Density perturbation and cosmological evolution in the presence of magnetic field in \(f(R)\) gravity models
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Publication:2084487
DOI10.1155/2022/5195251zbMath1496.83046arXiv2111.14898OpenAlexW3215633545MaRDI QIDQ2084487
Sarbari Guha, Samarjit Chakraborty
Publication date: 18 October 2022
Published in: Advances in High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2111.14898
Cites Work
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- Fluid dynamics in higher order gravity
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- <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
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- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- Modified Gravity Models of Dark Energy
- The Nature of Primordial Fluctuations from Anisotropic Inflation
- Perturbations in Bianchi I universes
- Magnetic brane-worlds
- General relativistic orthonormal frame approach
- Partially locally rotationally symmetric perfect fluid cosmologies
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- CURVATURE QUINTESSENCE
- A dynamical systems approach to Bianchi cosmologies: orthogonal models of class A
- Asymptotic states of magnetic Bianchi VI cosmologies
- Small-scale CMB anisotropies induced by the primordial magnetic fields
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Dynamical systems analysis of anisotropic cosmologies in R n -gravity
- Shear dynamics in Bianchi I cosmologies with R n -gravity
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