. Treatment of a ecaying particle.

More information

Euler equations for multiple integrals

Euler equations for multiple integrals Euler equations for multiple integrals January 22, 2013 Contents 1 Reminer of multivariable calculus 2 1.1 Vector ifferentiation......................... 2 1.2 Matrix ifferentiation........................

More information

Lecture XVI: Symmetrical spacetimes

Lecture XVI: Symmetrical spacetimes Lecture XVI: Symmetrical spacetimes Christopher M. Hirata Caltech M/C 350-17, Pasaena CA 91125, USA (Date: January 4, 2012) I. OVERVIEW Our principal concern this term will be symmetrical solutions of

More information

u t v t v t c a u t b a v t u t v t b a

u t v t v t c a u t b a v t u t v t b a Nonlinear Dynamical Systems In orer to iscuss nonlinear ynamical systems, we must first consier linear ynamical systems. Linear ynamical systems are just systems of linear equations like we have been stuying

More information

CHM 532 Notes on Creation and Annihilation Operators

CHM 532 Notes on Creation and Annihilation Operators CHM 53 Notes on Creation an Annihilation Operators These notes provie the etails concerning the solution to the quantum harmonic oscillator problem using the algebraic metho iscusse in class. The operators

More information

arxiv: v1 [physics.flu-dyn] 8 May 2014

arxiv: v1 [physics.flu-dyn] 8 May 2014 Energetics of a flui uner the Boussinesq approximation arxiv:1405.1921v1 [physics.flu-yn] 8 May 2014 Kiyoshi Maruyama Department of Earth an Ocean Sciences, National Defense Acaemy, Yokosuka, Kanagawa

More information

A Model of Electron-Positron Pair Formation

A Model of Electron-Positron Pair Formation Volume PROGRESS IN PHYSICS January, 8 A Moel of Electron-Positron Pair Formation Bo Lehnert Alfvén Laboratory, Royal Institute of Technology, S-44 Stockholm, Sween E-mail: Bo.Lehnert@ee.kth.se The elementary

More information

arxiv: v1 [gr-qc] 24 Jan 2019

arxiv: v1 [gr-qc] 24 Jan 2019 A moment approach to compute quantum-gravity effects in the primorial universe Davi Brizuela 1 an Unai Muniain Fisika Teorikoa eta Zientziaren Historia Saila, UPV/EHU, 644 P.K., 48080 Bilbao, Spain arxiv:1901.08391v1

More information

Math 342 Partial Differential Equations «Viktor Grigoryan

Math 342 Partial Differential Equations «Viktor Grigoryan Math 342 Partial Differential Equations «Viktor Grigoryan 6 Wave equation: solution In this lecture we will solve the wave equation on the entire real line x R. This correspons to a string of infinite

More information

Spectral Flow, the Magnus Force, and the. Josephson-Anderson Relation

Spectral Flow, the Magnus Force, and the. Josephson-Anderson Relation Spectral Flow, the Magnus Force, an the arxiv:con-mat/9602094v1 16 Feb 1996 Josephson-Anerson Relation P. Ao Department of Theoretical Physics Umeå University, S-901 87, Umeå, SWEDEN October 18, 2018 Abstract

More information

Hyperbolic Moment Equations Using Quadrature-Based Projection Methods

Hyperbolic Moment Equations Using Quadrature-Based Projection Methods Hyperbolic Moment Equations Using Quarature-Base Projection Methos J. Koellermeier an M. Torrilhon Department of Mathematics, RWTH Aachen University, Aachen, Germany Abstract. Kinetic equations like the

More information

Slide10 Haykin Chapter 14: Neurodynamics (3rd Ed. Chapter 13)

Slide10 Haykin Chapter 14: Neurodynamics (3rd Ed. Chapter 13) Slie10 Haykin Chapter 14: Neuroynamics (3r E. Chapter 13) CPSC 636-600 Instructor: Yoonsuck Choe Spring 2012 Neural Networks with Temporal Behavior Inclusion of feeback gives temporal characteristics to

More information

NOTES ON EULER-BOOLE SUMMATION (1) f (l 1) (n) f (l 1) (m) + ( 1)k 1 k! B k (y) f (k) (y) dy,

