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Holographic cosmology from the first law of thermodynamics and the generalized uncertainty principle

2009/11/30 by James E. Lidsey · 29 citations
Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Holographic principle #Holography #Laws of thermodynamics #Non-equilibrium thermodynamics #Noncommutative and Quantum Gravity Theories #Physics #Quantum mechanics #Second law of thermodynamics #Statistical physics #Theoretical physics #Thermodynamics #Uncertainty principle #astro-ph.CO #gr-qc #hep-th

paper · pdf · doi:10.1103/physrevd.88.103519

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 88(10) (American Physical Society) · Extended discussion post-Planck results; In press, Physical Review D

arxiv created 2013/09/30 · openalex publication_date 2013/11/14 · arxiv updated 2013/11/20 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The cosmological Friedmann equation sourced by the trace anomaly of a conformal field theory that is dual to the five-dimensional Schwarzschild-AdS geometry can be derived from the first law of thermodynamics if the apparent horizon of the boundary spacetime acquires a logarithmically corrected Bekenstein-Hawking entropy. It is shown that such a correction to the entropy can arise when the generalized uncertainty principle (GUP) is invoked. The necessary condition for such a thermodynamic derivation directly relates the GUP parameter to the conformal anomaly. It is consistent with the existence of a gravitational cutoff at a scale luv\ensuremath\gtrsim√(n)l4 for a theory containing n light species. The absolute minimum in position uncertainty can be identified with the scale at which gravity becomes effectively five dimensional.

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