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S. P. Klevansky

Publications and source records attributed to S. P. Klevansky.

At least 37 records · Page 2Linked to original sources

Coupled Oscillator Systems Having Partial PT Symmetry

This paper examines chains of $N$ coupled harmonic oscillators. In isolation, the $j$th oscillator ($1\leq j\leq N$) has the natural frequency $ω_j$ and is described by the Hamiltonian $\frac{1}{2}p_j^2+\frac{1}{2}ω_j^2x_j^2$. The oscillators are coupled adjacently with coupling constants that are purely imaginary; the coupling of the $j$th oscillator to the $(j+1)$st oscillator has the bilinear form $iγx_jx_{j+1}$ ($γ$ real). The complex Hamiltonians for these systems exhibit {\it partial} $\mathcal{PT}$ symmetry; that is, they are invariant under $i\to-i$ (time reversal), $x_j\to-x_j$ ($j$ odd), and $x_j\to x_j$ ($j$ even). [They are also invariant under $i\to-i$, $x_j\to x_j$ ($j$ odd), and $x_j\to- x_j$ ($j$ even).] For all $N$ the quantum energy levels of these systems are calculated exactly and it is shown that the ground-state energy is real. When $ω_j=1$ for all $j$, the full spectrum consists of a real energy spectrum embedded in a complex one; the eigenfunctions corresponding to real energy levels exhibit partial $\mathcal{PT}$ symmetry. However, if the $ω_j$ are allowed to vary away from unity, one can induce a phase transition at which {\it all} energies become real. For the special case $N=2$, when the spectrum is real, the associated classical system has localized, almost-periodic orbits in phase space and the classical particle is confined in the complex-coordinate plane. However, when the spectrum of the quantum system is partially real, the corresponding classical system displays only open trajectories for which the classical particle spirals off to infinity. Similar behavior is observed when $N>2$.

quant-ph↗

Systems of coupled PT-symmetric oscillators

The Hamiltonian for a PT-symmetric chain of coupled oscillators is constructed. It is shown that if the loss-gain parameter $γ$ is uniform for all oscillators, then as the number of oscillators increases, the region of unbroken PT-symmetry disappears entirely. However, if $γ$ is localized in the sense that it decreases for more distant oscillators, then the unbroken-PT-symmetric region persists even as the number of oscillators approaches infinity. In the continuum limit the oscillator system is described by a PT-symmetric pair of wave equations, and a localized loss-gain impurity leads to a pseudo-bound state. It is also shown that a planar configuration of coupled oscillators can have multiple disconnected regions of unbroken PT symmetry.

math-ph↗

Generation of families of spectra in PT-symmetric quantum mechanics and scalar bosonic field theory

This paper explains the systematics of the generation of families of spectra for the PT-symmetric quantum-mechanical Hamiltonians $H=p^2+x^2(ix)^ε$, $H=p^2+(x^2)^δ$, and $H=p^2-(x^2)^μ$. In addition, it contrasts the results obtained with those found for a bosonic scalar field theory, in particular in one dimension, highlighting the similarities and differences to the quantum-mechanical case. It is shown that the number of families of spectra can be deduced from the number of noncontiguous pairs of Stokes' wedges that display PT-symmetry. To do so, simple arguments that use the WKB approximation are employed, and these imply that the eigenvalues are real. However, definitive results are in most cases presently only obtainable numerically, and not all eigenvalues in each family may be real. Within the approximations used, it is illustrated that the difference between the quantum-mechanical and the field-theoretical cases lies in the number of accessible regions in which the eigenfunctions decay exponentially. This paper reviews and implements well-known techniques in complex analysis and PT-symmetric quantum theory.

