7,909 research outputs found
"Just So" Neutrino Oscillations Are Back
Recent evidence for oscillations of atmospheric neutrinos at Super-Kamiokande
suggest, in the simplest see-saw interpretation, neutrino masses such that
`just so' vacuum oscillations can explain the solar neutrino deficit. Super-K
solar neutrino data provide preliminary support for this interpretation. We
describe how the just-so signal---an energy dependent seasonal variation of the
event rate, might be detected within the coming years and provide general
arguments constraining the sign of the variation. The expected variation at
radiochemical detectors may be below present sensitivity, but a significant
modulation in the Be signal could shed light on the physics of the solar
core---including a direct measure of the solar core temperature.Comment: 4 pages, revtex, 4 ps figs: new refs added, and Super-K energy
resolution function incorporate
Next-to-Leading Order NMSSM Decays with CP-odd Higgs Bosons and Stops
We compute the full next-to-leading order supersymmetric (SUSY) electroweak
(EW) and SUSY-QCD corrections to the decays of CP-odd NMSSM Higgs bosons into
stop pairs. In our numerical analysis we also present the decay of the heavier
stop into the lighter stop and an NMSSM CP-odd Higgs boson. Both the EW and the
SUSY-QCD corrections are found to be significant and have to be taken into
account for a proper prediction of the decay widths.Comment: 28 pages, 10 figure
Observation of Cosmic Acceleration and Determining the Fate of the Universe
Current observations of Type Ia supernovae provide evidence for cosmic
acceleration out to a redshift of z \lsim 1, leading to the possibility that
the universe is entering an inflationary epoch. However, inflation can take
place only if vacuum-energy (or other sufficiently slowly redshifting source of
energy density) dominates the energy density of a region of physical radius
1/H. We argue that for the best-fit values of and
inferred from the supernovae data, one must confirm cosmic acceleration out to
at least to infer that the universe is inflating.Comment: 4 pages;important changes in conclusion; published in Phys. Rev. Let
Old Galaxies at High Redshift and the Cosmological Constant
In a recent striking discovery, Dunlop {\bf \it et al} observed a galaxy at
redshift z=1.55 with an estimated age of 3.5 Gyr. This is incompatible with age
estimates for a flat matter dominated universe unless the Hubble constant is
less than . While both an open universe, and a universe
with a cosmological constant alleviate this problem, I argue here that this
result favors a non-zero cosmological constant, especially when considered in
light of other cosmological constraints. In the first place, for the favored
range of matter densities, this constraint is more stringent than the globular
cluster age constraint, which already favors a non-zero cosmological constant.
Moreover, the age-redshift relation for redshifts of order unity implies that
the ratio between the age associated with redshift 1.55 and the present age is
also generally larger for a cosmological constant dominated universe than for
an open universe. In addition, structure formation is generally suppressed in
low density cosmologies, arguing against early galaxy formation. The additional
constraints imposed by the new observation on the parameter space of vs
(where ) are derived for both
cosmologies. For a cosmological constant dominated universe this constraint is
consistent with the range allowed by other cosmological constraints, which also
favor a non-zero value.Comment: latex, 10 pages, including two embedded postscript figure
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