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space-time coordinate (0, 0) followed by particle creation at (τ, r) and (b) the creation of a particle at (0, 0) followed by its annihilation at (τ, r).65 The annihilation process initiating (a) may be interpreted alternatively as the creation of a hole, i.e. the composite process D describes the joint propagation of ... |
= ωn, i.e. q eiq·xDq, whereD q = T Ld limR→0 R−1 p e−ip·xψa ¯ψa p2+qψa p2 ¯ψa p1 p1+q p1+q ψa p1p2 Dq = T Ld lim R→0 1 R ωn p1p2 ¯ψa p1,ωn ψa p1+q,ωn+m ¯ψa p2+q,ωn+m ψa p2,ωn ψ. (6.54) A3: Only diagrams that contain one free summation over the Fermi surface per impurity line contribute to leading order in (pF)−1. (Form... |
C is defined as the solution of the equation (|ωm| + D(−i∇r + 2A)2)Γ(r, ωm) = (2πντ Ld)−1δd(r) (a formal solution of which is given by the right-hand side of the definition above). Crucially, the presence of the vector potential spoils the singularity of the cooperon mode in the limit q, ωm → 0. In other words, the magne... |
nate representation) wherein time-reversal amounts to transposition. 75 Note that, under time-reversal, the sign of the time-derivative is reversed: dτ ( ¯ψ∂τ ψ)T = − dτ (∂τ ψT ) ¯ψT = − dτ ψT (−∂τ ) ¯ψT . 76 Notice that the temporal minus sign in the fields ψT and ¯ψT is introduced to remove the unwanted sign multiplyi... |
d conductors at low temperatures. Our target is a low-energy action of the elements Q = T ΛT −1 ∈ Sp(4RM )/(Sp(2RM ) × Sp(2RM )) of the Goldstone mode manifold. The action of this nonlinear σ-model can be constructed by substituting the slowly fluctuating matrix configuration Q = {Qα,α nn (r)} into the action (6.59) and ... |
essing a spatially homogeneous mean-field configuration may host other solutions of physical significance. Indeed, we have encountered a scenario of this type already in Chapter 3 above. Exploring quantum double-well tunneling, we observed that the imaginary time Euler–Lagrange equations of a particle in a doubly degenera... |
than Tc. To this end, add to and subtract from the right-hand side of . Then expand to leading order in the small the gap equation the integral parameters δT /Tc and Δ/Tc, whereδT = Tc − T > 0. dx tanh x x Answer: (a) For Δ = 0, λ(ξ) = (ξ2 + Δ2)1/2 = |ξ| and Eq. (6.28) assumes the form 1 gν = 0 ωD/2Tc dx tanh x x , wh... |
dependent free energy by Z [ ˜V0] = exp(−βF [ ˜V0]), noting that ˜V0 shifts the chemical potential, F [ ˜V0](μ) =F (μ − i ˜V0), and neglecting the ˜V0-dependence of G[ ˜V0] G, we obtain the saddle-point equation 0 = ∂ ∂ ˜V0 1 4EC ˜V 2 0 − iN0 ˜V0 − F (μ − i ˜V0) = 1 2EC ˜V0 − iN0 + i ˆN μ−i ˜V0 , F (μ − i ˜V0) =− i∂μF ... |
g to the superconducting case, show that, at an intermediate stage, the action is given by Seff [V, φ] = Sc[V ] − tr ln ∂τ + ( ˆξ1 + i( ˙φ1 + V )/2)σ3 + Δσ1 T †ei(φ1−φ2)σ3/2 e−i(φ1−φ2)σ3/2T ∂τ + ( ˆξ2 + i( ˙φ2 − V )/2)σ3 + Δσ1 , where ˆξi, i = 1, 2, comprise the single-particle energies of the system, and Sc[V ] = dτ V ... |
Leggett 1938– Co-recipient of the 2003 Nobel Prize in Physics (with Alexei A. Abrikosov and Vitaly L. Ginzburg) “for pioneering contributions to the theory of superconductors and superfluids.” He has made important contributions to the theory of normal and superfluid helium liquids and other strongly coupled superfluids,... |
ctron–hole condensate. As a result experimentalists have used “Feshbach resonance” phenomena to tune the atomic pair interaction from weak to strong coupling, whence the atoms exist as tightly bound pairs. By monitoring the dynamics of BEC formation, attempts have been made to infer the properties of the ephemeral BCS-... |
ternatively, if the transition to the magnetic phase is of second order (i.e. the expectation value of the magnetization field grows continously from zero as the interaction is increased through Uc), a field theory of the system near the critical point can be developed as a perturbative expansion 6.7 Problems 353 of the ... |