hep-th↗

Negative-energy PT-symmetric Hamiltonians

The non-Hermitian PT-symmetric quantum-mechanical Hamiltonian $H=p^2+x^2(ix)^ε$ has real, positive, and discrete eigenvalues for all $ε\geq 0$. These eigenvalues are analytic continuations of the harmonic-oscillator eigenvalues $E_n=2n+1$ (n=0, 1, 2, 3, ...) at $ε=0$. However, the harmonic oscillator also has negative eigenvalues $E_n=-2n-1$ (n=0, 1, 2, 3, ...), and one may ask whether it is equally possible to continue analytically from these eigenvalues. It is shown in this paper that for appropriate PT-symmetric boundary conditions the Hamiltonian $H=p^2+x^2(ix)^ε$ also has real and {\it negative} discrete eigenvalues. The negative eigenvalues fall into classes labeled by the integer N (N=1, 2, 3, ...). For the Nth class of eigenvalues, $ε$ lies in the range $(4N-6)/3<ε<4N-2$. At the low and high ends of this range, the eigenvalues are all infinite. At the special intermediate value $ε=2N-2$ the eigenvalues are the negatives of those of the conventional Hermitian Hamiltonian $H=p^2+x^{2N}$. However, when $ε\neq 2N-2$, there are infinitely many complex eigenvalues. Thus, while the positive-spectrum sector of the Hamiltonian $H=p^2+x^2(ix)^ε$ has an unbroken PT symmetry (the eigenvalues are all real), the negative-spectrum sector of $H=p^2+x^2(ix)^ε$ has a broken PT symmetry (only some of the eigenvalues are real).

hep-th↗

PT-Symmetric Representations of Fermionic Algebras

A recent paper by Jones-Smith and Mathur extends PT-symmetric quantum mechanics from bosonic systems (systems for which $T^2=1$) to fermionic systems (systems for which $T^2=-1$). The current paper shows how the formalism developed by Jones-Smith and Mathur can be used to construct PT-symmetric matrix representations for operator algebras of the form $η^2=0$, $\barη^2=0$, $η\barη+\bar η =α1$, where $\bar{eta}=η^{PT} =PT ηT^{-1}P^{-1}$. It is easy to construct matrix representations for the Grassmann algebra ($α=0$). However, one can only construct matrix representations for the fermionic operator algebra ($α\neq0$) if $α= -1$; a matrix representation does not exist for the conventional value $α=1$.

hep-th↗

Response to Shalaby's Comment on "Families of Particles with Different Masses in PT-Symmetric Quantum Field Theory"

In a recent Comment [arXiv: 1101.3980] Shalaby criticised our paper "Families of Particles with Different Masses in PT-Symmetric Quantum Field Theory" [arXiv:1002.3253]. On examining his arguments, we find that there are serious flaws at almost every stage of his Comment. In view of space and time considerations, we point out the major flaws that render his arguments invalid. Essentially Shalaby is attempting to obtain our results from a variational principle and to find a physical interpretation of his calculation. The variational procedure that he uses is inapplicable, and his description of the physics is wrong. We thus refute his criticism on all levels.

hep-th↗

Families of particles with different masses in PT-symmetric quantum field theory

An elementary field-theoretic mechanism is proposed that allows one Lagrangian to describe a family of particles having different masses but otherwise similar physical properties. The mechanism relies on the observation that the Dyson-Schwinger equations derived from a Lagrangian can have many different but equally valid solutions. Nonunique solutions to the Dyson-Schwinger equations arise when the functional integral for the Green's functions of the quantum field theory converges in different pairs of Stokes' wedges in complex field space, and the solutions are physically viable if the pairs of Stokes' wedges are PT symmetric.

hep-th↗

Nonunique C operator in PT Quantum Mechanics

The three simultaneous algebraic equations, $C^2=1$, $[C,PT]=0$, $[C,H]=0$, which determine the $C$ operator for a non-Hermitian $PT$-symmetric Hamiltonian $H$, are shown to have a nonunique solution. Specifically, the $C$ operator for the Hamiltonian $H={1/2}p^2+{1/2}μ^2q^2+iεq^3$ is determined perturbatively to first order in $ε$ and it is demonstrated that the $C$ operator contains an infinite number of arbitrary parameters. For each different $C$ operator, the corresponding equivalent isospectral Dirac-Hermitian Hamiltonian $h$ is calculated.

hep-th↗

Collision integral in a model for scalar quarks and gluons

A model of scalar quarks and scalar gluons is used to derive transport equations for quarks and gluons. In particular, the collision integral is studied. The self-energy diagrams are organized according to the number of loops. A generalized Boltzmann equation is obtained, which involves at the level up to two loops all possible two -> two parton scattering processes and corrections to the process q bar q -> g.

hep-ph↗

Classification of higher order diagrams in non-equilibrium theory, and the removal of pinch singularities

The non-equilibrium two loop self-energy is reexamined in the framework of a scalar quark and gluon model, with specific attention to terms which do not give rise to the standard two -> two particle collisional terms in the semi-classical Boltzmann equation. It is shown that most of these terms contribute to renormalization of component lines at a lower level, rendering the theory correct to (gm)^4. This result can be generalized to a higher number of loops. The remaining terms, which do not fall into any physical category, are shown explicitly to vanish. We then examine the possibility that pinch singularities could arise in this theory, and demonstrate that this is not so for the case of equilibrium and small deviations from equilibrium, at the two loop level.

