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Ish: Global monopole induced wormholes in power-law gravity: stability and physical viability

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Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
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The cosmological constant and dark energy
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Modified gravity and cosmology
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Extended Theories of Gravity
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The Particle Problem in the General Theory of Relativity
A. Einstein, N. Rosen
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Non-Linear Lagrangians and Cosmological Theory
H. A. Buchdahl
Maqola197040 iqtibos
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Can modified gravity silence radio-loud pulsars?
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INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
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Modified gravity theories on a nutshell: Inflation, bounce and late-time evolution
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Cracking of self-gravitating compact objects
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Sarlavhasiz
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A new type of isotropic cosmological models without singularity
Alexei A. Starobinsky
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Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
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Ether flow through a drainhole: A particle model in general relativity
Homer G. Ellis
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Modified gravity with negative and positive powers of curvature: Unification of inflation and cosmic acceleration
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Causality and Multiply Connected Space-Time
Robert W. Fuller, John Wheeler
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Wormhole geometries in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>modified theories of gravity
Francisco S. N. Lobo, Miguel A. Oliveira
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Gravitational field of a global monopole
Manuel Barriola, Alexander Vilenkin
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Impact of quintessence and cloud of strings on self-consistent d-dimensional charged thin-shell wormholes
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A study of traversable wormhole solutions in extended teleparallel theory of gravity with matter coupling
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Impact of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si5.svg" display="inline" id="d1e24"><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> functions on the dynamical evolution of axially symmetric collapsing stars
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Viscous fluid cosmology: A path to cosmic acceleration
Z. Yousaf
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Further stable neutron star models from<i>f</i>(<i>R</i>) gravity
Artyom V Astashenok, Salvatore Capozziello, Sergei D Odintsov
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