619 research outputs found
Radiation can never again dominate Matter in a Vacuum Dominated Universe
We demonstrate that in a vacuum-energy-dominated expansion phase,
surprisingly neither the decay of matter nor matter-antimatter annihilation
into relativistic particles can ever cause radiation to once again dominate
over matter in the future history of the universe.Comment: updated version, as it will appear in Phys. Rev D. Title change, and
some other minor alteration
Current Acceleration from Dilaton and Stringy Cold Dark Matter
We argue that string theory has all the ingredients to provide us with
candidates for the cold dark matter and explain the current acceleration of our
Universe. In any generic string compactification the dilaton plays an important
role as it couples to the Standard Model and other heavy non-relativistic
degrees of freedom such as the string winding modes and wrapped branes, we
collectively call them stringy cold dark matter. These couplings are
non-universal which results in an interesting dynamics for a rolling dilaton.
Initially, its potential can track radiation and matter while beginning to
dominate the dynamics recently, triggering a phase of acceleration. This
scenario can be realized as long as the dilaton also couples strongly to some
heavy modes. We furnish examples of such modes. We provide analytical and
numerical results and compare them with the current supernovae result. This
favors certain stringy candidates.Comment: 16 pages, 4 figures (colour
Limits on MeV Dark Matter from the Effective Number of Neutrinos
Thermal dark matter that couples more strongly to electrons and photons than
to neutrinos will heat the electron-photon plasma relative to the neutrino
background if it becomes nonrelativistic after the neutrinos decouple from the
thermal background. This results in a reduction in N_eff below the
standard-model value, a result strongly disfavored by current CMB observations.
Taking conservative lower bounds on N_eff and on the decoupling temperature of
the neutrinos, we derive a bound on the dark matter particle mass of m_\chi >
3-9 MeV, depending on the spin and statistics of the particle. For p-wave
annihilation, our limit on the dark matter particle mass is stronger than the
limit derived from distortions to the CMB fluctuation spectrum produced by
annihilations near the epoch of recombination.Comment: 5 pages, 1 figure, discussion added, references added and updated,
labels added to figure, to appear in Phys. Rev.
Effective Hedging of Mortgage Interest Rate Risk
Unfortunately, the hedging effectiveness of the GNMA futures market has been diminished by a lack of understanding of the selection of proper hedge ratios. This paper presents a derivation of the optimal hedge ratio for hedging interest rate risk with a GNMA futures contract. The hedge ratio is then applied to different hedging situations and the results of the traditional and newly derived hedging strategies are examined
Stringy Effects During Inflation and Reheating
We consider inflationary cosmology in the context of string compactifications
with multiple throats. In scenarios where the warping differs significantly
between throats, string and Kaluza-Klein physics can generate potentially
observable corrections to the cosmology of inflation and reheating. First we
demonstrate that a very low string scale in the ground state compactification
is incompatible with a high Hubble scale during inflation, and we propose that
the compactification geometry is altered during inflation. In this
configuration, the lowest scale is just above the Hubble scale, which is
compatible with effective field theory but still leads to potentially
observable CMB corrections. Also in the appropriate region of parameter space,
we find that reheating leads to a phase of long open strings in the Standard
Model sector (before the usual radiation-dominated phase). We sketch the
cosmology of the long string phase and we discuss possible observational
consequences.Comment: 33pp, RevTeX4, v2. minor changes, added ref
Anisotropic higher derivative gravity and inflationary universe
Stability analysis of the Kantowski-Sachs type universe in pure higher
derivative gravity theory is studied in details. The non-redundant generalized
Friedmann equation of the system is derived by introducing a reduced one
dimensional generalized KS type action. This method greatly reduces the labor
in deriving field equations of any complicate models. Existence and stability
of inflationary solution in the presence of higher derivative terms are also
studied in details. Implications to the choice of physical theories are
discussed in details in this paper.Comment: 9 page
Can the Acceleration of Our Universe Be Explained by the Effects of Inhomogeneities?
No. It is simply not plausible that cosmic acceleration could arise within
the context of general relativity from a back-reaction effect of
inhomogeneities in our universe, without the presence of a cosmological
constant or ``dark energy.'' We point out that our universe appears to be
described very accurately on all scales by a Newtonianly perturbed FLRW metric.