hep-ph↗

Collision integral for multigluon production in a scalar quark and gluon model

A model of scalar gluons and scalar quarks that successfully gives a ln s behavior in high energy qq scattering and which contains a three gluon vertex is used to derive transport equations for the quarks and gluons. Quasiparticle and semiclassical approximations are utilized. In particular, the collision integral is studied. At first the terms are organized according to the number of gluon exchange interactions, and it is shown explicitly that the occurrence of all two body differential scattering cross sections in the Boltzmann equation requires an evaluation of all terms to this order. One obtains qg-> qg, q bar q->gg, qq->qq, and q bar q -> q bar q. An additional ordering according to the inverse number of colors reveals that the quark loop diagrams are suppressed, and diagrams that lead to gluon production or scattering dominate. The self energy with three gluons exchanged is then examined. From this, it is evident that initial as well as final state interactions enter into a generalized collision integral. The generalized Boltzmann-like equation involving n gluon exchange for quark transport is given.

hep-ph↗

The Das-Mathur-Okubo sum rule for the charged pion polarizability in a chiral model

The Das-Mathur-Okubo (DMO) sum rule for the polarizability of charged pions is evaluated for the Nambu-Jona-Lasinio model Lagrangian in both its minimal and extended forms. A comparison is made with the results obtained using the same sum rule from chiral perturbation theory (CHPT), approximate QCD sum rule calculations, explicit calculations on the lattice by Wilcox, and using the semi-empirical Kapusta-Shuryak spectral densities. The $χ$PT results from Compton scattering are also given. We point to a delicate cancellation between the intrinsic and recoil contributions to $α_{π^\pm}$ in the DMO sum rule approach that can lead to calculated polarizabilities of either sign.

hep-ph↗

Chiral symmetry breaking in hot matter

This series of three lectures covers (a) a basic introduction to symmetry breaking in general and chiral symmetry breaking in QCD, (b) an overview of the present status of lattice data and the knowlegde that we have at finite temperature from chiral perturbation theory. (c) Results obtained from the Nambu--Jona-Lasinio model describing static mesonic properties are discussed as well as the bulk thermodynamic quantities. Divergences that are observed in the elastic quark-antiquark scattering cross-section, reminiscent of the phenomenon of critical opalescence in light scattering, is also discussed. (d) Finally, we deal with the realm of systems out of equilibrium, and examine the effects of a medium dependent condensate in a system of interacting quarks.

hep-ph↗

Transition rates for q q bar -> pi pi pi in a chiral model

We investigate the nature of transition rates for the hadronization process of q q bar -> Pi Pi Pi as opposed to the transition rates for q q bar -> Pi Pi, within the Nambu--Jona-Lasinio model that has manifest chiral symmetry. Feynman diagrams appropriate to this process can be classified according to the expansion in the inverse number of colors 1/N_c. Two of these types of graphs are seen to be either 's-like' or 't-like' in nature. A further graph that contains both s-like and t-like elements, and which is denoted as st-like, is also present. To describe such a process with two incoming and three outgoing particles, it is necessary to extend the number of Mandelstam invariants. It is convenient to introduce seven such variables, of which only five are independent. The cross section for two incoming particles to three outgoing particles is then reexpressed in integral form in terms of these invariants. As a function of sqrt s, the final expression is reduced to an integral over the four remaining invariants. The limits of integration, which are now non-trivial, are also discussed. The transition rate for the explicit case of u u bar -> Pi^+ Pi^- Pi^0, is evaluated numerically, assuming non-chiral pions, m_Pi = 135MeV. The rate for three pion production is found to be of the same order of magnitude as for two pion production, making this a non-negligible contribution to hadronization.

hep-ph↗

$π$-$K$ scattering lengths at finite temperature in the Nambu--Jona-Lasinio model

The transition amplitude for $πK$ scattering is evaluated within the SU(3) Nambu--Jona-Lasinio model. Ordering terms according to the expansion in $1/N_c$ leads to a box-like diagram, $t$ channel diagrams that admit scalar isoscalar $(σ,σ')$ exchanges, and a $u$ channel exchange of a scalar isodoublet $σ_K$ that has quantum numbers corresponding to the $K_0^*(1430)$. Both the Pauli-Villars and O(3) regularization procedures are used to evaluate the T=0 values of the $l=0$ scattering lengths $a_0^{3/2}$ and $a_0^{1/2}$. The finite temperature dependence is studied. We find that the variation in the $t$ channel in the calculation of $a_0^{3/2}$ leads to a change in $a_0^{3/2}$ of a factor of about two over the temperature range of T=150 MeV.