NOTES ON EULER-BOOLE SUMMATION (1) f (l 1) (n) f (l 1) (m) + ( 1)k 1 k! B k (y) f (k) (y) dy, NOTES ON EULER-BOOLE SUMMATION JONATHAN M BORWEIN, NEIL J CALKIN, AND DANTE MANNA Abstract We stuy a connection between Euler-MacLaurin Summation an Boole Summation suggeste in an AMM note from 196, which

More information

05 The Continuum Limit and the Wave Equation

05 The Continuum Limit and the Wave Equation Utah State University DigitalCommons@USU Founations of Wave Phenomena Physics, Department of 1-1-2004 05 The Continuum Limit an the Wave Equation Charles G. Torre Department of Physics, Utah State University,

More information

6. Friction and viscosity in gasses

6. Friction and viscosity in gasses IR2 6. Friction an viscosity in gasses 6.1 Introuction Similar to fluis, also for laminar flowing gases Newtons s friction law hols true (see experiment IR1). Using Newton s law the viscosity of air uner

More information

Survival Facts from Quantum Mechanics

Survival Facts from Quantum Mechanics Survival Facts from Quantum Mechanics Operators, Eigenvalues an Eigenfunctions An operator O may be thought as something that operates on a function to prouce another function. We enote operators with

More information

Problem Set 6: Workbook on Operators, and Dirac Notation Solution

Problem Set 6: Workbook on Operators, and Dirac Notation Solution Moern Physics: Home work 5 Due ate: 0 March. 014 Problem Set 6: Workbook on Operators, an Dirac Notation Solution 1. nswer 1: a The cat is being escribe by the state, ψ >= ea > If we try to observe it

More information

Math Notes on differentials, the Chain Rule, gradients, directional derivative, and normal vectors

Math Notes on differentials, the Chain Rule, gradients, directional derivative, and normal vectors Math 18.02 Notes on ifferentials, the Chain Rule, graients, irectional erivative, an normal vectors Tangent plane an linear approximation We efine the partial erivatives of f( xy, ) as follows: f f( x+

More information

Lagrangian and Hamiltonian Dynamics

Lagrangian and Hamiltonian Dynamics Lagrangian an Hamiltonian Dynamics Volker Perlick (Lancaster University) Lecture 1 The Passage from Newtonian to Lagrangian Dynamics (Cockcroft Institute, 22 February 2010) Subjects covere Lecture 2: Discussion

More information

Quantum optics of a Bose-Einstein condensate coupled to a quantized light field

Quantum optics of a Bose-Einstein condensate coupled to a quantized light field PHYSICAL REVIEW A VOLUME 60, NUMBER 2 AUGUST 1999 Quantum optics of a Bose-Einstein conensate couple to a quantize light fiel M. G. Moore, O. Zobay, an P. Meystre Optical Sciences Center an Department

More information

Lagrangian and Hamiltonian Mechanics

Lagrangian and Hamiltonian Mechanics Lagrangian an Hamiltonian Mechanics.G. Simpson, Ph.. epartment of Physical Sciences an Engineering Prince George s Community College ecember 5, 007 Introuction In this course we have been stuying classical

More information

Introduction to Markov Processes

Introduction to Markov Processes Introuction to Markov Processes Connexions moule m44014 Zzis law Gustav) Meglicki, Jr Office of the VP for Information Technology Iniana University RCS: Section-2.tex,v 1.24 2012/12/21 18:03:08 gustav

More information

The derivative of a function f(x) is another function, defined in terms of a limiting expression: f(x + δx) f(x)

The derivative of a function f(x) is another function, defined in terms of a limiting expression: f(x + δx) f(x) Y. D. Chong (2016) MH2801: Complex Methos for the Sciences 1. Derivatives The erivative of a function f(x) is another function, efine in terms of a limiting expression: f (x) f (x) lim x δx 0 f(x + δx)

More information

Can we derive Newton s F = ma from the SE?

