Dependence of the induced vacuum energy of scalar matter in the background of an impenetrable magnetic tube on the coupling to the space-time curvature
- URL: http://arxiv.org/abs/2412.06814v1
- Date: Sun, 01 Dec 2024 21:01:23 GMT
- Title: Dependence of the induced vacuum energy of scalar matter in the background of an impenetrable magnetic tube on the coupling to the space-time curvature
- Authors: V. M. Gorkavenko, A. O. Zaporozhchenko, M. S. Tsarenkova,
- Abstract summary: We consider the vacuum polarization of a quantized charged scalar matter field in the background of a finite-thickness tube with magnetic flux inside.
For generalized Robin boundary conditions, the total induced vacuum energy depends on the coupling $xi$ in flat space-time.
- Score: 0.0
- License:
- Abstract: We considered the vacuum polarization of a quantized charged scalar matter field in the background of a finite-thickness tube with magnetic flux inside. The tube is impenetrable for quantum matter and a Robin-type boundary condition is imposed at its surface. We have shown that in the flat space-time the total induced vacuum energy does not depend on the coupling $(\xi)$ of the scalar field's interaction with the space-time curvature only for the partial cases of the Dirichlet and Neumann boundary conditions on the tube's edge. However, for generalized Robin boundary conditions, the total induced energy depends on the coupling $\xi$ in flat space-time, at least for negative values of the boundary condition parameter $-\pi/2<\theta<0$.
Related papers
- Dynamical Aharonov-Bohm cages and tight meson confinement in a $\mathbb{Z}_2$-loop gauge theory [44.99833362998488]
We study the finite-density phases of a $mathbbZ$ lattice gauge theory (LGT) of interconnected loops and dynamical $mathbbZ$ charges.
arXiv Detail & Related papers (2024-12-17T00:26:24Z) - Hamiltonians for Quantum Systems with Contact Interactions [49.1574468325115]
We show that in the limit one obtains the one-body Hamiltonian for the light particle subject to $N$ (non-local) point interactions placed at fixed positions.
We will verify that such non-local point interactions do not exhibit the ultraviolet pathologies that are present in the case of standard local point interactions.
arXiv Detail & Related papers (2024-07-09T14:04:11Z) - Quantum electrodynamics of lossy magnetodielectric samples in vacuum: modified Langevin noise formalism [55.2480439325792]
We analytically derive the modified Langevin noise formalism from the established canonical quantization of the electromagnetic field in macroscopic media.
We prove that each of the two field parts can be expressed in term of particular bosonic operators, which in turn diagonalize the electromagnetic Hamiltonian.
arXiv Detail & Related papers (2024-04-07T14:37:04Z) - Hamiltonian for a Bose gas with Contact Interactions [49.1574468325115]
We study the Hamiltonian for a Bose gas in three dimensions of $N geq 3$ spinless particles interacting via zero-range or contact interactions.
arXiv Detail & Related papers (2024-03-19T10:00:12Z) - The Fermionic Entanglement Entropy and Area Law for the Relativistic Dirac Vacuum State [44.99833362998488]
We consider the fermionic entanglement entropy for the free Dirac field in a bounded spatial region of Minkowski spacetime.
An area law is proven in the limiting cases where the volume tends to infinity and/or the regularization length tends to zero.
arXiv Detail & Related papers (2023-10-05T12:08:03Z) - Measurement phase transitions in the no-click limit as quantum phase
transitions of a non-hermitean vacuum [77.34726150561087]
We study phase transitions occurring in the stationary state of the dynamics of integrable many-body non-Hermitian Hamiltonians.
We observe that the entanglement phase transitions occurring in the stationary state have the same nature as that occurring in the vacuum of the non-hermitian Hamiltonian.
arXiv Detail & Related papers (2023-01-18T09:26:02Z) - Induced vacuum energy density of quantum charged scalar matter in the
background of an impenetrable magnetic tube with the Neumann boundary
condition [0.0]
We consider vacuum polarization of charged scalar matter field outside the tube with magnetic flux inside.
We show that vacuum energy is periodic in the value of the magnetic flux of the tube.
It is shown that the value of the induced vacuum energy density in the case of the Neumann boundary condition is greater than in the case of the Dirichlet boundary condition.
arXiv Detail & Related papers (2022-12-07T17:36:13Z) - Magnetic flux in the vacuum of quantum bosonic matter in the cosmic
string background [0.0]
The relativistic spin-0 matter field is quantized in the background of a straight cosmic string with nonvanishing transverse size.
The role of the bound states in the spectrum of solutions to the Fock-Klein-Gordon equation is elucidated.
The dependence of the induced vacuum magnetic flux on the string flux and tension, as well as on the transverse size of the string, is analyzed.
arXiv Detail & Related papers (2022-08-12T17:46:03Z) - Induced vacuum magnetic field in the cosmic string background [0.0]
We find that a magnetic field is induced in the vacuum and that a sheath in the form of a tube of the magnetic flux lines encloses a cosmic string.
The dependence of the induced vacuum magnetic field strength on the string flux and tension, as well as on the transverse size of the string, is unambiguously determined.
arXiv Detail & Related papers (2021-03-10T17:47:05Z) - Quantum vacuum effects in braneworlds on AdS bulk [0.0]
Two geometries are considered: a brane parallel to the AdS boundary and a brane intersecting the AdS boundary.
The contribution in the vacuum expectation value (VEV) of the energy-momentum tensor is separated explicitly.
The influence of the gravitational field on the local properties of the quantum vacuum is essential at distance from the brane.
arXiv Detail & Related papers (2020-09-17T14:01:17Z) - The Casimir densities for a sphere in the Milne universe [0.0]
The influence of a spherical boundary on the vacuum fluctuations of a massive scalar field is investigated in background of $(D+1)$-dimensional Milne universe.
The normalized mode functions are derived for the regions inside and outside the sphere and different vacuum states are discussed.
As important local characteristics of the vacuum state the vacuum expectation values (VEVs) of the field squared and of the energy-momentum tensor are investigated.
arXiv Detail & Related papers (2020-02-25T11:20:49Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.