s point, see J. Zinn-Justin, Quantum Field Theory and Critical Phenomena (Oxford University Press, 1993). 6.7 Problems 357 Notice that both the lack of gauge invariance of the measure and the UV problems manifest themselves in an integral over (quantum) fluctuations, i.e. while the symmetry is preserved on the classical... |
th the other two categories of experiment the situation is different. Transport and spectroscopic measurements can be used to probe both static and dynamical features of a system; further, fully angle/frequency-resolved spectroscopic data contain detailed information on the spatio-temporal structure of the dominant exci... |
sion (Ω(K), K)) of the states inside the solid. This is where the detective work of spectroscopy begins. What we know is that the dispersions of the scattered particles and conof the (k, ω(k)) stituents, and (K, Ω(k)), respecrelated are tively, sample Sir Chandrasekhara V. Raman 1888– 1970 (left), Lord (John Rayleigh S... |
ction, we argued that condensed matter experiments typically probe the . Such linear (linear) response of a system to the application of weak perturbations response can be cast in terms of a generalized susceptibility χ: Eq. (7.2). In the following we try to give the formal expression (7.2) a concrete meaning. Specifica... |
ditional operator representation, i.e. expressions with circumflexes, ˆX, represent canonically quantized operators and · · · = Z −1tr(· · ·exp{− β[ ˆH − μ ˆN ]}) represents the quantumthermal expectation value. Restricting ourselves to correlation functions of operators taken at two different times,11 the general definit... |
epresentations above apply to C T,+,−(z = ω) whereω is restricted to the real axis.) This extended interpretation allows us to view C T,+,− as complex functions with singularities in the immediate vicinity of the real axis. More specifically: The retarded correlation function C + has singularities for z = −Ξαβ − iη slig... |
the eigenvalues of this operator – which are still functions of z – are given by the correlation function Ga(z) above. Numerous physical observables can be compactly represented in terms of the operator Green function. For example, using Eq. (7.19), it is straightforward to verify that the single-particle density of s... |
ion of A as a probability measure describing in what way the spectral weight carried by the state c† a|α is spread out over the 18 Strictly speaking, we can integrate A only if the variance of Σ(ω) over the interval [ξa + Σ − Σ, ξa + Σ + Σ] in which the Lorentzian is peaked is negligible (but see below). 7.3 Analytic s... |
n, Many Particle Physics (Plenum Press, 1981). 21 We assume that we are dealing with a Fermi liquid, i.e. that we can think of the constituents of the system as fermionic quasi-particles, in the spirit of Landau’s theory. 7.3 Analytic structure of correlation functions 387 a linear approximation, the induced charge den... |
dx ∂μ this condition can only be generally valid if → ∂μ Kμν = 0. Summarizing, Gauge invariance and particle number conservation demand the identity → ∂μ Kμν = Kμν ← ∂ν= 0. We next turn to the derivation of the linear response kernel. Our starting point is an observation made already in Chapter 1 (and several times th... |
the Info block above shows that any meaningful analysis of the conductivity must take account of the presence of static disorder; without disorder, the field would make the electrons freely accelerate, i.e. there would be no such thing as a steady current flow in metals. Thus, what we should have in mind when we think ab... |
es the (fictitious) propagation of an electron backwards in time. However, an electron propagating in a chronologically reversed direction can be interpreted as a hole moving forward in time. Thus, the advanced electronic Green function effectively represents a descriptor of hole dynamics. That the product of two Green f... |
in turn implies that the overlap |Ψ|Ψ|2 vanishes as some negative power of N . sin2 δm (n−m+ δm n<nF,m>nF π )2 7.6.2 RPA dielectric function Much of the response of a system of charged fermions to an external electromagnetic perturbation is encoded in the dielectric function q. While the dielectric function cannot be c... |
