Results 21 to 30 of about 18,709 (253)
Higher Flavor Symmetries in the Standard Model
The Standard Model enjoys a higher‐group symmetry which mixes the zero‐form flavor symmetries with the one‐form magnetic hyper charge symmetry. This structure greatly restricts the possible flavor symmetries that may remain unbroken in any ultraviolet completion that includes magnetic monopoles.
Clay Córdova, Seth Koren
wiley +1 more source
The Low‐Scale Seesaw Solution to the MW$M_W$ and (g−2)μ$(g-2)_\umu$ Anomalies
Abstract The recent CDF‐II measurement of the W‐boson mass shows a strong tension with the corresponding Standard Model prediction. Once active neutrino masses are explained in the context of the Low‐Scale Seesaw mechanisms, this tension can be resolved.
Arturo de Giorgi +2 more
wiley +1 more source
Probing HNL‐ALP Couplings at Colliders
Abstract Axion‐like particles (ALPs) and heavy neutral leptons (HNLs) are both well‐motivated extensions of the Standard Model. As ALPs couple to on‐shell fermions proportionally to their masses, processes involving both types of particles may give rise, for TeV HNLs, to relevant phenomenology at colliders.
Arturo de Giorgi +2 more
wiley +1 more source
Who's Afraid of the Supersymmetric Dark? The Standard Model vs Low‐Energy Supergravity
Abstract Use of supergravity equations in astronomy and late‐universe cosmology is often criticized on three grounds: (i) phenomenological success usually depends on the supergravity form for the scalar potential applying at the relevant energies; (ii$ii$) the low‐energy scalar potential is extremely sensitive to quantum effects involving very massive ...
C.P. Burgess, F. Quevedo
wiley +1 more source
Axion–Sterile Neutrino Dark Matter [PDF]
Extending the standard model with three right-handed neutrinos and a simple QCD axion sector can account for neutrino oscillations, dark matter and baryon asymmetry; at the same time, it solves the strong CP problem, stabilizes the electroweak vacuum and can implement critical Higgs inflation (satisfying all current observational bounds).
Salvio A., Scollo S.
openaire +4 more sources
A novel solution for controlling hardware components of accelerators and beamlines
A novel approach to the remote‐control system for the compact multi‐crystal energy‐dispersive spectrometer for X‐ray emission spectroscopy applications is described.A novel approach to the remote‐control system for the compact multi‐crystal energy‐dispersive spectrometer for X‐ray emission spectroscopy (XES) applications has been developed.
Igor Khokhriakov +4 more
wiley +1 more source
Neutrinoastronomie in der Antarktis
Vor zehn Jahren ging in der Antarktis das Neutrinoteleskop IceCube in Betrieb. Bis heute wurden damit über hundert Neutrinos von kosmischen „Beschleunigern” nachgewiesen. In einem Fall ließ sich eine aktive Galaxie als mögliche Quelle identifizieren. Zusammenfassung Fast hundert Jahre nach der Vorhersage von Neutrinos sind wir heute in der Lage, diese ...
Markus Ackermann
wiley +1 more source
Atomic ionization by sterile-to-active neutrino conversion and constraints on dark matter sterile neutrinos with germanium detectors [PDF]
The transition magnetic moment of a sterile-to-active neutrino conversion gives rise to not only radiative decay of a sterile neutrino, but also its non-standard interaction (NSI) with matter.
Chen, Jiunn-Wei +7 more
core +2 more sources
Sterile neutrino as a bulk neutrino [PDF]
If light sterile neutrinos are needed to understand the neutrino puzzles, as is currently indicated, a major theoretical challenge is to understand why its mass is so small. It is a more serious problem than understanding the small mass of the familiar neutrinos.
Mohapatra, R. N., Perez-Lorenzana, A.
openaire +2 more sources
Can Neutrino Self-interactions Save Sterile Neutrino Dark Matter?
Sterile neutrinos only interact with the standard model through the neutrino sector, and thus represent a simple dark matter (DM) candidate with many potential astrophysical and cosmological signatures.
Rui An +3 more
doaj +1 more source

