1,099 research outputs found
Adiabatic CMB perturbations in pre-big bang string cosmology
We consider the pre-big bang scenario with a massive axion field which starts
to dominate energy density when oscillating in an instanton-induced potential
and subsequently reheats the universe as it decays into photons, thus creating
adiabatic CMB perturbations. We find that the fluctuations in the axion field
can give rise to a nearly flat spectrum of adiabatic perturbations with a
spectral tilt in the range .Comment: 15 pages, 1 figure; Version to appear in Nucl.Phys.B. Figure
improved, discussion and one reference adde
Numerical simulations of fragmentation of the Affleck-Dine condensate
We present numerical simulations of fragmentation of the Affleck-Dine
condensate in two spatial dimensions. We argue analytically that the final
state should consist of both Q-balls and anti-Q-balls in a state of maximum
entropy, with most of the balls small and relativistic. Such a behaviour is
found in simulations on a 100x100 lattice with cosmologically realistic
parameter values. During fragmentation process, we observe filament-like
texture in the spatial distribution of charge. The total charge in Q-balls is
found to be almost equal to the charge in anti-Q-balls and typically orders of
magnitude larger than charge asymmetry. Analytical considerations indicate
that, apart from geometrical factors, the results of the simulated two
dimensional case should apply also to the fully realistic three dimensional
case.Comment: 28 pages, 39 figure
Q-ball formation in the gravity-mediated SUSY breaking scenario
We study the formation of Q-balls which are made of flat directions that
appear in the supersymmetric extension of the standard model in the context of
gravity-mediated supersymmetry breaking. The full non-linear calculations for
the dynamics of the complex scalar field are made. Since the scalar potential
in this model is flatter than \phi^2, we have found that fluctuations develop
and go non-linear to form non-topological solitons, Q-balls. The size of a
Q-ball is determined by the most amplified mode, which is completely determined
by the model parameters. On the other hand, the charge of Q-balls depends
linearly on the initial charge density of the Affleck-Dine (AD) field. Almost
all the charges are absorbed into Q-balls, and only a tiny fraction of the
charges is carried by a relic AD field. It may lead to some constraints on the
baryogenesis and/or parameters in the particle theory. The peculiarity of
gravity-mediation is the moving Q-balls. This results in collisions between
Q-balls. It may increase the charge of Q-balls, and change its fate.Comment: 9 pages, RevTex, 11 postscript figures included, to appear in Phys.
Rev.
Searching for a holographic connection between dark energy and the low-l CMB multipoles
We consider the angular power spectrum in a finite universe with different
boundary conditions and perform a fit to the CMB, LSS and supernova data. A
finite universe could be the consequence of a holographic constraint, giving
rise to an effective IR cutoff at the future event horizon. In such a model
there is a cosmic duality relating the dark energy equation of state and the
power spectrum, which shows a suppression and oscillatory behaviour that is
found to describe the low l features extremely well. However, much of the
discussion here will also apply if we actually live inside an expanding bubble
that describes our universe. The best fit to the CMB and LSS data turns out to
be better than in the standard Lambda-CDM model, but when combined with the
supernova data, the holographic model becomes disfavored. We speculate on the
possible implications.Comment: 16 pages, 5 figures, to appear in JCA
Q-ball Formation through Affleck-Dine Mechanism
We present the full nonlinear calculation of the formation of a Q-ball
through the Affleck-Dine (AD) mechanism by numerical simulations. It is shown
that large Q-balls are actually produced by the fragmentation of the condensate
of a scalar field whose potential is very flat. We find that the typical size
of a Q-ball is determined by the most developed mode of linearized
fluctuations, and almost all the initial charges which the AD condensate
carries are absorbed into the formed Q-balls, whose sizes and the charges
depend only on the initial charge densities.Comment: 4 pages, RevTex, 3 postscript figures included, the published versio
Solitosynthesis of Q-balls
We study the formation of Q-balls in the early universe, concentrating on
potentials with a cubic or quartic attractive interaction. Large Q-balls can
form via solitosynthesis, a process of gradual charge accretion, provided some
primordial charge assymetry and initial ``seed'' Q-balls exist. We find that
such seeds are possible in theories in which the attractive interaction is of
the form , with a light ``Higgs'' mass. Condensate formation
and fragmentation is only possible for masses in the sub-eV range;
these Q-balls may survive untill present.Comment: 9 pages, 1 figur
Seed perturbations for primordial magnetic fields from MSSM flat directions
We demonstrate that the MSSM flat directions can naturally account for the
seed magnetic fields in the early Universe. The non-zero vacuum expectation
value of an MSSM flat direction condensate provides masses to the gauge fields
and thereby breaks conformal invariance. During inflation the condensate
receives spatial perturbations and gauge currents are
generated together with (hyper)magnetic fields. When these long wavelength
vector perturbations reenter our horizon they give rise to magnetic
fields with an amplitude of Gauss, as required by the dynamo
mechanism.Comment: 4 pages, RevTeX
Q-ball formation: Obstacle to Affleck-Dine baryogenesis in the gauge-mediated SUSY breaking ?
We consider the Affleck-Dine baryogenesis comprehensively in the minimal
supersymmetric standard model with gauge-mediated supersymmetry breaking.
Considering the high temperature effects, we see that the Affleck-Dine field is
naturally deformed into the form of the Q ball. In the natural scenario where
the initial amplitude of the field and the A-terms are both determined by the
nonrenormalizable superpotential, we obtain only very a narrow allowed region
in the parameter space in order to explain the baryon number of the universe
for the case that the Q-ball formation occurs just after baryon number
production. Moreover, most of the parameter sets suited have already been
excluded by current experiments. We also find new situations in which the
Q-ball formation takes place rather late compared with baryon number creation.
This situation is more preferable, since it allows a wider parameter region for
naturally consistent scenarios, although it is still difficult to realize in
the actual cosmological scenario.Comment: 27 pages, RevTeX, 21 postscript figures included. The version to be
publishe
Neutrino oscillations in the early universe: How large lepton asymmetry can be generated?
The lepton asymmetry that could be generated in the early universe through
oscillations of active to sterile neutrinos is calculated (almost) analytically
for small mixing angles, sin 2\theta < 10^{-2}. It is shown that for a mass
squared difference, \delta m^2=-1 eV^2 it may rise at most by 6 orders of
magnitude from the initial ``normal'' value of 10^{-10}, since the
back-reaction from the refraction index terminates this rise while the
asymmetry is still small. Only for very large mass differences, \delta m^2
about 10^9 eV^2, the lepton asymmetry could reach a significant magnitude
exceeding 0.1.Comment: 25 pages, LaTeX (5 graphs
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