B ˆN . (7.61) (d) In Chapter 9, we apply the linear response formulae derived above to a field-theoretical analysis of the quantum Hall effect, the physics of a two-dimensional electron gas subject to a strong perpendicular field. Our starting point will be the replicated partition sum Z = D(ψ, ¯ψ) exp(−S[ψ, ¯ψ]), where S... |
entary particle theory and condensed matter physics (critical phenomena and the Kondo problem) to quantum chemistry and computer science. (Image c The Nobel Foundation.) The general line of reasoning above summarizes much of the thinking behind the renormalization group. Of course, the approach would be quite useless h... |
nality? Consider, for example, a two-dimensional variant of the model. Here the formation of a large connected region of M mismatched spins incurs an energy cost U ∼ M 1/2J. To understand why, one may note that the energy cost is proportional to the length of the one-dimensional boundary that encloses a (circular) doma... |
f the conceptual foundations of the RG on a model application. According to the general scheme outlined at the beginning of the chapter, our aim is to devise an algorithm to recursively trace out parts of the short-scale fluctuations of the system and assess their influence on the remaining degrees of freedom. 418 The re... |
. Indeed, we expect on general grounds that (see the discussion of the previous section) the reduced free energy should scale with the inverse of the correlation length ξ, which in turn diverges upon approaching the zero-temperature fixed point. Comparing with Eq. (8.10), and noting that there are no reasons for the res... |
carries the dimension [dτ ] = [frequency]−1 and, therefore, changes by a factor b. We are now in a position to compare the effective actions S[θ] andS [θ] before and after the integration over the fast modes. Obviously, the principal effect of the integration over fast modes is that the coupling constant of the periodic ... |
t that the integration area is proportional to b, and we have used the fact that, for those narrow time windows, the field integration will be oblivious to the difference between θ(τ ) andθ (τ ). The second proportionality is obtained by averaging the integrand along the lines of our previous calculations. After the resc... |
ese operators in the action from the very beginning (with an a priori undetermined coupling constant). One then verifies whether the augmented action represents a complete system, i.e. one that does not lead to the generation of operators beyond those that are already present. If necessary, one has to repeat this step u... |
epts of RG theory (such as the scaling laws to be discussed below). 17 A marginal scaling field corresponds to a direction in coupling constant space with vanishing partial derivative, ∂φα R|g∗=0 = 0. In this case, to obtain a refined picture, one sometimes considers the second-order derivative, ∂2 α. For x > 0 φα (x <0)... |
th diverges as ξ ∼ |t|−ν . η: This implies that the correlation function, * C(r) ∼ 1 |r|d−2+η , exp[−|r|/ξ], |r| ξ, |r| ξ, crosses over from exponential to a power law scaling behaviour at the length scale ξ. To motivate the power, one may notice that C ∼ φφ carries twice the dimension of the field 20 Unfortunately, the... |
gα>1 are irrelevant (or, for that matter, marginal). We can then write C(pi, g1, gα) = bndφ C(pib, g1bλ1 , gαbλα ) = g −ndφ/λ1 1 g11≈ g −1/λ1 1 C(pig , 1, 0) ≡ g −ndφ/λ1 1 C(pig −1/λ1 1 , 1, gαg −λα/λ1 1 ) −ndφ/λ1 1 F (pig −1/λ1 1 ). Here, we have used the freedom of arbitrarily choosing the parameter b to set g1bλ1 = ... |
e it is straightforward to attribute engineering dimensions to all other operators: φ2 = L2, φ4 = L−d+4, φn = Ld+(2−d)n/2, (∇mφ)2 = L2(1−m). These relations convey much about the potential significance of all structurally allowed operators: The engineering dimension of the non-gradient operator ∼ φ2 is positive in all d... |
