Search results for "NEUTRINOS"
showing 10 items of 206 documents
Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and Ic…
2019
[EN] Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the out¿ow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCub…
Radiative neutrino masses: A window to new physics
2021
Currently, the Standard Model of particle physics (SM) is the best theory we have to describe particles and their interactions. However, there is evidence of physics beyond it, which motivates us to seek for a more complete theory. Neutrino oscillations constitute the first experimental confirmation of new physics, as they require a new piece that is absent in the SM, non-zero neutrino masses. Neutrino masses brought new theoretical challenges, for instance questions as how these masses are generated or why are they so small compared to other masses, are still under investigation. In this thesis, we aim to study radiative neutrino mass models, a class of models where small neutrino masses a…
Probing neutrino magnetic moments at the Spallation Neutron Source facility
2015
24 pages.- 8 figures
LHC dijet constraints on double beta decay
2015
13 pages.- 5 figures
Theory and phenomenology of Dirac neutrinos: Symmetry breaking patterns, flavour implications and Dark Matter
2021
El Modelo Estándar (SM en ingles) de interacciones Electro-Débiles (EW en inglés) ha sido un gran éxito desde un punto de vista teórico y experimental. Si bien este éxito no se puede negar, es hora de avanzar y abordar las preguntas que el SM deja sin respuesta, como las masas de neutrinos, la naturaleza de la materia oscura, el problema de la jerarquía o el problema de violación de CP en el sector de las interacciones fuertes, entre otros. De hecho, el SM predice neutrinos sin masa. Sin embargo, los experimentos de oscilación de neutrinos, que ahora alcanzan la era de la precisión, muestran claramente que al menos dos neutrinos son masivos y arrojan luz sobre su patrón de mezcla. Sin embar…
Updated determination of the solar neutrino fluxes from solar neutrino data
2016
Journal of High Energy Physics 2016.3 (2016): 132 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Three-neutrino mixing after the first results from K2K and KamLAND
2003
We analyze the impact of the data on long baseline \nu_\mu disappearance from the K2K experiment and reactor \bar\nu_e disappearance from the KamLAND experiment on the determination of the leptonic three-generation mixing parameters. Performing an up-to-date global analysis of solar, atmospheric, reactor and long baseline neutrino data in the context of three-neutrino oscillations, we determine the presently allowed ranges of masses and mixing and we consistently derive the allowed magnitude of the elements of the leptonic mixing matrix. We also quantify the maximum allowed contribution of \Delta m^2_{21} oscillations to CP-odd and CP-even observables at future long baseline experiments.
Composite scalars and dark matter from four-fermion interactions
2022
Parte I: Emergencia de masas en el Modelo Estándar El bosón de Higgs es un campo escalar del Modelo Estándar (SM, por sus siglas en inglés) de partı́culas elementales que cumple dos funciones muy importantes. Por un lado permite construir una teorı́a renormalizable. El potencial escalar contiene un término de masa y un término cuadrático en el campo de Higgs, los cuales son ajus- tados en base a mediciones experimentales y haciéndolos compatible con la aparición de una ruptura espontánea de la simetrı́a SU (2) L × U (1) Y del SM. Y por otra parte ayuda a explicar la masa de todos los fermiones en el esquema de la teorı́a cuántica de campos, al poseer interacciones de tipo Yukawa que son aju…
A fast algorithm for muon track reconstruction and its application to the ANTARES neutrino telescope.
2011
An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained …
The next-generation liquid-scintillator neutrino observatory LENA
2012
We propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a next-generation neutrino observatory on the scale of 50 kt. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. LENA's physics objectives comprise the observation of astrophysical and terrestrial neutrino sources as well as the investigation of neutrino oscillations. In the GeV energy range, the search for proton decay and long-baseline neutrino oscillation experiments complement the low-energy program. Based on the considerable expertise present in European and international research groups, the …