SCENARIOS OF COSMIC STRING WITH A VARIABLE COSMOLOGICAL CONSTANT
From MaRDI portal
Publication:5325582
DOI10.1142/S0218271809014753zbMath1181.83251arXivastro-ph/0610519OpenAlexW2015461163MaRDI QIDQ5325582
Saibal Ray, Utpal Mukhopadhyay, Farook Rahaman
Publication date: 10 August 2009
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/astro-ph/0610519
Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Cites Work
- Acceleration field of a universe modeled as a mixture of scalar and matter fields
- Negative energies on the brane
- Cosmological constant -- the weight of the vacuum
- Energy density in general relativity: a possible role for the cosmological constant
- Nonsingular vacuum cosmologies with a variable cosmological term
- Closed timelike curves produced by pairs of moving cosmic strings: Exact solutions
- Can vacuum decay in our universe?
- A space–time in toroidal coordinates
- The cosmological constant problem
- A FLUID OF STRINGS AS A VIABLE CANDIDATE FOR THE DARK SIDE OF THE UNIVERSE
- Cosmic strings and domain walls
This page was built for publication: SCENARIOS OF COSMIC STRING WITH A VARIABLE COSMOLOGICAL CONSTANT
