TY - JOUR
T1 - A late-accelerating universe with no dark energy—and a finite-temperature big bang
AU - Brown, R.
AU - Maartens, Roy
AU - Papantonopoulos, E.
AU - Zamarias, V.
PY - 2005
Y1 - 2005
N2 - Brane-world models offer the possibility of explaining the late acceleration of the universe via infra-red modifications to general relativity, rather than a dark energy field. However, one also expects ultra-violet modifications to general relativity, when high-energy stringy effects in the early universe begin to grow. We generalize the DGP brane-world model via an ultra-violet modification, in the form of a Gauss–Bonnet term in the bulk action. The combination of infra-red and ultra-violet modifications produces an intriguing cosmology. The DGP feature of late-time acceleration without dark energy is preserved, but there is an entirely new feature—there is no infinite-temperature big bang in the early universe. The universe starts with finite density and pressure, from a 'quiet' and 'sudden' curvature singularity
AB - Brane-world models offer the possibility of explaining the late acceleration of the universe via infra-red modifications to general relativity, rather than a dark energy field. However, one also expects ultra-violet modifications to general relativity, when high-energy stringy effects in the early universe begin to grow. We generalize the DGP brane-world model via an ultra-violet modification, in the form of a Gauss–Bonnet term in the bulk action. The combination of infra-red and ultra-violet modifications produces an intriguing cosmology. The DGP feature of late-time acceleration without dark energy is preserved, but there is an entirely new feature—there is no infinite-temperature big bang in the early universe. The universe starts with finite density and pressure, from a 'quiet' and 'sudden' curvature singularity
U2 - 10.1088/1475-7516/2005/11/008
DO - 10.1088/1475-7516/2005/11/008
M3 - Article
SN - 1475-7516
VL - 2005
SP - 8
EP - 8
JO - Journal of Cosmology and Astroparticle Physics
JF - Journal of Cosmology and Astroparticle Physics
IS - 11
ER -