that we are expanding not around the “true” mean-field, i.e. the exact solution of (8.24), but rather around the solution ¯φ = 0 of the field-free system. However, in view of the fact that h has the status of an external perturbation, this choice of the reference configuration is quite natural. 8.4 RG analysis of the ferr... |
action31 is multiplied by a large parameter (which, in the case of a quantum theory, might be −1). The expansion in the number of loops is then equivalent to an expansion in the inverse of that parameter (for a quantum theory, an expansion away from the classical limit). 30 L. H. Ryder, Quantum Field Theory, (Cambridg... |
sion. Of course, a more qualified approach to the question is to explore what happens at higher order in the -expansion. Needless to say, the price to be paid for this ambition is that, at orders O(n>1), the analysis indeed becomes laborious. Nonetheless, the success of the first-order expansion prompted researchers to d... |
= J(π) encapsulates both the geometry of the Haar measure and the Jacobian associated with the transformation g → a πaTa. Referring for a more detailed discussion of the function J to text books on group theory, we here merely note that its Taylor expansion in π starts as J(π) = 1 + O(π4) where theO (π4) term will not ... |
rehensive discussion of the role of geometry and topology in quantum field theory will be developed in the next chapter.) Consider then a two-dimensional square lattice with a phase-like variable exp(iθi) ∈ S1 defined on each of its sites i. Demanding that the Hamiltonian or action of the system be periodic in all θi and... |
ormation at low temperatures and protects the integrity of the quasi-long-range ordered phase. To explore the range over which vortices are suppressed, one may explore the partition function for a configuration with just a single vortex of unit 41 Notice that, if the spin degrees of freedom have three components or more... |
ression into Eq. (8.45), and changing integration variables, one finds that the term linear in x integrates to zero while the angular average of (x · ∇XC)2 leads to x2(∇XC)2/2. Thus, to O(r4), one obtains e−Seff (r−r) e−4π2JC(r−r) × 1 + y2 0 (dx 2π x)e−4π2JC(x)8πJ 2 x2 2 d2X (∇X(C(r − X) − C(r − X)))2 . d2X [∇X(C(r−X)−C... |
cussion was substantial enough to convince the reader of the enormous power and versatility RG methods have in disclosing “deep” physical information and to motivate further exploration of the subject. INFO While, for the most part, previous chapters were guided by symmetry principles, little has been said so far about... |
critical theory. The aim of the present problem is to explore the nature of the critical phenomena when the critical point is driven to zero temperature – a quantum critical point. Motivated by the coherent state formulation of the quantum partition function of an interacting system, it is tempting to associate direct... |
δ(b) = 1) while v(b) remains small, the perturbative expansion remains valid. However, (ii) if v(b) grows to order unity while δ(b) remains small, the scaling behavior moves into a region potentially controlled by non-Gaussian fluctuations. From the equations above, the condition for Gaussian behavior, i.e. δ(b) = 1 and... |
ariant (up to a phase) and can be omitted. In Section 3.3 we used this representation to identify the phase space of spin as the coset space SU(2)/U(1), the 2 sphere. In the Q language, the same sphere is represented as Q = gσ3g−1, where ˆSi = σi/2 are identified with the Pauli matrices. Again, the ψ factor, commutative... |
es of the conductance, the scaling function approaches the asymptote β(g) → d − 2 corresponding to ohmic behavior. For very small values of conductance, the scaling function approaches β(g) → ln g, which is characteristic of insulating behavior. According to the weak localization expansion, a localization transition is... |
lems 493 is associated with eight possible contributions, which can be grouped in pairs. (You may find it helpful to enumerate these possibilities diagrammatically.) In particular, show that there exists a contribution J+J− k skskf ˆS−c † k s ↑ckf ↓ 1 E − ˆH22 † ˆS+c kf ↓cks↑|ψ1, where the wavevectors kf (ks) index stat... |
