Interacting modified Chaplygin gas in f(T) gravity framework and analysis of its stability against gravitational perturbation

DOI10.1142/S0219887817500359zbMath1364.83030MaRDI QIDQ2980089

Surajit Chattopadhyay

Publication date: 27 April 2017

Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)

zbMATH Keywords

cosmological evolutionmodified Chaplygin gas\(f(T)\) gravitygravitational perturbationprimordial perturbations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items

A study on the bouncing behavior of modified Chaplygin gas in presence of bulk viscosity and its consequences in the modified gravity framework, A reconstruction scheme for f(T) gravity and its consequences in the perturbation level, Reconstruction of f(T) gravity in the context of standard Chaplygin gas as tachyon scalar field and study of the stability against gravitational perturbation

Cites Work

• Periodic cosmological evolutions of equation of state for dark energy
• Effective \(F(T)\) gravity from the higher-dimensional Kaluza-Klein and Randall-Sundrum theories
• \(f(R)\) theories
• Power-law solutions in \(f(T)\) gravity
• On the thermodynamic stability of the modified Chaplygin gas
• Instability of holographic dark energy models
• Density evolution in the new modified Chaplygin gas model
• Modified Chaplygin gas cosmology
• FRW cosmology with the extended Chaplygin gas
• Constraining the parameters of modified Chaplygin gas in Einstein-Aether gravity
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• Holographic polytropic \(f(T)\) gravity models
• Israel-Stewart approach to viscous dissipative extended holographic Ricci dark energy dominated universe
• Dark energy and gravity
• THERMODYNAMICAL DESCRIPTION OF THE INTERACTING NEW AGEGRAPHIC DARK ENERGY
• f(T) GRAVITY FROM HOLOGRAPHIC RICCI DARK ENERGY MODEL WITH NEW BOUNDARY CONDITIONS
• THE LAWS OF THERMODYNAMICS AND THERMODYNAMIC STABILITY OF THE MODIFIED CHAPLYGIN GAS
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• The cosmological constant and dark energy
• Matter bounce cosmology with the f ( T ) gravity
• DYNAMICS OF DARK ENERGY
• RECONSTRUCTING DARK ENERGY
• Thermodynamics of dark energy
• Role of modified Chaplygin gas in accelerated universe
• CURVATURE QUINTESSENCE
• RECONSTRUCTION OF MODIFIED GRAVITY WITH GHOST DARK ENERGY MODELS
• INSTABILITY OF QCD GHOST DARK ENERGY MODEL
• Modified Chaplygin gas cosmology with bulk viscosity
• The universe dominated by the extended Chaplygin gas
• HOLOGRAPHIC MODIFIED GRAVITY
• ENTROPY CORRECTED HOLOGRAPHIC DARK ENERGY f(T) GRAVITY MODEL
• The covariant formulation of f ( T ) gravity
• An alternative to quintessence
• No further gravitational wave modes in \(F(T)\) gravity