hep-ph↗

$ππ$ scattering in the $ρ$-meson channel at finite temperature

We study $ππ$ scattering in the I=1, $J^P=1^-$ channel at finite temperature in the framework of the extended Nambu-Jona-Lasinio model that explicitly includes vector and axial-vector degrees of freedom in addition to the usual scalar and pseudoscalar sector. The S-matrix in the coupled channels $q\bar q$ and $ππ$ is constructed via $ρ$-exchange in the $s$-channel. The self-energy of the $ρ$-meson contains both quark and pion loop contributions. The analytic structure of the S-matrix for $T\geq 0$ is investigated and the motion of the $ρ$-pole as a function of coupling constant and temperature is followed in the complex $\sqrt{s}$-plane. For numerical calculations, parameters are chosen in order that $m_π$, $f_π$ and the experimental $ππ$ phase shifts $δ_1^1$ at zero temperature are reproduced, and then the behavior of the $ρ$-pole as well as the $ππ$ cross section is investigated as a function of the temperature. We find that the position of the $ρ$ mass stays practically constant for $0\leq T\leq 130$ MeV, and then moves down in energy by about 200 MeV for 130 MeV$\leq T\leq 230$ MeV.

nucl-th↗

Derivation of transport equations for a strongly interacting Lagrangian in powers of $\hbar$ and $1/N_c$

Transport theory for an interacting fermionic system is reviewed and applied to the chiral Lagrangian of the Nambu-Jona-Lasinio model. Two expansions must be applied: an expansion in the inverse number of colors, $1/N_c$, due to the nature of the strong coupling theory, and a semiclassical expansion, in powers of $\hbar$. The quasiparticle approximation is implemented at an early stage, and spin effects are omitted. The self-energy is evaluated, self-consistently only in the Hartree approximation, and semi-perturbatively in the collision integral. In the Hartree approximation, $O((1/N_c)^0)$, the Vlasov equation is recovered to $O(\hbar^1)$, together with an on-mass shell constraint equation, that is automatically fulfilled by the quasiparticle ansatz. The expressions for the self-energy to order $O((1/N_c))$ lead to the collision term. Here one sees explicitly that particle-antiparticle creation and annihilation processes are suppressed that would otherwise be present, should an off-shell energy spectral function be admitted. A clear identification of the $s$, $t$ and $u$ channel scattering processes in connection with the self-energy graphs is made and the origin of the mixed terms is made evident. Finally, after ordering according to powers in $\hbar$, a Boltzmann-like form for the collision integral is obtained.

hep-ph↗

Spectral Density Functions and Their Sum Rules in an Effective Chiral Field Theory

The validity of Weinberg's two sum rules for massless QCD, as well as the six additional sum rules introduced into chiral perturbation theory by Gasser and Leutwyler, are investigated for the extended Nambu-Jona-Lasinio chiral model that includes vector and axial vector degrees of freedom. A detailed analysis of the vector, axial vector and coupled pion plus longitudinal axial vector modes is given. We show that, under Pauli-Villars regularization of the meson polarization amplitudes that determine the spectral density functions, all of the sum rules involving inverse moments higher than zero are automatically obeyed by the model spectral densities. By contrast, the zero moment sum rules acquire a non-vanishing right hand side that is proportional to the quark condensate density of the non-perturbative groundstate. We use selected sum rules in conjunction with other calculations to obtain explicit expressions for the scale-independent coupling constants $\bar l_i$ of chiral perturbation theory in the combination $\bar l_i+\ln(m^2_π/μ^2)$, to evaluate the Das-Guralnik-Mathur-Low-Young current algebra expression for the electromagnetic mass difference of the pion, and to compute the pion electrical polarizability $α_E$. The sum rule calculations %of $α_E$ set an upper limit of $α_E\leq α/(8π^2m_πf^2_π) \approx 6\times10^{-4}$fm$^3$ on this quantity, that is independent of the quark mass up to ${\cal O}(m^2_π/m^2)$, and only depends on the fundamental constants: pion mass $m_π$ and pion decay constant $f_π$, in addition to fine structure constant $α\approx 1/137$.

hep-ph↗