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Иш: Physical viability of the general relativistic wormholes sourced by dark matter distributions

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Wormholes in spacetime and their use for interstellar travel: A tool for teaching general relativity
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Einstein-Gauss-Bonnet Gravity in Four-Dimensional Spacetime
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Wormholes, Time Machines, and the Weak Energy Condition
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Static Solutions of Einstein's Field Equations for Spheres of Fluid
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Local anisotropy in self-gravitating systems
L. Herrera
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Ether flow through a drainhole: A particle model in general relativity
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History of dark matter
Gianfranco Bertone, Dan Hooper
Мақола201816 иқтибос
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A family of potential-density pairs for spherical galaxies and bulges
Walter Dehnen
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Modified theories of gravity: Why, how and what?
S. Shankaranarayanan, Joseph P. Johnson
Мақола202213 иқтибос
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Viscous fluid cosmology: A path to cosmic acceleration
Z. Yousaf
Мақола202512 иқтибос
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Geons
John Wheeler
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Generalized uncertainty principle corrections in Rastall–Rainbow Casimir wormholes
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Imprints of monopole charge in Morris-Thorne type wormholes and energy conditions under the influence of higher dimensional gravity
Enhua Dai, M. Yousaf, Faisal Javed +2
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Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles
Aaron A. Dutton, Andrea V. Macciò
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Spin, torsion and violation of null energy condition in traversable wormholes
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Testing wormhole solutions in extended gravity through the Poynting-Robertson effect
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New definition of complexity for self-gravitating fluid distributions: The spherically symmetric, static case
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A theory of dark matter
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Reconstructing wormhole solutions in curvature based Extended Theories of Gravity
Vittorio De Falco, Emmanuele Battista, Salvatore Capozzıello +1
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Traversable Wormholes in f(R) Gravity: Influence of Global Monopole Charge and Energy Conditions
H. Asad, M. Yousaf, Ujala Zafar +2
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Imprints of global monopole charge on the stability and energy conditions of traversable wormholes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si2.svg" display="inline" id="d1e1938"> <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> gravity
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