in a single chapter.2 Consequently, our discussion is example–oriented and often regrettably superficial (with regard to both physical depth and, especially, mathematical structures). In fact, the aim of the present text is to demystify the subject of topology in field theory, to arouse the interest of readers and to mo... |
φ) removes A from the Hamiltonian while changing the boundary conditions to ψ(0) = e2πiAψ(2π). In the gauge-transformed picture, the presence of the magnetic field thus amounts to a twist in the boundary conditions of the wavefunctions, and the persistent current is a measure of the sensitivity of the spectrum to this t... |
ce yourself of the veracity of this statement) π1(T d . Turning to higher dimensions, it becomes more and more difficult to identify homotopy classes simply by invoking one’s imagination. One of the last intuitively accessible examples is π2(S2) = Z: maps of the 2-sphere into itself can be classified according to how ofte... |
. theories where the base manifold represents space-time) are called “instantons.” By contrast, “solitons” are topological solutions of classical equations of motions. However, this rule is also sometimes broken. The ubiquitous presence of the suffix “-on” reflects a widespread tendency in physics to associate excitations... |
agnetic spin chains. Surprisingly, though, this expectation does not conform with experimental observation. Neutron scattering experiments on one-dimensional spin 1/2 antiferromagnets have indeed shown that, in the vicinity of the N´eel ordering wavevector q = π/a, the dispersion is linear. However, spin S = 1 chains s... |
topological term modify this behavior? To get some idea of what might happen, let us reformulate the partition function as a sum over disjoint topological sectors, Z = DnW e2πiSW e−S0[nW ], (9.16) W ∈Z where nW denotes field configurations of winding number W . Equation (9.16) provides a preliminary explanation for the ... |
same time, the longitudinal resistivity/conductivity drops by as much as 13 orders of magnitude. In passing we note that the rapid oscillations visible in the figure at small field strengths represent the familiar Shubnikov–de Haas oscillations. 21 One may recall that the flux quantum is defined through the relation Φ0 = ... |
y a gauge transformation that does not alter the boundary conditions.) That, however, does not necessarily imply that individual basis states map onto themselves upon the completion of the path φ = 0 → φ = 2π. I.e., while the set of eigenstates as a whole gets reproduced, permutations of individual states are consisten... |
any other characteristics. 27 J. E. Avron and R. Seiler, Quantization of the Hall conductance for general, multiparticle Schr¨odinger Hamil- tonians, Phys. Rev. Lett. 54 (1985), 259–62. 28 D. J. Thouless, M. Kohmoto, M. P. Nightingale, and M. den Nijs, Quantized Hall conductance in a two- dimensional periodic potential... |
discussed in Section 9.4, this is not accidental but rather reflects a fundamental property of topological terms. For future reference, we also anticipate that the boundary descendant of the bulk θ-term Eq. (9.23) is an example of a Wess–Zumino term. 3 T −1 → T hσar We next show that, under the conditions stated above,... |
f an Onsager relation. Consistency with these relations requires that the topological series be of the form σ11 = σ0 11 + δσ11 + ∞ W =1 cos(2πW σ0 12) a(W )(σ0 11), σ12 = σ0 12 + ∞ W =1 sin(2πW σ0 12) b(W )(σ0 11), (9.27) 534 Topology where a(W ) and b(W ) are expansion coefficients. The notation emphasizes that, in the ... |
φ (x) T U′ z z′ z–1 z (φ (x)) V z′ z′(φ (x)) V′ Figure 9.10 On the construction of coordinate representations of field manifolds. For a discussion, see the main text. then explain the general ideas behind WZ field theory before we turn to the discussion of a number of interesting applications. 9.4.1 A crash-course in diff... |
vince yourself that, for manifolds T ⊂ Rn, this reduces to the standard definition of the differential with which you are familiar.) However, not every 1-form is a differential of a function. Consider, for example, the tangent basis of T = S1 constructed in the exercise on page 539. Let us define a 1-form by setting ω(e) =... |
