del Aguila , F.; Ametller, L.; Illana, J.I.; Santiago, J.; Talavera, P.; Vega-Morales, R. Journal of high energy physics Vol. 08, num. 028, p. 1-26 DOI: 10.1007/JHEP08(2017)028 Data de publicació: 2017-08-08 Article en revista
We calculate loop induced lepton flavor violating Higgs decays in the Littlest
Higgs model with T-parity. We find that a finite amplitude is obtained only when all
contributions from the T-odd lepton sector are included. This is in contrast to lepton fla-
vor violating processes mediated by gauge bosons where the partners of the right-handed
mirror leptons can be decoupled from the spectrum. These partners are necessary to can-
cel the divergence in the Higgs mass introduced by the mirror leptons but are otherwise
unnecessary and assumed to be decoupled in previous phenomenological studies. Further-
more, as we emphasize, including the partner leptons in the spectrum also introduces a
new source of lepton flavor violation via their couplings to the physical pseudo-Goldstone
electroweak triplet scalar. Although this extra source also affects lepton flavor changing
gauge transitions, it decouples from these amplitudes in the limit of heavy mass for the
partner leptons. We find that the corresponding Higgs branching ratio into taus and muons
can be as large as ~ 0.2 × 10 -6 for T-odd masses of the order a few TeV, a demanding
challenge even for the high luminosity LHC.
Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid, M.; Aubert, J.; Avgitas, T.; Baret, B.; Barrios, J.; Basa, S. Journal of high energy physics Vol. 2017, p. 1-19 DOI: 10.1007/JHEP07(2017)054 Data de publicació: 2017-07-01 Article en revista
A search for magnetic monopoles using five years of data recorded with the ANTARES neutrino telescope from January 2008 to December 2012 with a total live time of 1121 days is presented. The analysis is carried out in the range ß > 0.6 of magnetic monopole velocities using a strategy based on run-by-run Monte Carlo simulations. No signal above the background expectation from atmospheric muons and atmospheric neutrinos is observed, and upper limits are set on the magnetic monopole flux ranging from 5.7 × 10-16 to 1.5 × 10-18 cm-2·s-1·sr-1.[Figure not available: see fulltext.].
Studying atmospheric neutrino oscillations in the few-GeV range with a multi-megaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the Mediterranean Sea. In this paper, the processes that limit the obtainable resolution in both energy and direction in charged-current neutrino events in the ORCA detector are investigated. These processes include the composition of the hadronic fragmentation products, the subsequent particle propagation and the photon-sampling fraction of the detector. GEANT simulations of neutrino interactions in seawater produced by GENIE are used to study the effects in the 1-20 GeV range. It is found that fluctuations in the hadronic cascade in conjunction with the variation of the inelasticity y are most detrimental to the resolutions. The effect of limited photon sampling in the detector is of significantly less importance. These results will therefore also be applicable to similar detectors/media, such as those in ice.
The Souriau massless Galilean particle of “colour” k and spin s is shown to be the Galilean limit of the Souriau tachyon of mass m = ik and spin s. We compare and contrast this result with the Galilean limit of the Nambu-Goto string and Green-Schwarz superstring.
We consider two non-relativistic strings and their Galilean symmetries. These strings are obtained as the two possible non-relativistic (NR) limits of a relativistic string. One of them is non-vibrating and represents a continuum of non-relativistic massless particles, and the other one is a non-relativistic vibrating string. For both cases we write the generator of the most general point transformation and impose the condition of Noether symmetry. As a result we obtain two sets of non-relativistic Killing equations for the vector fields that generate the symmetry transformations. Solving these equations shows that NR strings exhibit two extended, infinite dimensional space-time symmetries which contain, as a subset, the Galilean symmetries. For each case, we compute the associated conserved charges and discuss the existence of non-central extensions.