1,729 research outputs found
Cosmology of Antisymmetric Tensor Field in D-brane Universe
We analyze homogeneous, anisotropic cosmology driven by a self-interacting
``massive'' antisymmetric tensor field which is present in string
theories with D-branes. Time-dependent magnetic field existing in the early
universe can lead to the Bianchi type I universe. Evolutions of such a tensor
field are solved exactly or numerically in the universe dominated by vacuum
energy, radiation, and field itself. The matter-like behavior of the
field (dubbed as ``-matter'') ensures that the anisotropy disappears at late
time and thus becomes unobservable in a reasonable cosmological scenario. Such
a feature should be contrasted to the cosmology of the conventional massless
antisymmetric tensor field.Comment: 13 page
Searching for Flavored Gauge Bosons
Standard Model may allow an extended gauge sector with anomaly-free flavored
gauge symmetries, such as , , and ,
where are flavor indices. We investigate phenomenological
implications of the new flavored gauge boson in the above three
classes of gauge symmetries. Focusing on the gauge boson mass above 5 GeV, we
use the lepton universality test in the and decays, LEP
searches, LHC searches, neutrino trident production bound, and LHC
searches to put constraints on the
plane. When is involved, the LEP bounds on
the processes give the most stringent
bounds, while the LHC bound becomes the strongest constraints in the large
region when is involved. The bound from productions, which is applicable for -involved scenarios, provides
stringent bounds in the small region. One exception is the
scenario, in which case only a small region is favored due to the
lepton universality.Comment: v3: updated LHC bounds for B-3L_i model
String Cosmology of the D-brane Universe
We analyze homogeneous anisotropic cosmology driven by the dilaton and the
self-interacting ``massive'' antisymmetric tensor field which are indispensable
bosonic degrees with the graviton in the NS-NS sector of string theories with
D-branes. We found the attractor solutions for this system, which show the
overall features of general solutions, and confirmed it through numerical
analysis. The dilaton possesses the potential due to the presence of the
D-brane and the curvature of extra dimensions. In the presence of the
non-vanishing antisymmetric tensor field, the homogeneous universe expands
anisotropically while the D-brane term dominates. The isotropy is recovered as
the dilaton rolls down and the curvature term dominates. With the stabilizing
potential for the dilaton, the isotropy can also be recovered.Comment: 23 pages, 8 figures. Final version, to appear in Phys. Rev.
Cosmology of Light Moduli
In string/M-theory with a large compactification radius, some axion-like
moduli can be much lighter than the gravitino. Generic moduli in gauge-mediated
supersymmetry breaking models also have a mass far below the weak scale.
Motivated by these, we examine the cosmological implications of light moduli
for the mass range from the weak scale to an extremely small scale of order
10^{-26} eV, and obtain an upper bound on the initial moduli misalignment for
both cases with and without a late entropy production.Comment: 23 pages including 3 pictex-figures, Late
Axino-Neutrino Mixing in Gauge-Mediated Supersymmetry Breaking Models
When the strong CP problem is solved by spontaneous breaking of an anomalous
global symmetry in theories with gauge-mediated supersymmetry breaking, the
pseudo Goldstone fermion (the axino) is a good candidate of a light sterile
neutrino. Its mixing with neutrinos relevant for current neutrino experiments
can arise in the presence of R-parity violation. The realistic four neutrino
mass matrix is obtained when the see-saw mechanism is brought in, and an ansatz
for the right-handed neutrino mass is constructed.Comment: Revtex, 7 pp. Version to appear in Phys. Lett.
- …