with an atlas of identically oriented charts is said to be orientable. (A prominent counterexample is presented by the M¨obius strip.) The definition of the integral above implies that we have chosen a definite orientation. For future reference, we remark that, if φ : T1 ⊃ U1 → U2 ⊂ T2 is a diffeomorphism 9.4 Wess–Zumino ... |
ot familiar with Stokes’ theorem may be helpful. First note that ∂C is a manifold by itself, with dim ∂C = n−1. Thus, ω is top-dimensional on ∂C and can be integrated. To gain some insight into the substance of Eq. (9.39) let us consider a few special cases. For example, let M be a three-dimensional manifold, n = 3. Co... |
quantized according to Eq. (9.43). Having discussed the structure and geometry of WZ theories, we now return to physics. Using a simple prototype system as an example, we begin by exploring how WZ terms enter low-energy theories of many-body quantum systems. 9.4.3 Example: magnetic moment coupled to fermions Consider a... |
erits its time dependence from the parameters x(t). We may thus write t γ(t) = i t 0 dt 0(x(t))|∂xi(t)|0(x(t))∂txi(t) = i c dx 0(x)|∂x|0(x) = i 0|d0. c Here, the second integral has to be interpreted as a line integral in parameter space. It is taken along a curve c which starts at x(0), follows the evolution of the pa... |
ystem. In fact, we shall begin by considering the totally non-interacting case.64 Switching from a lattice to a continuum description and linearizing around the two Fermi points (for details, see Section 2.2), we describe this prototypical system in terms of the action S[ψ†, ψ] = s=±1 dx dτ ψ†r s (−isvF∂x + ∂τ ) ψr s =... |
ze. This tells us that S[g] alone does not suffice to establish the boson–fermion correspondence. But let us now inspect the second term in the action proposed by Witten, the two-dimensional WZ functional. The first thing we have to understand is why the second term of the action indeed represents a WZ functional in the s... |
its invariance under spin transformations, the bosonic representation of the umklapp operator reads ∼ λuk cos 4φ. ∂zφ and js = 1√ 8π 2π EXERCISE To obtain the bosonic representation of the umklapp operator, substitute Eq. (9.63) into its definition and obtain ∼ λukei4φtr(gσ2gT σ2) + h.c. ∼ λuk cos(4φ). Here the last equ... |
system is described by the O(3)-model with topological angle 2πS = π. On the other hand, we might have approached the problem via the WZW route discussed above. Within that context, the ferromagnetic perturbation turns out to be irrelevant (see Affleck and Haldane62), i.e. the long-range physics of the system is describ... |
f vanishing strength. This nicely conforms with the experimental observation of Fermi-liquid-like behavior (no QHE) close to half filling. We have seen in Section 9.3.4 that, when a flux quantum is adiabatically pushed through an annular quantum Hall geometry, an electron charge flows from the inner to the outer perimeter... |
In the following we will investigate what information can be obtained from the functional integral Eq. (9.76) about the physical behavior of the FQH system. Particle exchange in two dimensions Before embarking on this program, it may be of interest to discuss a few general aspects of Chern–Simons field theory and partic... |
iτ ∈ −i[0, β] is that the initial and final points of our two space-time trajectories now have to be identified (the usual temporally periodic boundary conditions of the imaginary time formulation101). A glance at the figure shows that this leads to a pair of two closed world line curves which, for a winding angle φ = 2πn... |
(a, σ) → (¯a, 0) in the action. Using the fact that aext = 2sνAext, we arrive at the last line, where the coupling constant qeff = 1 − 2sν = 1 1 + 2sp , (9.82) is identified as the effective charge of the CF. The line of reasoning above tells us that CFs effectively carry fractional charge. The partial “screening” of the b... |