Can we derive Newton s F = ma from the SE? 8.04 Quantum Physics Lecture XIII p = pˆ (13-1) ( ( ) ) = xψ Ψ (13-) ( ) = xψ Ψ (13-3) [ ] = x (ΨΨ ) Ψ Ψ (13-4) ( ) = xψ Ψ (13-5) = p, (13-6) where again we have use integration by parts an the fact that

More information

How the potentials in different gauges yield the same retarded electric and magnetic fields

How the potentials in different gauges yield the same retarded electric and magnetic fields How the potentials in ifferent gauges yiel the same retare electric an magnetic fiels José A. Heras a Departamento e Física, E. S. F. M., Instituto Politécnico Nacional, México D. F. México an Department

More information

Sources and Sinks of Available Potential Energy in a Moist Atmosphere. Olivier Pauluis 1. Courant Institute of Mathematical Sciences

Sources and Sinks of Available Potential Energy in a Moist Atmosphere. Olivier Pauluis 1. Courant Institute of Mathematical Sciences Sources an Sinks of Available Potential Energy in a Moist Atmosphere Olivier Pauluis 1 Courant Institute of Mathematical Sciences New York University Submitte to the Journal of the Atmospheric Sciences

More information

LATTICE-BASED D-OPTIMUM DESIGN FOR FOURIER REGRESSION

LATTICE-BASED D-OPTIMUM DESIGN FOR FOURIER REGRESSION The Annals of Statistics 1997, Vol. 25, No. 6, 2313 2327 LATTICE-BASED D-OPTIMUM DESIGN FOR FOURIER REGRESSION By Eva Riccomagno, 1 Rainer Schwabe 2 an Henry P. Wynn 1 University of Warwick, Technische

More information

and from it produce the action integral whose variation we set to zero:

and from it produce the action integral whose variation we set to zero: Lagrange Multipliers Monay, 6 September 01 Sometimes it is convenient to use reunant coorinates, an to effect the variation of the action consistent with the constraints via the metho of Lagrange unetermine

More information

Advanced Partial Differential Equations with Applications

Advanced Partial Differential Equations with Applications MIT OpenCourseWare http://ocw.mit.eu 18.306 Avance Partial Differential Equations with Applications Fall 2009 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.eu/terms.

More information

The total derivative. Chapter Lagrangian and Eulerian approaches

The total derivative. Chapter Lagrangian and Eulerian approaches Chapter 5 The total erivative 51 Lagrangian an Eulerian approaches The representation of a flui through scalar or vector fiels means that each physical quantity uner consieration is escribe as a function

More information

SOLUTIONS for Homework #3

SOLUTIONS for Homework #3 SOLUTIONS for Hoework #3 1. In the potential of given for there is no unboun states. Boun states have positive energies E n labele by an integer n. For each energy level E, two syetrically locate classical

More information

Least-Squares Regression on Sparse Spaces

Least-Squares Regression on Sparse Spaces Least-Squares Regression on Sparse Spaces Yuri Grinberg, Mahi Milani Far, Joelle Pineau School of Computer Science McGill University Montreal, Canaa {ygrinb,mmilan1,jpineau}@cs.mcgill.ca 1 Introuction

More information

Examining Geometric Integration for Propagating Orbit Trajectories with Non-Conservative Forcing

Examining Geometric Integration for Propagating Orbit Trajectories with Non-Conservative Forcing Examining Geometric Integration for Propagating Orbit Trajectories with Non-Conservative Forcing Course Project for CDS 05 - Geometric Mechanics John M. Carson III California Institute of Technology June

More information

Generalization of the persistent random walk to dimensions greater than 1

Generalization of the persistent random walk to dimensions greater than 1 PHYSICAL REVIEW E VOLUME 58, NUMBER 6 DECEMBER 1998 Generalization of the persistent ranom walk to imensions greater than 1 Marián Boguñá, Josep M. Porrà, an Jaume Masoliver Departament e Física Fonamental,

More information

The Press-Schechter mass function

The Press-Schechter mass function The Press-Schechter mass function To state the obvious: It is important to relate our theories to what we can observe. We have looke at linear perturbation theory, an we have consiere a simple moel for

More information

19 Eigenvalues, Eigenvectors, Ordinary Differential Equations, and Control

19 Eigenvalues, Eigenvectors, Ordinary Differential Equations, and Control 19 Eigenvalues, Eigenvectors, Orinary Differential Equations, an Control This section introuces eigenvalues an eigenvectors of a matrix, an iscusses the role of the eigenvalues in etermining the behavior

More information

BEYOND THE CONSTRUCTION OF OPTIMAL SWITCHING SURFACES FOR AUTONOMOUS HYBRID SYSTEMS. Mauro Boccadoro Magnus Egerstedt Paolo Valigi Yorai Wardi

