20,647 research outputs found
Markoff-Rosenberger triples in geometric progression
Solutions of the Markoff-Rosenberger equation ax^2+by^2+cz^2 = dxyz such that
their coordinates belong to the ring of integers of a number field and form a
geometric progression are studied.Comment: To appear in Acta Mathematica Hungaric
An algorithm for determining torsion growth of elliptic curves
We present a fast algorithm that takes as input an elliptic curve defined
over and an integer and returns all the number fields of
degree dividing such that contains as a
proper subgroup, for all . We ran this algorithm on all
elliptic curves of conductor less than 400.000 (a total of 2.483.649 curves)
and all and collected various interesting data. In particular, we
find a degree 6 sporadic point on , which is so far the lowest known
degree a sporadic point on , for .Comment: 15 pages, Added Supplementary materia
Strangeness on the nucleon
Observables from parity violation in elastic electron-nucleon scattering and
neutral current quasi-elastic neutrino-nucleus scattering are employed as tools
to improve the current knowledge on the strangeness content in the nucleon.Comment: Proceedings of International Scientific Meeting on Nuclear Physics,
9-13th September 2012. La R\'abida, Huelva, Spai
Markoff-Rosenberger triples in arithmetic progression
We study the solutions of the Rosenberg--Markoff equation ax^2+by^2+cz^2 =
dxyz (a generalization of the well--known Markoff equation). We specifically
focus on looking for solutions in arithmetic progression that lie in the ring
of integers of a number field. With the help of previous work by Alvanos and
Poulakis, we give a complete decision algorithm, which allows us to prove
finiteness results concerning these particular solutions. Finally, some
extensive computations are presented regarding two particular cases: the
generalized Markoff equation x^2+y^2+z^2 = dxyz over quadratic fields and the
classic Markoff equation x^2+y^2+z^2 = 3xyz over an arbitrary number field.Comment: To appear in Journal of Symbolic Computatio
Pion production within the hybrid relativistic plane wave impulse approximation model at MiniBooNE and MINERvA kinematics
The hybrid model for electroweak single-pion production (SPP) off the
nucleon, presented in [Gonz\'alez-Jim\'enez et al., Phys. Rev. D 95, 113007
(2017)], is extended here to the case of incoherent pion-production on the
nucleus. Combining a low-energy model with a Regge approach, this model
provides valid predictions in the entire energy region of interest for current
and future accelerator-based neutrino-oscillation experiments. The Relativistic
Mean-Field model is used for the description of the bound nucleons while the
outgoing hadrons are considered as plane waves. This approach, known as
Relativistic Plane-Wave Impulse Approximation (RPWIA), is a first step towards
the development of more sophisticated models, it is also a test of our current
understanding of the elementary reaction. We focus on the charged-current
()-nucleus interaction at MiniBooNE and MINERvA kinematics. The
effect on the cross sections of the final-state interactions, which affect the
outgoing hadrons on their way out of the nucleus, is judged by comparing our
results with those from the NuWro Monte Carlo event generator. We find that the
hybrid-RPWIA predictions largely underestimate the MiniBooNE data. In the case
of MINERvA, our results fall below the -induced 1 production data,
while a better agreement is found for -induced 1 and
-induced 1 production.Comment: 13 pages, 10 figure
Rotochemical heating with a density-dependent superfluid energy gap in neutron stars
When a rotating neutron star loses angular momentum, the reduction of the
centrifugal force makes it contract. This perturbs each fluid element, raising
the local pressure and originating deviations from beta equilibrium, inducing
reactions that release heat (rotochemical heating). This effect has previously
been studied by Fern\'andez and Reisenegger for neutron stars of non-superfluid
matter and by Petrovich and Reisenegger for superfluid matter, finding that the
system in both cases reaches a quasi-steady state, corresponding to a partial
equilibration between compression, due to the loss of angular momentum, and
reactions that try to restore the equilibrium. However, Petrovich and
Reisenegger assumes a constant value of the superfluid energy gap, whereas
theoretical models predict density-dependent gap amplitudes, and therefore gaps
that depend on the location in the star. In this work, we try to discriminate
between several proposed gap models, comparing predicted surface temperatures
to the value measured for the nearest millisecond pulsar, J0437-4715.Comment: 2 pages, 1 figure. VIII Symposium in Nuclear Physics and
Applications: Nuclear and Particle Astrophysics. Appearing in the American
Institute of Physics (AIP) conference proceedings
Parity violation in quasielastic electron-nucleus scattering within the relativistic impulse approximation
We study parity violation in quasielastic (QE) electron-nucleus scattering
using the relativistic impulse approximation. Different fully relativistic
approaches have been considered to estimate the effects associated with the
final-state interactions. We have computed the parity-violating quasielastic
(PVQE) asymmetry and have analyzed its sensitivity to the different ingredients
that enter in the description of the reaction mechanism: final-state
interactions, nucleon off-shellness effects, current gauge ambiguities.
Particular attention has been paid to the description of the weak neutral
current form factors. The PVQE asymmetry is proven to be an excellent
observable when the goal is to get precise information on the axial-vector
sector of the weak neutral current. Specifically, from measurements of the
asymmetry at backward scattering angles good knowledge of the radiative
corrections entering in the isovector axial-vector sector can be gained.
Finally, scaling properties shown by the interference nuclear
responses are also analyzed.Comment: 15 pages, 11 figure
- …