52 research outputs found
Quantum Gravity Effects in Black Holes at the LHC
We study possible back-reaction and quantum gravity effects in the
evaporation of black holes which could be produced at the LHC through a
modification of the Hawking emission. The corrections are phenomenologically
taken into account by employing a modified relation between the black hole mass
and temperature. The usual assumption that black holes explode around TeV
is also released, and the evaporation process is extended to (possibly much)
smaller final masses. We show that these effects could be observable for black
holes produced with a relatively large mass and should therefore be taken into
account when simulating micro-black hole events for the experiments planned at
the LHC.Comment: 14 pages, 8 figures, extended version of hep-ph/0601243 with new
analysis of final products, final version accepted for publication in J.
Phys.
Cosmological constraints on R-parity violation from neutrino decay
If the neutrino mass is non-zero, as hinted by several experiments, then
R-parity-violating supersymmetric Yukawa couplings can drive a heavy neutrino
decay into lighter states. The heavy neutrino may either decay radiatively into
a lighter neutrino, or it may decay into three light neutrinos through a
Z-mediated penguin. For a given mass of the decaying neutrino, we calculate its
lifetime for the various modes, each mode requiring certain pairs of
R-parity-violating couplings be non-zero. We then check whether the calculated
lifetimes fall in zones allowed or excluded by cosmological requirements. For
the latter case, we derive stringent new constraints on the corresponding
products of R-parity-violating couplings for given values of the decaying
neutrino mass.Comment: 13 pages, Latex, uses axodraw.sty; version to appear in Physical
Review
On the Spontaneous CP Breaking at Finite Temperature in a Nonminimal Supersymmetric Standard Model
We study the spontaneous CP breaking at finite temperature in the Higgs
sector in the Minimal Supersymmetric Standard Model with a gauge singlet. We
consider the contribution of the standard model particles and that of stops,
charginos, neutralinos, charged and neutral Higgs boson to the one-loop
effective potential. Plasma effects for all bosons are also included. Assuming
CP conservation at zero temperature, so that experimental constraints coming
from, {\it e.g.}, the electric dipole moment of the neutron are avoided, and
the electroweak phase transition to be of the first order and proceeding via
bubble nucleation, we show that spontaneous CP breaking cannot occur inside the
bubble mainly due to large effects coming from the Higgs sector. However,
spontaneous CP breaking can be present in the region of interest for the
generation of the baryon asymmetry, namely inside the bubble wall. The
important presence of very tiny explicit CP violating phases is also commented.Comment: 28 pages, 4 figures available upon request, DFPD 94/TH/38 and SISSA
94/81-A preprint
How generic is cosmic string formation in SUSY GUTs
We study cosmic string formation within supersymmetric grand unified
theories. We consider gauge groups having a rank between 4 and 8. We examine
all possible spontaneous symmetry breaking patterns from the GUT down to the
standard model gauge group. Assuming standard hybrid inflation, we select all
the models which can solve the GUT monopole problem, lead to baryogenesis after
inflation and are consistent with proton lifetime measurements. We conclude
that in all acceptable spontaneous symmetry breaking schemes, cosmic string
formation is unavoidable. The strings which form at the end of inflation have a
mass which is proportional to the inflationary scale. Sometimes, a second
network of strings form at a lower scale. Models based on gauge groups which
have rank greater than 6 can lead to more than one inflationary era; they all
end by cosmic string formation.Comment: 31 pages, Latex, submitted to PR
Recycling universe
If the effective cosmological constant is non-zero, our observable universe
may enter a stage of exponential expansion. In such case, regions of it may
tunnel back to the false vacuum of an inflaton scalar field, and inflation with
a high expansion rate may resume in those regions. An ``ideal'' eternal
observer would then witness an infinite succession of cycles from false vacuum
to true, and back. Within each cycle, the entire history of a hot universe
would be replayed. If there were several minima of the inflaton potential, our
ideal observer would visit each one of these minima with a frequency which
depends on the shape of the potential. We generalize the formalism of
stochastic inflation to analyze the global structure of the universe when this
`recycling' process is taken into account.Comment: 43 pages, 10 figure
Inflation in Supersymmetric Unified Theories
We construct supersymmetric unified models which automatically lead to a
period of inflation. The models all involve a U(1) symmetry which does not
belong to the MSSM. We consider three different types of models depending on
whether this extra U(1) is the subgroup of a non abelian gauge group, is a U(1)
factor belonging to the visible sector or is a U(1) factor belonging to the
hidden sector. Depending on the structure of the unified theory, on the
spontaneous symmetry breaking pattern and on whether we have global or local
supersymmetry, inflation may be driven by the non-vanishing vacuum expectation
value of a F-term or by that of a D-term. In both scenarios cosmic strings form
at the end of inflation, and they have different properties in each model. Both
inflation and cosmic strings contribute to the CMBR temperature anisotropies.
We show that the strings contribute to the 's up to the level of 75 %.
Hence the contribution from strings to the CMBR and to the density
perturbations in the early Universe which lead to structure formation cannot be
neglected. We also discuss a very interesting class of models which involve a
gauge symmetry.Comment: 22 pages, uses Revte
Non-perturbative renormalization of QCD
In these lectures, we discuss different types of renormalization problems in
QCD and their non-perturbative solution in the framework of the lattice
formulation. In particular the recursive finite size methods to compute the
scale-dependence of renormalized quantities is explained. An important
ingredient in the practical applications is the Schr\"odinger functional. It is
introduced and its renormalization properties are discussed.
Concerning applications, the computation of the running coupling and the
running quark mass are covered in detail and it is shown how the
-parameter and renormalization group invariant quark mass can be
obtained. Further topics are the renormalization of isovector currents and
non-perturbative Symanzik improvement.Comment: 49 pages, lectures at Schladming-9
Crescimento dos frutos de laranjeira 'Salustiana' situados em ramos anelados com diversas relações de folhas/frutos
A relação entre a área foliar e o crescimento dos frutos é um tema que freqüentemente recebe a atenção dos pesquisadores, por influenciar diretamente na produtividade das plantas e na qualidade dos frutos. Neste trabalho, avaliou-se o efeito da área foliar sobre o crescimento dos frutos da laranjeira 'Salustiana'. Foram utilizados ramos com 12 meses de idade e com apenas um fruto terminal. Os ramos foram anelados visando a manter diversas relações de folhas/fruto. Avaliaram-se, semanalmente, o crescimento dos frutos e os teores de amido presentes nas folhas durante um período de 42 dias. O crescimento dos frutos, avaliado na "fase de crescimento II", dependeu da área foliar disponível por fruto, sendo que 30 folhas foram suficientes para garantir o seu crescimento. As reservas de amido nas folhas dependeram da área foliar disponível por fruto e reduziram à medida que os frutos apresentaram aumentos no diâmetro e nas massas fresca e seca.The relationship between the foliar area and the fruit growth is an important theme because affects the tree productivity and fruits quality. In this work was evaluated the effect of the foliar area on the growth of the Salustiana's sweet orange fruits. Girdled shoots of 12 months were used with a single terminal fruit and several leaves-fruit ratios. It was evaluated, weekly, the fruit growth and the leaves starch contents during 42 days. The fruit growth, evaluated in the stage II, depended on the available leaf area per fruit, provided that 30 leaves were enough to guarantee its growth. The starch reserves in the leaves depended on the available leaf area per fruit and they reduced with the increase in the diameter and dry and fresh weight of the fruits
Demonstration of Ignition Radiation Temperatures in Indirect-Drive Inertial Confinement Fusion Hohlraums
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