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Published on: June 8, 2018
Horizon Edge Partition Functions in Λ>0 Quantum Gravity
Y T Albert Law1, Varun Lochab2
1Leinweber Institute for Theoretical Physics at Stanford, 382 Via Pueblo, Stanford, California 94305, USA.
We analyzed horizon "edge" degrees of freedom for gravity and higher-spin fields in de Sitter and Nariai spacetimes. Novel symmetry breaking in one-loop thermodynamics was revealed, with graviton modes interpreted as cosmic horizon fluctuations.
Area of Science:
- Theoretical physics
- Quantum gravity
- Cosmology
Background:
- Previous analyses explored one-loop thermodynamics using Lorentzian and Euclidean methods.
- Understanding horizon thermodynamics is crucial for quantum gravity.
Purpose of the Study:
- To obtain spectra of codimension-2 horizon
- edge
- degrees of freedom for gravity and higher-spin fields.
- To investigate one-loop thermodynamics in de Sitter and Nariai spacetimes.
- To reveal novel symmetry-breaking structures.
Main Methods:
- Spectral analysis of horizon degrees of freedom.
- One-loop thermodynamic calculations.
- Investigation in de Sitter and Nariai spacetime backgrounds.
Main Results:
- The edge spectra exhibit universal shift symmetries.
- A novel symmetry-breaking structure was found in one-loop partition functions with a positive cosmological constant.
- Graviton modes were geometrically interpreted as cosmic horizon fluctuations, a finding consistent in both spacetimes.
Conclusions:
- The study advances the understanding of one-loop thermodynamics in curved spacetimes.
- The identified symmetry-breaking structure offers new insights into quantum gravity effects.
- The geometric interpretation of graviton modes provides a deeper connection between gravity and horizon physics.
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