120 research outputs found
Cosmology of "Visible" Sterile Neutrinos
We point out that in scenarios with a low reheating temperature
MeV at the end of (the last episode of) inflation or entropy production, the
abundance of sterile neutrinos becomes largely independent of their coupling to
active neutrinos. Thus, cosmological bounds become less stringent than usually
assumed, allowing sterile neutrinos to be ``visible'' in future experiments.
For example, the sterile neutrino required by the LSND result does not have any
cosmological problem within these scenarios.Comment: Talk given at the ``8th Workshop on Non-Perturbative Quantum
Chromodynamics", June 7-11, 2004, Paris, France; 7 pages, 2 figure
Theory of Dark Matter
The search for dark matter is a very wide and active field of research. Many
potential hints of dark matter have appeared recently which led to a burst of
theoretical activity and model building. I necessarily concentrate here only in
some aspects of it. I review here some recent hints and some of the ways in
which they could be explained.Comment: Plenary review talk at "Physics at the LHC 2010", 7-12 June 2010,
DESY, Hamburg, Germany; 6 pages, no figures, desyproc.cls file needed to
typese
Experimental relevance of low reheating temperature cosmologies
Standard simple assumptions are usually made about the pre-Big Bang
Nucleosynthesis epoch, from which we do not have observations. Modifying these
assumptions, the predicted density of relic particles such as neutralinos and
sterile neutrinos can be very different from that in the standard case. For
example, neutralinos could have the dark matter density in (almost) any
supersymmetric model, and sterile neutrinos with mixings large enough to be
soon detected in neutrino experiments would become cosmologically acceptable.
These possibilities are important in view of what the LHC, and neutrino
experiments could soon find.Comment: Talk given at the 43rd Rencontres de Moriond- Cosmology, La Thuile,
Italy, March 15 - 22, 2008. 4 pages, 3 figures, uses moriond.st
Neutralino with the Right Cold Dark Matter Abundance in (Almost) Any Supersymmetric Model
We consider non-standard cosmological models in which the late decay of a
scalar field reheats the Universe to a low reheating temperature,
between 5 MeV and the standard freeze-out temperature of neutralinos of mass
. We point out that in these models all neutralinos with standard
density can have the
density of cold dark matter, provided the right combination of the following
two parameters can be achieved in the high energy theory: the reheating
temperature, and the ratio of the number of neutralinos produced per
decay over the field mass. We present the ranges of these parameters
where a combination of thermal and non-thermal neutralino production leads to
the desired density, as functions of and .Comment: 4 pages, 1 figur
Low reheating temperatures in monomial and binomial inflationary potentials
We investigate the allowed range of reheating temperature values in light of
the Planck 2015 results and the recent joint analysis of Cosmic Microwave
Background (CMB) data from the BICEP2/Keck Array and Planck experiments, using
monomial and binomial inflationary potentials. While the well studied
inflationary potential is no longer favored by current CMB data, as well as
with , a potential and canonical reheating ()
provide a good fit to the CMB measurements. In this last case, we find that the
Planck 2015 confidence limit upper bound on the spectral index, ,
implies an upper bound on the reheating temperature of , and excludes instantaneous reheating. The low reheating
temperatures allowed by this model open the possiblity that dark matter could
be produced during the reheating period instead of when the Universe is
radiation dominated, which could lead to very different predictions for the
relic density and momentum distribution of WIMPs, sterile neutrinos, and
axions. We also study binomial inflationary potentials and show the effects of
a small departure from a potential. We find that as a subdominant
term in the potential increases, first instantaneous reheating becomes
allowed, and then the lowest possible reheating temperature of is excluded by the Planck 2015 confidence limit.Comment: 17 pages, 5 figures, v2: some references added and typos correcte
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