eates an accumulation of statistical flux that in turn acts as a scattering center of CFs, etc. Thus, we readily wind up with a full-blown problem “interaction + disorder + strong magnetic field” whose rigorous microscopic solution seems to be elusive. Nonetheless, all evidence suggests that eventually the CFs will be lo... |
on around the ring), many modes contribute to the integral and a continuum approximation is valid. Thus, the dominant contribution to 590 Topology the correlation function comes from frequencies |ω| < Ec, for which the discreteness of the sum really matters.114 Carry out the sum over momenta by the methods otherwise em... |
e WZW action reduces to the θ-term for the unit-modular field n ∈ S2 : Γ[in · σ] = πStop[n], where Stop[n] = 1 4π S2 d2x n · (∂1n × ∂2n). Answer: (a) Using the fact that g−1dg g−1 = −dg−1 (why?) the form ω can be rewritten as ω = tr(dg−1 ∧ dg ∧ dg−1 g), i.e. dω = −tr(dg−1 ∧ dg ∧ dg−1 ∧ dg). To show that this expression ... |
φ ≡ ∂iφdxi, where we use the symbol d to denote the real space contribution to the exterior derivative. Plug this ansatz into the residual contribution to the action (after a0 has been integrated out) to reduce the field strength tensor to dτ ∂xφ∂τ φ. Recalling that the CS action enters the boundary action S[φ] = the th... |
nonequilibrium statistical (field) theory. In the following, we introduce a spectrum of concepts central to the description of many particle systems out of statistical equilibrium. We will see that key elements of the theory – Langevin theory and the formalism of the Fokker–Planck equation – can be developed from the co... |
Eq. (10.3), with first and second cumulant μ1 = N ˜μ1 and μ2 = N ˜μ2, respectively. (All higher cumulants of the Gaussian distribution vanish. Exercise: verify this statement by showing that the generating function of the Gaussian distribution is again a Gaussian.) The ubiquity of additive random variables in nature ex... |
2) = f (x 2). Assuming that f (x) =f (H(x)) ≡ f () is a function of energy, we conclude that probability conservation is compatible with energy conservation, 1 + 2 = 1 + 2, if ln f () = a + b is linear in energy. In this case, f (x1)f (x2) = exp(a(1 + 2) + 2b) = exp(a( 2) is indeed satisfied. To fix the constants a and b... |
dissipation or friction are intimately linked to the presence of fluctuating forces. However, unlike the everyday phenomenon of friction, the corresponding fluctuation forces are usually less noticeable. The reason is that friction acts in a directed way (cf. the action of a brake), while the response caused by fluctuati... |
bability to find v at t for initial data (v0, t0). Weighing by the conditional probability to move on to v and summing over all intermediate configurations, v, we obtain the total probability (v0, t0) → (v, t). Equation (10.20) is the defining property of a Markovian process, i.e. a process which is fully determined by on... |
y now think of them as amoebae or another not too complex animal) with a mechanism of self-propulsion. To this end, we imagine the particles endowed with an energy storage. The time-dependent energy level, (t), will (a) increase due to food intake at some rate, q, (b) decrease at rate −c(t) due to metabolic activity (n... |
obabilities. Identifying (1, 2) ↔ |i as a classical approximation to a (coherent) state in two particle Hilbert space,16 and (1, 2) ↔ |f as a final state, we have the identification, w(1, 2; 1, 2) ↔ |Sfi|2, where Sfi is the scattering matrix. Unitarity means that |Sfi|2 = i |Sif |2 = 1, or i d1d2 w(1, 2; 1, 2) = d1d2 w(1, 2... |
reservoirs kept at different temperature), we may then expect a scenario wherein the collision integral aims to establish local thermal equilibrium, while the left hand side will try to compromise between the “cost” of spatial variations and the need to adjust to the conditions imposed by the external perturbation. The ... |
state (an+1, tn+1) depends on the current state (an, tn), but not on the history that got us there, (an−1, tn−1; . . .). Put differently, a Markov process lacks memory. Markov processes owe their popularity to the fact that they optimally compromise between descriptive power and analytical tractability; if possible, on... |