(This assertion is entirely consistent with the fact that we commonly encounter
.) If the universe is accurately described by a
Newtonianly perturbed FLRW metric, then the back-reaction of inhomogeneities on
the dynamics of the universe is negligible. If not, then it is the burden of an
alternative model to account for the observed properties of our universe. We
emphasize with concrete examples that it is {\it not} adequate to attempt to
justify a model by merely showing that some spatially averaged quantities
behave the same way as in FLRW models with acceleration. A quantity
representing the ``scale factor'' may ``accelerate'' without there being any
physically observable consequences of this acceleration. It also is {\it not}
adequate to calculate the second-order stress energy tensor and show that it
has a form similar to that of a cosmological constant of the appropriate
magnitude. The second-order stress energy tensor is gauge dependent, and if it
were large, contributions of higher perturbative order could not be neglected.
We attempt to clear up the apparent confusion between the second-order stress
energy tensor arising in perturbation theory and the ``effective stress energy
tensor'' arising in the ``shortwave approximation.''Comment: 20 pages, 1 figure, several footnotes and references added, version
accepted for publication in CQG;some clarifying comments adde
Probing Unstable Massive Neutrinos with Current Cosmic Microwave Background Observations
The pattern of anisotropies in the Cosmic Microwave Background depends upon
the masses and lifetimes of the three neutrino species. A neutrino species of
mass greater than 10 eV with lifetime between 10^{13} sec and 10^{17} sec
leaves a very distinct signature (due to the integrated Sachs-Wolfe effect):
the anisotropies at large angles are predicted to be comparable to those on
degree scales. Present data exclude such a possibility and hence this region of
parameter space. For eV, sec, we find
an interesting possibility: the Integrated Sachs Wolfe peak produced by the
decaying neutrino in low- models mimics the acoustic peak expected in
an model.Comment: 5 pages, 4 figure
Triad representation of the Chern-Simons state in quantum gravity
We investigate a triad representation of the Chern-Simons state of quantum
gravity with a non-vanishing cosmological constant. It is shown that the
Chern-Simons state, which is a well-known exact wavefunctional within the
Ashtekar theory, can be transformed to the real triad representation by means
of a suitably generalized Fourier transformation, yielding a complex integral
representation for the corresponding state in the triad variables. It is found
that topologically inequivalent choices for the complex integration contour
give rise to linearly independent wavefunctionals in the triad representation,
which all arise from the one Chern-Simons state in the Ashtekar variables. For
a suitable choice of the normalization factor, these states turn out to be
gauge-invariant under arbitrary, even topologically non-trivial
gauge-transformations. Explicit analytical expressions for the wavefunctionals
in the triad representation can be obtained in several interesting asymptotic
parameter regimes, and the associated semiclassical 4-geometries are discussed.
In restriction to Bianchi-type homogeneous 3-metrics, we compare our results
with earlier discussions of homogeneous cosmological models. Moreover, we
define an inner product on the Hilbert space of quantum gravity, and choose a
natural gauge-condition fixing the time-gauge. With respect to this particular
inner product, the Chern-Simons state of quantum gravity turns out to be a
non-normalizable wavefunctional.Comment: Latex, 30 pages, 1 figure, to appear in Phys. Rev.
Evaluation of a -defensin in a murine model of herpes simplex virus type 1 keratitis
PURPOSE. To test the activity of a synthetic -defensin, retrocyclin (RC)-2, in a murine herpes simplex virus (HSV)-1 keratitis model. METHODS. The in vitro antiviral activity of RC-2 against HSV-1 KOS was determined by yield reduction and viral inactivation assays. Efficacy in an experimental murine HSV-1 keratitis model was tested using pre-or postinfection treatment with 0.1% peptide in PBS with or without 2% methylcellulose. Viral titers in the tear film were determined by plaque assay. RESULTS. RC-2 inhibited HSV-1 KOS in vitro with an EC 50 of 10 M (ϳ20 g/mL) in yield-reduction assays, but was not directly virucidal. RC-106 (a less active analogue) did not inhibit HSV-1 KOS in culture. Incubating the virus with RC-2 or applying the peptide in 2% methylcellulose to the cornea before viral infection significantly reduced the severity of ocular disease, but postinfection treatment with 0.1% RC-2 in PBS with or without 2% methylcellulose did not. Viral titers were significantly reduced on some days after infection in the preincubation and prophylaxis groups. CONCLUSIONS. RC-2 was active against HSV-1 KOS in cultures and showed protective activity in vivo when used in a prophylactic mode, but the peptide showed limited activity in a postinfection herpes keratitis model. These findings support data obtained from experiments with HIV-1, HSV-2, and influenza A, indicating that RCs inhibit the entry of viruses rather than their replication. (Invest Ophthalmol Vis Sci. 2007;48: 5118 -5124
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