Fetching the paper…
Reading the bibliography…
The sensitivity of the lightest supersymmetric particle relic density calculation to the variation of the cosmological expansion rate before nucleosynthesis is discussed.
B. Ratra & P.J.E. Peebles, Cosmological Consequences of a Rolling Homogeneous Scalar Field
1988
Earlier work this paper cites.
J. Ellis, T. Falk, K.A. Olive & M. Schmitt, Constraints on neutralino dark matter from LEP-2 and cosmology
1997
Earlier work this paper cites.
P. Gondolo & G. Gelmini, Cosmic abundances of stable particles: Improved analysis
1997
Earlier work this paper cites.
S. Burles & D. Tytler, The Deuterium abundance towards Q1937-1009
1998
Earlier work this paper cites.
C. Armendariz-Picon et al
2001
Earlier work this paper cites.
B.C. Allanach, SOFTSUSY: A C++ program for calculating supersymmetric spectra
2002
Cited alongside, same era.
J. Ellis et al
2003
Cited alongside, same era.
M. Kamionkowski & M.S. Turner, Thermal relics: Do we know their abundances?
2003
Cited alongside, same era.
P. Gondolo et al
2004
Cited alongside, same era.
V. Barger et al
2004
Cited alongside, same era.
Cited in the paper.
W.-M. Yao et al
2006
Later among the works it cites.
G. Bélanger et al
2007
Later among the works it cites.
A. Arbey, Is it possible to consider dark energy and dark matter as a same and unique dark fluid?
2007
Later among the works it cites.
F. Mahmoudi, New constraints on supersymmetric models from b → s γ b\to s\gamma
2007
Later among the works it cites.
2067
Closest in time.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…