2,160 research outputs found
Non-decoupling effects of SUSY in the physics of Higgs bosons and their phenomenological implications
We consider a plausible scenario in the Minimal Supersymmetric Standard Model
(MSSM) where all the genuine supersymmetric (SUSY) particles are heavier than
the electroweak scale. In this situation, indirect searches via their radiative
corrections to low energy observables are complementary to direct searches, and
they can be crucial if the SUSY masses are at the TeV energy range. We
summarize the most relevant heavy SUSY radiative effects in Higgs boson physics
and emphasize those that manifest a non-decoupling behaviour. We focus, in
particular, on the SUSY-QCD non-decoupling effects in fermionic Higgs decays,
flavour changing Higgs decays and Yukawa couplings. Some of their
phenomenological implications at future colliders are also studied.Comment: Invited talk given by M. J. Herrero at the X Mexican School of
Particles and Fields, Playa del Carmen, Mexico, November 200
A simple algorithm for optimization and model fitting: AGA (asexual genetic algorithm)
Context. Mathematical optimization can be used as a computational tool to
obtain the optimal solution to a given problem in a systematic and efficient
way. For example, in twice-differentiable functions and problems with no
constraints, the optimization consists of finding the points where the gradient
of the objective function is zero and using the Hessian matrix to classify the
type of each point. Sometimes, however it is impossible to compute these
derivatives and other type of techniques must be employed such as the steepest
descent/ascent method and more sophisticated methods such as those based on the
evolutionary algorithms. Aims. We present a simple algorithm based on the idea
of genetic algorithms (GA) for optimization. We refer to this algorithm as AGA
(Asexual Genetic Algorithm) and apply it to two kinds of problems: the
maximization of a function where classical methods fail and model fitting in
astronomy. For the latter case, we minimize the chi-square function to estimate
the parameters in two examples: the orbits of exoplanets by taking a set of
radial velocity data, and the spectral energy distribution (SED) observed
towards a YSO (Young Stellar Object). Methods. The algorithm AGA may also be
called genetic, although it differs from standard genetic algorithms in two
main aspects: a) the initial population is not encoded, and b) the new
generations are constructed by asexual reproduction. Results. Applying our
algorithm in optimizing some complicated functions, we find the global maxima
within a few iterations. For model fitting to the orbits of exoplanets and the
SED of a YSO, we estimate the parameters and their associated errors.Comment: 10 pages, 8 figures, Astronomy and Astrophysics (in press
Centimetre continuum emission from young stellar objects in Cederblad 110
The low-mass star formation region associated with the reflection nebula
Cederblad 110 in the Chamaeleon I cloud was mapped with the Australian
Telescope Compact Array (ATCA) at 6 and 3.5cm. Altogether 11 sources were
detected, three of which are previously known low mass young stellar objects
associated with the nebula: the illuminating star IRS2 (Class III, Einstein
X-ray source CHX7), the brightest far-infrared source IRS4 (Class I), and the
weak X-ray source CHX10a (Class III). The other young stellar objects in the
region, including the Class 0 protostar candidate Cha-MMS1, were not detected.
The radio spectral index of IRS4 (alpha = 1.7 +/- 0.3) is consistent with
optically thick free-free emission arising from a dense ionized region,
probably a jet-induced shock occurring in the circumstellar material. As the
only Class I protostar with a 'thermal jet' IRS4 is the strongest candidate for
the central source of the molecular outflow found previously in the region. The
emission from IRS2 has a flat spectrum (alpha = 0.05 +/- 0.05) but shows no
sign of polarization, and therefore its origin is likely to be optically thin
free-free emission either from ionized wind or a collimated jet. The strongest
source detected in this survey is a new compact object with a steep negative
spectral index (-1.1) and a weak linear polarization (about 2 %), which
probably represents a background radio galaxy.Comment: 7 pages, 2 Postscript figures. Accepted for publication in Astronomy
& Astrophysic
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