BEYOND THE CONSTRUCTION OF OPTIMAL SWITCHING SURFACES FOR AUTONOMOUS HYBRID SYSTEMS. Mauro Boccadoro Magnus Egerstedt Paolo Valigi Yorai Wardi BEYOND THE CONSTRUCTION OF OPTIMAL SWITCHING SURFACES FOR AUTONOMOUS HYBRID SYSTEMS Mauro Boccaoro Magnus Egerstet Paolo Valigi Yorai Wari {boccaoro,valigi}@iei.unipg.it Dipartimento i Ingegneria Elettronica

More information

Calculus of Variations

Calculus of Variations 16.323 Lecture 5 Calculus of Variations Calculus of Variations Most books cover this material well, but Kirk Chapter 4 oes a particularly nice job. x(t) x* x*+ αδx (1) x*- αδx (1) αδx (1) αδx (1) t f t

More information

Vectors in two dimensions

Vectors in two dimensions Vectors in two imensions Until now, we have been working in one imension only The main reason for this is to become familiar with the main physical ieas like Newton s secon law, without the aitional complication

More information

Linear First-Order Equations

Linear First-Order Equations 5 Linear First-Orer Equations Linear first-orer ifferential equations make up another important class of ifferential equations that commonly arise in applications an are relatively easy to solve (in theory)

More information

6 Wave equation in spherical polar coordinates

6 Wave equation in spherical polar coordinates 6 Wave equation in spherical polar coorinates We now look at solving problems involving the Laplacian in spherical polar coorinates. The angular epenence of the solutions will be escribe by spherical harmonics.

More information

Left-invariant extended Kalman filter and attitude estimation

Left-invariant extended Kalman filter and attitude estimation Left-invariant extene Kalman filter an attitue estimation Silvere Bonnabel Abstract We consier a left-invariant ynamics on a Lie group. One way to efine riving an observation noises is to make them preserve

More information

Construction of the Electronic Radial Wave Functions and Probability Distributions of Hydrogen-like Systems

Construction of the Electronic Radial Wave Functions and Probability Distributions of Hydrogen-like Systems Construction of the Electronic Raial Wave Functions an Probability Distributions of Hyrogen-like Systems Thomas S. Kuntzleman, Department of Chemistry Spring Arbor University, Spring Arbor MI 498 tkuntzle@arbor.eu

More information

arxiv:cond-mat/ v1 31 Jan 2003

arxiv:cond-mat/ v1 31 Jan 2003 Nosé-Hoover sampling of quantum entangle istribution functions D. Mentrup an J. Schnack 1 arxiv:con-mat/030165 v1 31 Jan 003 Abstract Universität Osnabrück, Fachbereich Physik Barbarastr. 7, D-49069 Osnabrück

More information

The Exact Form and General Integrating Factors

The Exact Form and General Integrating Factors 7 The Exact Form an General Integrating Factors In the previous chapters, we ve seen how separable an linear ifferential equations can be solve using methos for converting them to forms that can be easily

More information

The Three-dimensional Schödinger Equation

The Three-dimensional Schödinger Equation The Three-imensional Schöinger Equation R. L. Herman November 7, 016 Schröinger Equation in Spherical Coorinates We seek to solve the Schröinger equation with spherical symmetry using the metho of separation

More information

1. At time t = 0, the wave function of a free particle moving in a one-dimension is given by, ψ(x,0) = N

1. At time t = 0, the wave function of a free particle moving in a one-dimension is given by, ψ(x,0) = N Physics 15 Solution Set Winter 018 1. At time t = 0, the wave function of a free particle moving in a one-imension is given by, ψ(x,0) = N where N an k 0 are real positive constants. + e k /k 0 e ikx k,

More information

arxiv:hep-th/ v1 3 Feb 1993

arxiv:hep-th/ v1 3 Feb 1993 NBI-HE-9-89 PAR LPTHE 9-49 FTUAM 9-44 November 99 Matrix moel calculations beyon the spherical limit arxiv:hep-th/93004v 3 Feb 993 J. Ambjørn The Niels Bohr Institute Blegamsvej 7, DK-00 Copenhagen Ø,

More information

Thermal conductivity of graded composites: Numerical simulations and an effective medium approximation

Thermal conductivity of graded composites: Numerical simulations and an effective medium approximation JOURNAL OF MATERIALS SCIENCE 34 (999)5497 5503 Thermal conuctivity of grae composites: Numerical simulations an an effective meium approximation P. M. HUI Department of Physics, The Chinese University

