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Ivan G. Avramidi

Publications and source records attributed to Ivan G. Avramidi.

At least 19 recordsLinked to original sources

Heat Kernel on Warped Products

We study the spectral properties of the scalar Laplacian on a $n$-dimen\-sional warped product manifold $M=Σ\times_f N$ with a $(n-1)$-dimensional compact manifold $N$ without boundary, a one dimensional manifold $Σ$ without boundary and a warping function $f\in C^\infty(Σ)$. We consider two cases: $Σ=S^1$ when the manifold $M$ is compact, and $Σ=\mathbb{R}$ when the manifold $M$ is non-compact. In the latter case we assume that the warping function $f$ is such that the manifold $M$ has two cusps with a finite volume. In particular, we study the case of the warping function $f(y)=[\cosh(y/b)]^{-2ν/(n-1)}$ in detail, where $y\in\mathbb{R}$ and $b$ and $ν$ are some positive parameters. We study the properties of the spectrum of the Laplacian in detail and show that it has both the discrete and the continuous spectrum. We compute the resolvent, the eigenvalues, the scattering matrix, the heat kernel and the regularized heat trace. We compute the asymptotics of the regularized heat trace of the Laplacian on the warped manifold $M$ and show that some of its coefficients are global in nature expressed in terms of the zeta function on the manifold $N$.

math-ph

On Zero Energy States in SUSY Quantum Mechanics on Manifolds

We study the zero modes of the operator $H_f=D^*_fD_f$, with a Dirac type operator $D_f$, acting on the spinor bundle over a closed even dimensional Riemannian manifold $M$. The operator $D_f=D+ifI$ is a deformation of the Dirac operator $D$ by a smooth function $f$. We obtain sufficient conditions on the deformation function that guarantee the positivity of the operator $H_f$, that is, the absence of zero modes. We also show that these conditions are not necessary and provide an explicit counterexample of a zero mode of the operator $H_f$.

math-ph

Geometric Deformation of Quantum Mechanics

We develop a novel approach to Quantum Mechanics that we call Curved Quantum Mechanics. We introduce an infinite-dimensional Kähler manifold ${\cal M}$, that we call the state manifold, such that the cotangent space $T_z^*{\cal M}$ is a Hilbert space. In this approach, a state of a quantum system is described by a point in the cotangent bundle $T^*{\cal M}$, that is, by a point $z\in{\cal M}$ in the state manifold and a one-form $ψ\in T^*_z{\cal M}$. The quantum dynamics is described by an infinite-dimensional Hamiltonian system on the state manifold with a magnetic field $H$, which reduces to the Schrödinger equation for zero curvature and reduces to the equations of geodesics for zero magnetic field. The curvature of the state manifold is determined by gravity, that is, by the mass/energy of the system, so that for microscopic systems the manifold is flat and for macroscopic systems it is strongly curved, which prohibits Schrödinger cat type states. We solved the dynamical equations exactly for the complex projective space and the complex hyperbolic space and show that in the case of negative curvature there is a bifurcation at a critical value of the curvature. This means that for small mass all modes are in the quantum regime with the unitary periodic dynamics and for large mass there are classical modes, with not a periodic but rather an exponential time evolution leading to a collapse of the state vector.

quant-ph

MOND via Matrix Gravity

MOND theory has arisen as a promising alternative to dark matter in explaining the collection of discrepancies that constitute the so-called missing mass problem. The MOND paradigm is briefly reviewed. It is shown that MOND theory can be incorporated in the framework of the recently proposed Matrix Gravity. In particular, we demonstrate that Matrix Gravity contains MOND as a particular case, which adds to the validity of Matrix Gravity and proves it is deserving of further inquiry.

gr-qc

Spectral Asymptotics of Elliptic Operators on Manifolds

The study of spectral properties of natural geometric elliptic partial differential operators acting on smooth sections of vector bundles over Riemannian manifolds is a central theme in global analysis, differential geometry and mathematical physics. Instead of studying the spectrum of a differential operator $L$ directly one usually studies its spectral functions, that is, spectral traces of some functions of the operator, such as the spectral zeta function $ζ(s)=\Tr L^{-s}$ and the heat trace $Θ(t)=\Tr\exp(-tL)$. The kernel $U(t;x,x')$ of the heat semigroup $\exp(-tL)$, called the heat kernel, plays a major role in quantum field theory and quantum gravity, index theorems, non-commutative geometry, integrable systems and financial mathematics. We review some recent progress in the study of spectral asymptotics. We study more general spectral functions, such as $\Tr f(tL)$, that we call quantum heat traces. Also, we define new invariants of differential operators that depend not only on the their eigenvalues but also on the eigenfunctions, and, therefore, contain much more information about the geometry of the manifold. Furthermore, we study some new invariants, such as $\Tr\exp(-tL_+)\exp(-sL_-)$, that contain relative spectral information of two differential operators. Finally we show how the convolution of the semigroups of two different operators can be computed by using purely algebraic methods.

