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Sterile neutrinos can be produced in the early universe via interactions with their active counterparts. For small active-sterile mixing angles, thermal equilibrium with the standard model plasma is not reached and sterile neutrinos are…

High Energy Physics - Phenomenology · Physics 2022-07-06 Gonzalo Alonso-Álvarez , James M. Cline

We provide a consistent framework to set limits on properties of light sterile neutrinos coupled to all three active neutrinos using a combination of the latest cosmological data and terrestrial measurements from oscillations, $\beta$-decay…

The IceCube Neutrino Observatory recently published evidence for diffuse neutrino emission from the Galactic Plane at $4.5\sigma$ significance. This new source of astrophysical neutrinos provides an exciting laboratory for probing the…

High Energy Physics - Phenomenology · Physics 2025-07-08 Miller MacDonald , Kiara Carloni , Carlos A. Argüelles , Rafael Alves Batista , Ivan Martínez-Soler

Any interpretation of the astrophysical neutrinos discovered by IceCube must accommodate a variety of multimessenger constraints. We address implications of these neutrinos being produced in transient sources, principally if buried within…

High Energy Astrophysical Phenomena · Physics 2017-04-04 Matthew D. Kistler , Hasan Yuksel

In this paper we note that for neutrino mass squared differences in the range $10^{-4} - 10^{-1} eV^2$, vacuum neutrino oscillations can take place between the neutrino-sphere and the weak freeze-out radius in a type II supernova. Requiring…

High Energy Physics - Phenomenology · Physics 2007-05-23 Sandhya Choubey , Srubabati Goswami

In the minimal standard model it is possible to gauge any one of the following global symmetries in an anomaly free way: (i)$L_{e}-L_{\mu}$, (ii) $L_{e}-L_{\tau}$ or (iii) $L_{\mu}-L_{\tau}$. If the gauge boson corresponding to (i) or (ii)…

High Energy Physics - Phenomenology · Physics 2009-11-10 Anjan S. Joshipura , Subhendra Mohanty

Mixed dark matter models with one low-mass (e.g. 2.4eV) neutrino flavor are shown to be in good agreement with observations if the neutrinos have non-zero chemical potentials. This agreement holds (except for the problem with a low-age…

Astrophysics · Physics 2010-01-15 Georg B. Larsen , Jes Madsen

Thermal MeV neutrino emission from core-collapse supernovae offers a unique opportunity to probe physics beyond the Standard Model in the neutrino sector. The next generation of neutrino experiments, such as DUNE and Hyper-Kamiokande, can…

High Energy Physics - Phenomenology · Physics 2023-04-20 Jose Alonso Carpio , Ali Kheirandish , Kohta Murase

Long gamma-ray bursts have been widely associated with collapsing massive stars in the framework of collapsar model. High-energy neutrinos and photons can be produced in the internal shocks of middle relativistic jets from core-collapse…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Nissim Fraija

Neutrino oscillations are a widely observed and well established phenomenon. It is also well known that deviations with respect to flavor conversion probabilities in vacuum arise due to neutrino interactions with matter. In this work, we…

High Energy Astrophysical Phenomena · Physics 2016-12-06 P. F. de Salas , R. A. Lineros , M. Tórtola

The IceCube South Pole Neutrino Observatory is a Cherenkov detector instrumented in a cubic kilometer of ice at the South Pole. IceCube's primary scientific goal is the detection of TeV neutrino emissions from astrophysical sources. At the…

High Energy Physics - Experiment · Physics 2023-08-01 Shiqi Yu , Jessie Micallef

In the standard model neutrinos are assumed to have streamed across the Universe since they last scattered at the weak decoupling epoch when the temperature of the standard-model plasma was ~MeV. The shear stress of free-streaming neutrinos…

Cosmology and Nongalactic Astrophysics · Physics 2015-01-07 Francis-Yan Cyr-Racine , Kris Sigurdson

We examine scenarios in which a dark sector (dark matter, dark radiation, or dark energy) couples to the active neutrinos. For light and weakly-coupled exotic sectors we find that scalar, vector, or tensor dark backgrounds may appreciably…

High Energy Physics - Phenomenology · Physics 2018-07-18 Francesco Capozzi , Ian M. Shoemaker , Luca Vecchi

If there is a hidden photon -- i.e. a light abelian gauge boson in the hidden sector -- its kinetic mixing with the standard photon can produce a hidden cosmic microwave background (hCMB). For meV masses, resonant photon-hidden photon…

Astrophysics · Physics 2009-06-23 Joerg Jaeckel , Javier Redondo , Andreas Ringwald

The recent study on the the 6-year up-going muon neutrinos by the IceCube Collaboration support the hypothesis of a two-component scenario explaining the diffuse TeV-PeV neutrino flux. Once a hard astrophysical power-law is considered, an…

High Energy Physics - Phenomenology · Physics 2018-11-14 Marco Chianese

We discuss the possibility to explain the anomalies in short-baseline neutrino oscillation experiments in terms of sterile neutrinos. We work in a 3+1 framework and pay special attention to recent new data from reactor experiments, IceCube…

Data from several neutrino experiments suggest an anomalous neutrino flavor transition across relatively short baselines which is in conflict with the three-flavor neutrino oscillation paradigm. In particular, MiniBooNE and BEST…

High Energy Physics - Phenomenology · Physics 2023-05-16 Vedran Brdar

Although the MiniBooNE experiment has severely restricted the possible existence of light sterile neutrinos, a few anomalies persist in oscillation data, and the possibility of extra light species contributing as a subdominant hot (or warm)…

Astrophysics · Physics 2010-04-23 Mario A. Acero , Julien Lesgourgues

The IceCube Neutrino Observatory instruments roughly one cubic kilometer of deep, glacial ice below the geographic South Pole with 5160 optical sensors to register the Cherenkov light of passing relativistic, charged particles. Since its…

Instrumentation and Methods for Astrophysics · Physics 2019-11-26 Martin Rongen

Measurements of flavor ratios of astrophysical neutrino fluxes are sensitive to the two yet unknown mixing parameters $\theta_{13}$ and $\delta$ through the combination $\sin\theta_{13}\cos\delta$. We extend previous studies by considering…

High Energy Physics - Phenomenology · Physics 2007-07-03 Kfir Blum , Yosef Nir , Eli Waxman