More information

arxiv: v1 [cond-mat.stat-mech] 9 Jan 2012

arxiv: v1 [cond-mat.stat-mech] 9 Jan 2012 arxiv:1201.1836v1 [con-mat.stat-mech] 9 Jan 2012 Externally riven one-imensional Ising moel Amir Aghamohammai a 1, Cina Aghamohammai b 2, & Mohamma Khorrami a 3 a Department of Physics, Alzahra University,

More information

Assignment 1. g i (x 1,..., x n ) dx i = 0. i=1

Assignment 1. g i (x 1,..., x n ) dx i = 0. i=1 Assignment 1 Golstein 1.4 The equations of motion for the rolling isk are special cases of general linear ifferential equations of constraint of the form g i (x 1,..., x n x i = 0. i=1 A constraint conition

More information

Homework 7 Due 18 November at 6:00 pm

Homework 7 Due 18 November at 6:00 pm Homework 7 Due 18 November at 6:00 pm 1. Maxwell s Equations Quasi-statics o a An air core, N turn, cylinrical solenoi of length an raius a, carries a current I Io cos t. a. Using Ampere s Law, etermine

More information

Time-of-Arrival Estimation in Non-Line-Of-Sight Environments

Time-of-Arrival Estimation in Non-Line-Of-Sight Environments 2 Conference on Information Sciences an Systems, The Johns Hopkins University, March 2, 2 Time-of-Arrival Estimation in Non-Line-Of-Sight Environments Sinan Gezici, Hisashi Kobayashi an H. Vincent Poor

More information

Diagonalization of Matrices Dr. E. Jacobs

Diagonalization of Matrices Dr. E. Jacobs Diagonalization of Matrices Dr. E. Jacobs One of the very interesting lessons in this course is how certain algebraic techniques can be use to solve ifferential equations. The purpose of these notes is

More information

Switching Time Optimization in Discretized Hybrid Dynamical Systems

Switching Time Optimization in Discretized Hybrid Dynamical Systems Switching Time Optimization in Discretize Hybri Dynamical Systems Kathrin Flaßkamp, To Murphey, an Sina Ober-Blöbaum Abstract Switching time optimization (STO) arises in systems that have a finite set

More information

G4003 Advanced Mechanics 1. We already saw that if q is a cyclic variable, the associated conjugate momentum is conserved, L = const.

G4003 Advanced Mechanics 1. We already saw that if q is a cyclic variable, the associated conjugate momentum is conserved, L = const. G4003 Avance Mechanics 1 The Noether theorem We alreay saw that if q is a cyclic variable, the associate conjugate momentum is conserve, q = 0 p q = const. (1) This is the simplest incarnation of Noether

More information

Noether s theorem applied to classical electrodynamics

Noether s theorem applied to classical electrodynamics Noether s theorem applie to classical electroynamics Thomas B. Mieling Faculty of Physics, University of ienna Boltzmanngasse 5, 090 ienna, Austria (Date: November 8, 207) The consequences of gauge invariance

More information

Physics 505 Electricity and Magnetism Fall 2003 Prof. G. Raithel. Problem Set 3. 2 (x x ) 2 + (y y ) 2 + (z + z ) 2

Physics 505 Electricity and Magnetism Fall 2003 Prof. G. Raithel. Problem Set 3. 2 (x x ) 2 + (y y ) 2 + (z + z ) 2 Physics 505 Electricity an Magnetism Fall 003 Prof. G. Raithel Problem Set 3 Problem.7 5 Points a): Green s function: Using cartesian coorinates x = (x, y, z), it is G(x, x ) = 1 (x x ) + (y y ) + (z z

More information

The electrodynamics of rotating electrons.