math-ph

Heat Semigroups on Weyl Algebra

We study the algebra of semigroups of Laplacians on the Weyl algebra. We consider first-order partial differential operators $\nabla^\pm_i$ forming the Lie algebra $[\nabla^\pm_j,\nabla^\pm_k]= i\mathcal{R}^\pm_{jk}$ and $[\nabla^+_j,\nabla^-_k] =i\frac{1}{2}(\mathcal{R}^+_{jk}+\mathcal{R}^-_{jk})$ with some anti-symmetric matrices $\mathcal{R}^\pm_{ij}$ and define the corresponding Laplacians $Δ_\pm=g_\pm^{ij}\nabla^\pm_i\nabla^\pm_j$ with some positive matrices $g_\pm^{ij}$. We show that the heat semigroups $\exp(tΔ_\pm)$ can be represented as a Gaussian average of the operators $\exp\left<ξ,\nabla^\pm\right>$ and use these representations to compute the product of the semigroups, $\exp(tΔ_+)\exp(sΔ_-)$ and the corresponding heat kernel.

math-ph

Relative Spectral Invariants of Elliptic Operators on Manifolds

We introduce and study {\it new} relative spectral invariants of {\it two} elliptic partial differential operators of Laplace and Dirac type on compact smooth manifolds without boundary that depend on both the eigenvalues and the eigensections of these operators and contain much more information about geometry. We prove the existence of the homogeneous short time asymptotics of the new invariants with the coefficients of the asymptotic expansion being integrals of some invariants that depend on the symbols of both operators. The first two coefficients of the asymptotic expansion are computed explicitly.

math-ph

Bogolyubov invariant via relative spectral invariants on manifolds

We introduce and study new spectral invariant of two elliptic partial differential operators of Laplace and Dirac type on compact smooth manifolds without boundary that depends on both the eigenvalues and the eigensections of the operators, which is a equal to the regularized number of created particles from the vacuum when the dynamical operator depends on time. We study the asymptotic expansion of this invariant for small adiabatic parameter and compute explicitly the first two coefficients of the asymptotic expansion.

math-ph

One-Loop quantum gravity in the Einstein universe

We study quantum gravity with the Einstein-Hilbert action including the cosmological constant on the Euclidean Einstein universe $S^1\times S^3$. We compute exactly the spectra and the heat kernels of the relevant operators on $S^3$ and use these results to compute the heat trace of the graviton and ghost operators and the exact one-loop effective action on $S^1\times S^3$. We show that the system is unstable in the infrared limit due to the presence of the negative modes of the graviton and the ghost operators. We study the thermal properties of the model with the temperature $T=(2πa_1)^{-1}$ determined by the radius $a_1$ of the circle $S^1$. We show that the heat capacity $C_v$ is well defined and behaves like $\sim T^3$ in the high temperature limit and has a singularity of the type $\sim (T-T_c)^{-1}$, indicating a second-order phase transition, with the critical temperature $T_c$ determined by the cosmological constant $Λ$ and the radius $a$ of the sphere $S^3$. We also discuss some peculiar properties of the model such as the negative heat capacity as well as possible physical applications.

hep-th

Heat Determinant on Manifolds

We introduce and study new invariants associated with Laplace type elliptic partial differential operators on manifolds. These invariants are constructed by using the off-diagonal heat kernel; they are not pure spectral invariants, that is, they depend not only on the eigenvalues but also on the corresponding eigenfunctions in a non-trivial way. We compute the first three low-order invariants explicitly.

math-ph

Thermal Yang-Mills Theory In the Einstein Universe

We study the stability of a non-Abelian chromomagnetic vacuum in Yang-Mills theory in Euclidean Einstein universe $S^1\times S^3$. We assume that the gauge group is a simple compact group $G$ containing the group SU(2) as a subgroup and consider static covariantly constant gauge fields on $S^3$ taking values in the adjoint representation of the group $G$ and forming a representation of the group $SU(2)$. We compute the heat kernel for the Laplacian acting on fields on $S^3$ in an arbitrary representation of SU(2) and use this result to compute the heat kernels for the gluon and the ghost operators and the one-loop effective action. We show that the only configuration of the covariantly constant Yang-Mills background that is stable is the one that contains only spinor (fundamental) representations of the group SU(2); all other configurations contain negative modes and are unstable. For the stable configuration we compute the asymptotics of the effective action, the energy density, the entropy and the heat capacity in the limits of low/high temperature and small/large volume and show that the energy density has a non-trivial minimum at a finite value of the radius of the sphere $S^3$.

