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Isolated objects in quadratic gravity = from action principles to observations /

Record Type:	Electronic resources : Monograph/item
Title/Author:	Isolated objects in quadratic gravity/ by Samuele Silvervalle.
Reminder of title:	from action principles to observations /
Author:	Silvervalle, Samuele.
Published:	Cham :Springer Nature Switzerland : : 2024.,
Description:	xiii, 192 p. :ill. (some col.), digital ;24 cm.
Notes:	"Doctoral thesis accepted by University of Trento, Trento, Italy."
[NT 15003449]:	Introduction -- Quadratic Gravity -- Analytical approximations and numerical methods -- The Phase Diagram of Quadratic Gravity -- Solutions of Quadratic Gravity -- Quasi-normal Modes and Stability of the Solutions.
Contained By:	Springer Nature eBook
Subject:	General relativity (Physics) -
Online resource:	https://doi.org/10.1007/978-3-031-48994-5
ISBN:	9783031489945

Isolated objects in quadratic gravity = from action principles to observations /
Silvervalle, Samuele.

Isolated objects in quadratic gravityfrom action principles to observations /[electronic resource] :by Samuele Silvervalle. - Cham :Springer Nature Switzerland :2024. - xiii, 192 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5061. - Springer theses..

"Doctoral thesis accepted by University of Trento, Trento, Italy."

Introduction -- Quadratic Gravity -- Analytical approximations and numerical methods -- The Phase Diagram of Quadratic Gravity -- Solutions of Quadratic Gravity -- Quasi-normal Modes and Stability of the Solutions.

One of the main unanswered question of modern Physics is "How does gravity behave at small scales?". The aim of this thesis is to illustrate in a comprehensive but accessible way how to look for deviations from Einstein's theory of General Relativity in this regime, looking at the simplest celestial bodies: static and spherically symmetric ones. With a conservative and bottom-up approach, at smaller scales the first corrections to the action of General Relativity are generally considered to be terms quadratic in the curvature tensors; while these modifications do not cure the inconsistency between gravity and quantum mechanics, the solutions of this theory are plausible candidates to be the first-order corrections of the classical ones. Even with such simple modifications, a striking picture emerges from the study of isolated objects: the unique Schwarzschild solution of General Relativity is only a rare bird in the set of solutions, with non-Schwarzschild black holes, wormholes and naked singularities appearing as possible substitutes. Tailored to graduate students and researchers entering this field, this thesis shows how to construct these new solutions from action principles, how to characterize their metric, how to study their physical properties, such as their stability or Thermodynamics, and how to look for phenomenological signatures.

ISBN: 9783031489945

Standard No.: 10.1007/978-3-031-48994-5doiSubjects--Topical Terms:

533948
General relativity (Physics)

LC Class. No.: QC173.6

Dewey Class. No.: 530.11

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505 0 $a Introduction -- Quadratic Gravity -- Analytical approximations and numerical methods -- The Phase Diagram of Quadratic Gravity -- Solutions of Quadratic Gravity -- Quasi-normal Modes and Stability of the Solutions.
520 $a One of the main unanswered question of modern Physics is "How does gravity behave at small scales?". The aim of this thesis is to illustrate in a comprehensive but accessible way how to look for deviations from Einstein's theory of General Relativity in this regime, looking at the simplest celestial bodies: static and spherically symmetric ones. With a conservative and bottom-up approach, at smaller scales the first corrections to the action of General Relativity are generally considered to be terms quadratic in the curvature tensors; while these modifications do not cure the inconsistency between gravity and quantum mechanics, the solutions of this theory are plausible candidates to be the first-order corrections of the classical ones. Even with such simple modifications, a striking picture emerges from the study of isolated objects: the unique Schwarzschild solution of General Relativity is only a rare bird in the set of solutions, with non-Schwarzschild black holes, wormholes and naked singularities appearing as possible substitutes. Tailored to graduate students and researchers entering this field, this thesis shows how to construct these new solutions from action principles, how to characterize their metric, how to study their physical properties, such as their stability or Thermodynamics, and how to look for phenomenological signatures.
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