154 research outputs found
Predictions for Higgs and SUSY spectra from SO(10) Yukawa Unification with mu > 0
We use Yukawa unification to constrain SUSY parameter space. We
find a narrow region survives for (suggested by \bsgam and the
anomalous magnetic moment of the muon) with , , \gev and \gev. Demanding Yukawa unification thus makes definite predictions for
Higgs and sparticle masses.Comment: 10 pages, 3 figures, revised version to be published in PR
Sparticle mass spectra from SU(5) SUSY GUT models with Yukawa coupling unification
Supersymmetric grand unified models based on the gauge group SU(5) often
require in addition to gauge coupling unification, the unification of b-quark
and -lepton Yukawa couplings. We examine SU(5) SUSY GUT parameter space
under the condition of Yukawa coupling unification using 2-loop MSSM
RGEs including full 1-loop threshold effects. The Yukawa-unified solutions
break down into two classes. Solutions with low tan\beta ~3-11 are
characterized by gluino mass ~1-4 TeV and squark mass ~1-5 TeV. Many of these
solutions would be beyond LHC reach, although they contain a light Higgs scalar
with mass <123 GeV and so may be excluded should the LHC Higgs hint persist.
The second class of solutions occurs at large tan\beta ~35-60, and are a subset
of unified solutions. Constraining only unification to ~5%
favors a rather light gluino with mass ~0.5-2 TeV, which should ultimately be
accessible to LHC searches. While our unified solutions can be
consistent with a picture of neutralino-only cold dark matter, invoking
additional moduli or Peccei-Quinn superfields can allow for all of our
Yukawa-unified solutions to be consistent with the measured dark matter
abundance.Comment: 19 pages, 5 figures, 1 table, PDFLate
, and in Supersymmetry at Large
We present an effective Lagrangian formalism for the calculation of flavour
changing neutral and charged scalar currents in weak decays including
symmetry breaking effects and the effects of the electroweak
couplings and . We apply this formalism to the MSSM with large
with the CKM matrix as the only source of flavour violation, heavy
supersymmetric particles and light Higgs bosons. We give analytic formulae for
the neutral and charged Higgs boson couplings to quarks including large
resummed corrections in the limit and
demonstrate that these formulae can only be used for a semi-quantitative
analysis. In particular they overestimate the effects of large
resummed corrections. We give also improved analytic formulae that reproduce
the numerical results of the full approach within . We present for the
first time the predictions for the branching ratios
and the mass differences that
include simultaneously the resummed large corrections, breaking effects and the effects of the electroweak couplings. We perform
an anatomy of the correlation between the increase of the rates of the decays
and the suppression of , that for large
are caused by the enhanced flavour changing neutral Higgs couplings
to down quarks. We take into account the constraint from
clarifying some points in the calculation of the large enhanced
corrections to this decay.Comment: 86 pages, 10 postscript figures. Minor changes, some references
added. Version to be published in Nuclear Physics
Neutrino Masses and Lepton-Flavor Violation in Supersymmetric Models with lopsided Froggatt-Nielsen charges
We analyze in detail lepton-flavor violation (LFV) in the charged-lepton
sector such as , , and the
conversion in nuclei, within the framework of supersymmetric models
with lopsided Froggatt--Nielsen charges, in which the large mixing in the
neutrino sector as well as small mixings in the quark sector can be naturally
accommodated. We show that the present experimental limits on the LFV processes
already exclude some of the models. The future proposed search for LFV,
especially in muon processes, can provide a significant probe to this
framework. We also stress the importance of the measurement of
in neutrino experiments, and the fact that the KamLAND experiment could play a
significant role to test a certain class of models.Comment: 33 pages, 20 figure
Correlation between Delta M_s and B^0_{s,d} --> mu^+ mu^- in Supersymmetry at Large tan beta
Considering the MSSM with the CKM matrix as the only source of flavour
violation and heavy supersymmetric particles at large , we analyze
the correlation between {\it the increase} of the rates of the decays
and {\it the suppression} of , that are
caused by the enhanced flavour changing neutral Higgs couplings to down-type
quarks. We give analytic formulae for the neutral and charged Higgs couplings
to quarks including large resummed corrections in the limit and comment briefly on the accuracy of this approximation. For
we find 6\cdot
10^{-7}\ge BR(B^0_s\ra \mu^+\mu^-)^{\rm max} \ge 4\cdot 10^{-8} and 1.4\cdot
10^{-8}\ge BR(B^0_d\ra \mu^+\mu^-)^{\rm max}\ge 1\cdot 10^{-9}. For substantial enhancements of
B^0_{s,d}\ra\mu^+\mu^- relative to the expectations based on the Standard
Model are excluded. With ps a conservative
analysis of gives BR(B^0_s\ra
\mu^+\mu^-)\simlt1.2\cdot10^{-6} and BR(B^0_d\ra
\mu^+\mu^-)\simlt3\cdot10^{-8}. However, we point out that in the less likely
scenario in which the squark mixing is so large that the neutral Higgs
contributions dominate , the rates for
increase with increasing and the bounds in question are weaker.
