A thermodynamically inspired modified cosmology with parameter n changes expansion history and structure growth, claimed to falsify both flat and non-flat Lambda CDM while satisfying future thermodynamic equilibrium.
Padmanabhan, Emergence and Expansion of Cosmic Space as due to the Quest for Holographic Equipartition (6 2012)
2 Pith papers cite this work, alongside 51 external citations. Polarity classification is still indexing.
abstract
One possible interpretation of the holographic principle is the equality of the number of degrees of freedom in a bulk region of space and the number of degrees of freedom on the boundary surface. It is known that such an equality is maintained on equipotential surfaces in any static spacetime in the form of an equipartition law N_{bulk}= N_{sur}. In the cosmological context, the de Sitter universe obeys the same holographic equipartition. I argue that the difference between the surface degrees of freedom and the bulk degrees of freedom in a region of space (which has already emerged) drives the accelerated expansion of the universe through a simple equation dV/dt = (N_{sur} - N_{bulk}) where V is the Hubble volume in Planck units and t is the cosmic time in Planck units. This equation reproduces the standard evolution of the universe. This approach provides a novel paradigm to study the emergence of space and cosmology and has far reaching implications.
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gr-qc 2years
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UNVERDICTED 2roles
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background 2representative citing papers
A two-parameter extension of Bekenstein entropy is applied to derive the Friedmann equations and confirm thermodynamic consistency for an accelerating universe via entropy balance and maximization.
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Cosmological dynamics and structure formation in a generalized mass-to-horizon entropy-inspired modified gravity
A thermodynamically inspired modified cosmology with parameter n changes expansion history and structure growth, claimed to falsify both flat and non-flat Lambda CDM while satisfying future thermodynamic equilibrium.
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Generalized Mass-to-Horizon Entropy and Horizon Thermodynamics
A two-parameter extension of Bekenstein entropy is applied to derive the Friedmann equations and confirm thermodynamic consistency for an accelerating universe via entropy balance and maximization.