Perturbative Methods in Gravity Theory

A special issue of Universe (ISSN 2218-1997). This special issue belongs to the section "Gravitation".

Deadline for manuscript submissions: closed (31 January 2022) | Viewed by 2335

Special Issue Editor


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Guest Editor
Institute of Physics, Faculty of Science and Technology, University of Tartu, Wilhelm Ostwaldi 1, 50411 Tartu, Estonia
Interests: geometry in physics; multi-metric gravity; area metric gravity; Finsler gravity; Cartan geometry; quantum manifolds; category theory

Special Issue Information

Dear Colleagues,

The theory of small perturbations around a given exact background solution, with the aim of constructing approximate solutions by a perturbative expansion of a set of field equations, is one of the most important tools employed in the study of gravity theories. In the most simple case, the background solution is assumed to be maximally symmetric, such as Minkowski spacetime, leading to the well-known Newtonian and post-Newtonian approximations, as well as the description of gravitational waves. Relaxing the symmetry to only spatial homogeneity and isotropy leads to the theory of cosmological perturbations, which is the most important framework for assessing the viability of cosmological models using precision observations such as the angular spectrum of the cosmic microwave background. Another application, which has gained a significant amount of importance with the possibility of observing gravitational waves, is the perturbation of black hole spacetimes, which is used to model the gravitational waves emitted during the inspiral and ringdown phases of a merger event.

The aim of this Special Issue is to focus on the development of perturbative methods and their application in the field of gravity theory, including, but not limited to:

  1. the role of gauge invariance and its use in gauge-invariant formalisms;
  2. parametrized frameworks, such as the parametrized post-Newtonian formalism, and the further development of such frameworks in other areas of gravity theory;
  3. the study of modified gravity theories and extensions of general relativity using perturbation theory;
  4. observations in gravity and the measurement of perturbative quantities;
  5. perturbations beyond the metric paradigm and alternative geometric descriptions of spacetime; and
  6. tools for performing analytical and numerical calculations of perturbations in gravity theory.

Dr. Manuel Hohmann
Guest Editor

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Keywords

  • perturbation theory
  • general relativity
  • modified gravity
  • approximate solutions
  • parametrized formalisms

Published Papers (1 paper)

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Research

12 pages, 332 KiB  
Communication
ISCOs and OSCOs in the Presence of a Positive Cosmological Constant in Massive Gravity
by Ángel Rincón, Grigoris Panotopoulos, Ilídio Lopes and Norman Cruz
Universe 2021, 7(8), 278; https://doi.org/10.3390/universe7080278 - 1 Aug 2021
Cited by 4 | Viewed by 1401
Abstract
We study the impact of a non-vanishing (positive) cosmological constant on the innermost and outermost stable circular orbits (ISCOs and OSCOs, respectively) within massive gravity in four dimensions. The gravitational field generated by a point-like object within this theory is known, generalizing the [...] Read more.
We study the impact of a non-vanishing (positive) cosmological constant on the innermost and outermost stable circular orbits (ISCOs and OSCOs, respectively) within massive gravity in four dimensions. The gravitational field generated by a point-like object within this theory is known, generalizing the usual Schwarzschild–de Sitter geometry of General Relativity. In the non-relativistic limit, the gravitational potential differs by the one corresponding to the Schwarzschild–de Sitter geometry by a term that is linear in the radial coordinate with some prefactor γ, which is the only free parameter. Starting from the geodesic equations for massive test particles and the corresponding effective potential, we obtain a polynomial of fifth order that allows us to compute the innermost and outermost stable circular orbits. Next, we numerically compute the real and positive roots of the polynomial for several different structures (from the hydrogen atom to stars and globular clusters to galaxies and galaxy clusters) considering three distinct values of the parameter γ, determined using physical considerations, such as galaxy rotation curves and orbital precession. Similarly to the Kottler spacetime, both ISCOs and OSCOs appear. Their astrophysical relevance as well as the comparison with the Kottler spacetime are briefly discussed. Full article
(This article belongs to the Special Issue Perturbative Methods in Gravity Theory)
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