2q)t and variance ∼ √ t. Random processes whose distributions are Gaussian are generally called Gaussian processes. The example illustrates that Gaussian processes are typically the results of the addition of a large number of elementary random variables. Example: Poisson process n Now consider a sequence of elementar... |
he distribution, the Fokker–Planck prediction is by many orders of magnitude off the true result. 0 -10 -20 -30 -40 10 20 30 n 40 The origins of the this error can be traced to the second order expansion of the operator ˆE1 = e−∂x/N . Doing so, and replacing this operator by an effective long-range approximation wherein ... |
ni−1} is shorthand for the lattice time derivative. INFO The discretization leading to a unit functional determinant goes under the name Ito discretization. More general discretization schemes call for a treatment of the corresponding functional determinants. It is customary to represent these determinants in terms of... |
. By generalization of the ideas exemplified in Section 10.4.4 on the Poisson process, we can derive a path integral representation for the master equations describing Markovian stochastic processes. Unsurprisingly, this path integral turns out to be a close ally of the MSRJD functional integral above. For simplicity, ... |
Hamiltonian operator. The price to be paid for this simplicity is that the integration variables ψ and ¯ψ do not have a direct physical interpretation. The network of different theories constructed in the previous sections is summarized in Fig. 10.9. So far, we have been focusing on the case of low-dimensional problems... |
function of the field and its spatial derivatives. Representing the δ-constraint in terms of a Fourier integral over a “momentum field” ψ and integrating over the noise field we arrive at O[φ]ξ = D(φ, ψ) O[φ] ei dx ψ(x)(∂tφ(x)+D(−Δ)n δH[φ] δφ(x) )− dxdx ψ(x)K(x−x)ψ(x), 35 Typically, the dominant contribution (in the sense... |
hat χ(ω) = C+(ω) = −iΘ(t)[ ˆX(t), ˆX(0)], where C + was the retarded response function. We then established a connection between C + and another correlation function, the time ordered correlation function, C T (t) ≡ −iTt ˆX(t) ˆX(0), 36 Chapter 7 was formulated for quantum theories, but that aspect will not be of relev... |
xt allow the particles to hop between nearest neighbour lattice sites (subject to the condition of no more than single occupancy). This will render the system dynamical and allow it to settle in a configuration compromising between single particle dynamics and interactions. To see this more clearly, imagine the dynamics... |
of Eq. (10.93) will generate the bare version of a generalized Langevin equation. However, we must keep in mind that the strong anisotropy introduced by the field will, by way of renormalization, render the effective parameters of the Langevin anisotropic as well. This motivates the more general anisotropic representati... |
the dimension below which nonlinear terms become qualitatively important. To this end, let us use the freedom to independently scale q, ˆq, t, φ, ψ in a manner to leave the dominant quadratic contributions to the action invariant. Defining the scale transformation ˆq → b ˆq, φ → bdφ φ, q → bσq, t → b−zt, ψ → bdψ ψ, (10... |
1; in infinite dimensions, the unlimited number of options to go 43 H. Hinrichsen, Nonequilibrium critical phenomena and phase-transitions into absorbing states, Adv. Phys. 49, 815-958 (2000). 678 Nonequilibrium (classical) Figure 10.13 The two phases of a directed percolation network. Left, dry phase, wherein individua... |
hree distinct phase portraits of directed percolation. Left: phase supporting a finite concentration of active sites, center: phase transition, right: empty state. and κ ≡ (Aλ)1/2.(In deriving Eq. (10.112), we made use of the freedom to rescale fields so as to make the coefficients of the two nonlinear terms ∼ φψ2 and ∼ φ2... |
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