On a physical description and origin of the cosmological constant
From MaRDI portal
Publication:5218326
DOI10.1088/1361-6382/aae445zbMath1431.83063arXiv1810.00683OpenAlexW2894459085MaRDI QIDQ5218326
Publication date: 2 March 2020
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1810.00683
Relativistic cosmology (83F05) Black holes (83C57) Quantization of the gravitational field (83C45) Gravitational energy and conservation laws; groups of motions (83C40) Quantum coherence, entanglement, quantum correlations (81P40)
Related Items (4)
A proposal for Heisenberg uncertainty principle and STUR for curved backgrounds: an application to white dwarf, neutron stars and black holes ⋮ The cosmological constant from Planckian fluctuations and the averaging procedure ⋮ A new equation for a scalar field from thermodynamics first law and its cosmological implications ⋮ The physical nature of the cosmological constant and the decoherence scale in a renormalization-group approach
Cites Work
- Unnamed Item
- First law of thermodynamics for dynamical apparent horizons and the entropy of Friedmann universes
- Why there is nothing rather than something: A theory of the cosmological constant
- The quantum structure of spacetime of the Planck scale and quantum fields
- Entropy, temperature and internal energy of trapped gravitons and corrections to the black hole entropy
- Macroscopic aspects of the Unruh effect
- Entropy, energy and temperature–length inequality for Friedmann universes
- Building non-commutative spacetimes at the Planck length for Friedmann flat cosmologies
- On decoherence in quantum gravity
- Physically motivated uncertainty relations at the Planck length for an emergent non-commutative spacetime
- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><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>theories of gravity
- The cosmological constant and dark energy
- Why the Cosmological Constant Is Small and Positive
- Statistical description of massless excitations within a sphere with a linear equation of state and the dark energy case
- The cosmological constant problem
- The cosmological constant
- On average properties of inhomogeneous fluids in general relativity: Perfect fluid cosmologies
This page was built for publication: On a physical description and origin of the cosmological constant