The electrodynamics of rotating electrons. Die Elektroynamik es rotierenen Elektrons, Zeit. f. Phys. 37 (196), 43-6. The electroynamics of rotating electrons. By J. Frenkel 1 ) in Leningra. (Receive on May 196) Translate by D. H. Delphenich The

More information

On the Conservation of Information in Quantum Physics

On the Conservation of Information in Quantum Physics On the Conservation of Information in Quantum Physics Marco Roncaglia Physics Department an Research Center OPTIMAS, University of Kaiserslautern, Germany (Date: September 11, 2017 escribe the full informational

More information

Average value of position for the anharmonic oscillator: Classical versus quantum results

Average value of position for the anharmonic oscillator: Classical versus quantum results verage value of position for the anharmonic oscillator: Classical versus quantum results R. W. Robinett Department of Physics, The Pennsylvania State University, University Park, Pennsylvania 682 Receive

More information

Gravitation as the result of the reintegration of migrated electrons and positrons to their atomic nuclei. Osvaldo Domann

Gravitation as the result of the reintegration of migrated electrons and positrons to their atomic nuclei. Osvaldo Domann Gravitation as the result of the reintegration of migrate electrons an positrons to their atomic nuclei. Osvalo Domann oomann@yahoo.com (This paper is an extract of [6] liste in section Bibliography.)

More information

Characterizing Real-Valued Multivariate Complex Polynomials and Their Symmetric Tensor Representations

Characterizing Real-Valued Multivariate Complex Polynomials and Their Symmetric Tensor Representations Characterizing Real-Value Multivariate Complex Polynomials an Their Symmetric Tensor Representations Bo JIANG Zhening LI Shuzhong ZHANG December 31, 2014 Abstract In this paper we stuy multivariate polynomial

More information

APPROXIMATE SOLUTION FOR TRANSIENT HEAT TRANSFER IN STATIC TURBULENT HE II. B. Baudouy. CEA/Saclay, DSM/DAPNIA/STCM Gif-sur-Yvette Cedex, France

APPROXIMATE SOLUTION FOR TRANSIENT HEAT TRANSFER IN STATIC TURBULENT HE II. B. Baudouy. CEA/Saclay, DSM/DAPNIA/STCM Gif-sur-Yvette Cedex, France APPROXIMAE SOLUION FOR RANSIEN HEA RANSFER IN SAIC URBULEN HE II B. Bauouy CEA/Saclay, DSM/DAPNIA/SCM 91191 Gif-sur-Yvette Ceex, France ABSRAC Analytical solution in one imension of the heat iffusion equation

More information

Total Energy Shaping of a Class of Underactuated Port-Hamiltonian Systems using a New Set of Closed-Loop Potential Shape Variables*

Total Energy Shaping of a Class of Underactuated Port-Hamiltonian Systems using a New Set of Closed-Loop Potential Shape Variables* 51st IEEE Conference on Decision an Control December 1-13 212. Maui Hawaii USA Total Energy Shaping of a Class of Uneractuate Port-Hamiltonian Systems using a New Set of Close-Loop Potential Shape Variables*

More information

arxiv:physics/ v2 [physics.ed-ph] 23 Sep 2003

arxiv:physics/ v2 [physics.ed-ph] 23 Sep 2003 Mass reistribution in variable mass systems Célia A. e Sousa an Vítor H. Rorigues Departamento e Física a Universiae e Coimbra, P-3004-516 Coimbra, Portugal arxiv:physics/0211075v2 [physics.e-ph] 23 Sep

More information

Quantum circuit dynamics via path integrals: Is there a classical action for discrete-time paths?

Quantum circuit dynamics via path integrals: Is there a classical action for discrete-time paths? Quantum circuit ynamics via path integrals: Is there a classical action for iscrete-time paths? Mark D. Penney, 1, Dax Enshan Koh, 2, an Robert W. Spekkens 3, 1 Mathematical Institute, University of Oxfor,

More information

FLUCTUATIONS IN THE NUMBER OF POINTS ON SMOOTH PLANE CURVES OVER FINITE FIELDS. 1. Introduction

FLUCTUATIONS IN THE NUMBER OF POINTS ON SMOOTH PLANE CURVES OVER FINITE FIELDS. 1. Introduction FLUCTUATIONS IN THE NUMBER OF POINTS ON SMOOTH PLANE CURVES OVER FINITE FIELDS ALINA BUCUR, CHANTAL DAVID, BROOKE FEIGON, MATILDE LALÍN 1 Introuction In this note, we stuy the fluctuations in the number

More information

3-D FEM Modeling of fiber/matrix interface debonding in UD composites including surface effects

3-D FEM Modeling of fiber/matrix interface debonding in UD composites including surface effects IOP Conference Series: Materials Science an Engineering 3-D FEM Moeling of fiber/matrix interface eboning in UD composites incluing surface effects To cite this article: A Pupurs an J Varna 2012 IOP Conf.

More information