Violation of all these correlations and bounds would indicate new sources of
flavour violation.Comment: 15 pages, one postscript figur
SUSY GUTs under Siege : Proton Decay
SO(10) supersymmetric grand unified theories [SUSY GUTs] provide a beautiful
framework for physics beyond the standard model. Experimental measurements of
the three gauge couplings are consistent with unification at a scale GeV. In addition predictive models for fermion masses and
mixing angles have been found which fit the low energy data, including the
recent data for neutrino oscillations. SO(10) boundary conditions can be tested
via the spectrum of superparticles. The simplest models also predict neutron
and proton decay rates. In this paper we discuss nucleon decay rates and obtain
reasonable upper bounds. A clear picture of the allowed SUSY spectra as
constrained by nucleon decay is presented.Comment: 13 page
An empirical survey on wireless inductive power pad and resonant magnetic field coupling for in-motion EV charging system
EVs are the recent emerging automotive technology in the transportation sector to reduce
the CO2 emission from the internal combustion engine. The issues in EVs technology development are
battery tube capacity, heavy-size batteries, fast charging, and safe charging infrastructure. The dynamic
wireless charging technology shows a suitable alternative to address the charging system-related issues in
EV. However, a limited number of review studies are conducted to specifically address the wireless charging
pad design challenges. The wireless inductive power pad and magnetic coupling circuit design are the main
factors to decide the performance of the DWPT system. This review analyzes the current developments
and challenges associated with wireless charging pad design. Further, this study investigates the potential
parameters which improve the performance of a DWPT system to increase the distance traveled (mileage).
First, this paper discusses WRIPT technology for DWPT EV charging application, and several parameters
affecting the PTE are examined. Also, the aids factors considered for designing the DWPT power pad and
different magnetic resonance coupling topologies are presented. In addition, the performance evaluation of
the WRIPT power pad, with in-motion testing from the major findings in earlier studies is discussed. Finally,
the challenges and opportunities of the WRIPT power pad for in-motion EV charging applications are also
addressed. The current state of the art of DWPT and its future directions to make DWPT EV charging systems
a full-fledged method are highlighted.Web of Science114693466
On the possible space-time fractality of the emitting source
Using simple space-time implementation of the random cascade model we
investigate numerically a conjecture made some time ago which was joining the
intermittent behaviour of spectra of emitted particles with the possible
fractal structure of the emitting source. We demonstrate that such details are
seen, as expected, in the Bose-Einstein correlations between identical
particles. \\Comment: Thoroughly rewritten and modify version, to be published in Phys.
Rev.
Yukawa Unification as a Window into the Soft Supersymmetry Breaking Lagrangian
We study Yukawa unification, including the effects of a physical neutrino
mass consistent with the Superkamiokande observations, in a string/-brane
inspired Pati-Salam model which allows the most general non-universal scalar
and gaugino masses, including the usual -term contributions which arise in
SO(10). We investigate how the tight constraints from rare decays such as and can provide information about the
family dependent supersymmetry breaking soft Lagrangian, for example the
trilinears associated with the second and third family. Many of our results
also apply to SO(10) to which the model approximately reduces in a limiting
case. In both models we find that Yukawa unification is perfectly viable
providing the non-universal soft masses have particular patterns. In this sense
Yukawa unification acts as a window into the soft supersymmetry breaking
Lagrangian.Comment: References added. 82 pages, 57 figures, Late
Particle Physics Approach to Dark Matter
We review the main proposals of particle physics for the composition of the
cold dark matter in the universe. Strong axion contribution to cold dark matter
is not favored if the Peccei-Quinn field emerges with non-zero value at the end
of inflation and the inflationary scale is superheavy since, under these
circumstances, it leads to unacceptably large isocurvature perturbations. The
lightest neutralino is the most popular candidate constituent of cold dark
matter. Its relic abundance in the constrained minimal supersymmetric standard
model can be reduced to acceptable values by pole annihilation of neutralinos
or neutralino-stau coannihilation. Axinos can also contribute to cold dark
matter provided that the reheat temperature is adequately low. Gravitinos can
constitute the cold dark matter only in limited regions of the parameter space.
We present a supersymmetric grand unified model leading to violation of Yukawa
unification and, thus, allowing an acceptable b-quark mass within the
constrained minimal supersymmetric standard model with mu>0. The model
possesses a wide range of parameters consistent with the data on the cold dark
matter abundance as well as other phenomenological constraints. Also, it leads
to a new version of shifted hybrid inflation.Comment: 32 pages including 6 figures, uses svmult.cls, some clarifications
added, lectures given at the Third Aegean Summer School "The Invisible
Universe: Dark Matter and Dark Energy", 26 September-1 October 2005, Karfas,
Island of Chios, Greece (to appear in the proceedings
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