hep-th

Effective Action and Phase Transitions in Thermal Yang-Mills Theory on Spheres

We study the covariantly constant Savvidy-type chromomagnetic vacuum in finite-temperature Yang-Mills theory on the four-dimensional curved spacetime. Motivated by the fact that a positive spatial curvature acts as an effective gluon mass we consider the compact Euclidean spacetime $S^1\times S^1\times S^2$, with the radius of the first circle determined by the temperature $a_1=(2πT)^{-1}$. We show that covariantly constant Yang-Mills fields on $S^2$ cannot be arbitrary but are rather a collection of monopole-antimonopole pairs. We compute the heat kernels of all relevant operators exactly and show that the gluon operator on such a background has negative modes for any compact semi-simple gauge group. We compute the infrared regularized effective action and apply the result for the computation of the entropy and the heat capacity of the quark-gluon gas. We compute the heat capacity for the gauge group SU(2N) for a field configuration of $N$ monopole-antimonopole pairs. We show that in the high-temperature limit the heat capacity is well defined in the infrared limit and exhibits a typical behavior of second-order phase transition $\sim (T-T_c)^{-3/2}$ with the critical temperature $T_c=(2πa)^{-1}$, where $a$ is the radius of the 2-sphere $S^2$.

hep-th

Non-commutative Corrections in Spectral Matrix Gravity

We study a non-commutative deformation of general relativity based on spectral invariants of a partial differential operator acting on sections of a vector bundle over a smooth manifold. We compute the first non-commutative corrections to Einstein equations in the weak deformation limit and analyze the spectrum of the theory. Related topics are discussed as well.

gr-qc

On the Gravitationally Induced Schwinger Mechanism

In this paper we will present very recent results obtained in the ambit of quantum electrodynamics in curved spacetime. We utilize a newly developed non-perturbative heat kernel asymptotic expansion on homogeneous Abelian bundles over Riemannian manifolds in order to compute the one-loop effective action for scalar and spinor fields in curved spacetime under the influence of a strong covariantly constant electromagnetic field. In this framework we derived, in particular, the gravitational corrections, up to linear terms in Riemannian curvature, to Schwinger's result for the creation of particles in a strong electric field.

hep-th

Non-perturbative Effective Action in Gauge Theories and Quantum Gravity

We use our recently developed algebraic methods for the calculation of the heat kernel on homogeneous bundles over symmetric spaces to evaluate the non-perturbative low-energy effective action in quantum general relativity and Yang-Mills gauge theory in curved space. We obtain an exact integral repesentation for the effective action that generates all terms in the standard asymptotic epxansion of the effective action without derivatives of the curvatures effectively summing up the whole infinite subseries of all quantum corrections with low momenta.

hep-th

Low-Energy Effective Action in Non-Perturbative Electrodynamics in Curved Spacetime

We study the heat kernel for the Laplace type partial differential operator acting on smooth sections of a complex spin-tensor bundle over a generic $n$-dimensional Riemannian manifold. Assuming that the curvature of the U(1) connection (that we call the electromagnetic field) is constant we compute the first two coefficients of the non-perturbative asymptotic expansion of the heat kernel which are of zero and the first order in Riemannian curvature and of arbitrary order in the electromagnetic field. We apply these results to the study of the effective action in non-perturbative electrodynamics in four dimensions and derive a generalization of the Schwinger's result for the creation of scalar and spinor particles in electromagnetic field induced by the gravitational field. We discover a new infrared divergence in the imaginary part of the effective action due to the gravitational corrections, which seems to be a new physical effect.

hep-th

Mathematical Tools for Calculation of the Effective Action in Quantum Gravity

We review the status of covariant methods in quantum field theory and quantum gravity, in particular, some recent progress in the calculation of the effective action via the heat kernel method. We study the heat kernel associated with an elliptic second-order partial differential operator of Laplace type acting on smooth sections of a vector bundle over a Riemannian manifold without boundary. We develop a manifestly covariant method for computation of the heat kernel asymptotic expansion as well as new algebraic methods for calculation of the heat kernel for covariantly constant background, in particular, on homogeneous bundles over symmetric spaces, which enables one to compute the low-energy non-perturbative effective action.

hep-th

A Model for the Pioneer Anomaly

In a previous work we showed that massive test particles exhibit a non-geodesic acceleration in a modified theory of gravity obtained by a non-commutative deformation of General Relativity (so-called Matrix Gravity). We propose that this non-geodesic acceleration might be the origin of the anomalous acceleration experienced by the Pioneer 10 and Pioneer 11 spacecrafts.

gr-qc