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This proceeding presents recent results from a joint analysis of time-dependent neutrino and electromagnetic emissions from tidal disruption events (TDEs), using both isotropic wind models and relativistic jets. We discuss constraints from…

High Energy Astrophysical Phenomena · Physics 2025-08-12 Chengchao Yuan , Walter Winter , Cecilia Lunardini , B. Theodore Zhang , Kohta Murase , Bing Zhang

Tidal disruption events (TDE) have been considered as cosmic-ray and neutrino sources for a decade. We suggest two classes of new scenarios for high-energy multi-messenger emission from TDEs that do not have to harbor powerful jets. First,…

High Energy Astrophysical Phenomena · Physics 2020-10-19 Kohta Murase , Shigeo S. Kimura , B. Theodore Zhang , Foteini Oikonomou , Maria Petropoulou

We revisit the Ultra-High-Energy Cosmic Ray (UHECRs) production in Tidal Disruption Events (TDEs) in the light of recent neutrino-TDE associations. We use an isotropically emitting source-propagation model, which has been developed to…

High Energy Astrophysical Phenomena · Physics 2025-07-15 Pavlo Plotko , Walter Winter , Cecilia Lunardini , Chengchao Yuan

Tidal Disruption Events (TDEs) are processes where stars are torn apart by the strong gravitational force near to a massive or supermassive black hole. If a jet is launched in such a process, particle acceleration may take place in internal…

High Energy Astrophysical Phenomena · Physics 2019-07-15 Daniel Biehl , Denise Boncioli , Cecilia Lunardini , Walter Winter

Recently, a high-energy muon neutrino event was detected in association with a tidal disruption event (TDE) AT2019dsg at the time about 150 days after the peak of the optical/UV luminosity. We propose that such a association could be…

High Energy Astrophysical Phenomena · Physics 2020-11-18 Ruo-Yu Liu , Shao-Qiang Xi , Xiang-Yu Wang

Tidal Disruption Events (TDEs) occur when stars pass close to supermassive black holes, and have long been predicted to emit cosmic rays and neutrinos. Recently the TDE AT2109dsg was identified in spatial and temporal coincidence with…

High Energy Astrophysical Phenomena · Physics 2021-10-06 Robert Stein

A neutrino-like event with an energy of $\sim 220 \,{\rm PeV}$ was recently detected by the KM3NeT/ARCA telescope. If this neutrino comes from an astrophysical source, or from the interaction of an ultra-high-energy cosmic ray in the…

High Energy Astrophysical Phenomena · Physics 2025-03-19 Ke Fang , Francis Halzen , Dan Hooper

Recent observations of isotropic diffuse backgrounds by Fermi and IceCube allow us to get more insight into distant very-high-energy (VHE) and ultra-high-energy (UHE) gamma-ray/neutrino emitters, including cosmic-ray accelerators/sources.…

High Energy Astrophysical Phenomena · Physics 2012-08-29 Kohta Murase , John F. Beacom , Hajime Takami

Tidal disruption events (TDEs), in which stars are disrupted by supermassive black holes, have been proposed as potential sources of high-energy neutrinos through hadronic interactions. X-ray-bright TDEs provide dense photon fields…

High Energy Astrophysical Phenomena · Physics 2026-02-25 Rong-Lan Li , Chengchao Yuan , Hao-Ning He , Yun Wang , Ben-Yang Zhu , Yun-Feng Liang , Ning Jiang , Da-Ming Wei

Extremely high energy (up to 10**(22) eV) cosmic neutrino beams initiate high energy particle cascades in the background of relic neutrinos from the Big Bang. We perform numerical calculations to show that such cascades could contribute…

High Energy Physics - Phenomenology · Physics 2009-10-31 Shigeru Yoshida , Guenter Sigl , Sangjin Lee

The observation of a neutrino at IceCube in association with the Tidal Disruption Event (TDE) AT2019dsg has suggested TDEs as a new class of sources of astrophysical neutrinos. We present a model of this multi-messenger observation in a…

High Energy Astrophysical Phenomena · Physics 2021-08-02 Walter Winter , Cecilia Lunardini

Tidal disruption events (TDEs) have been proposed as candidate sources of high-energy neutrinos. Successful and choked jets, as well as the accretion disk, corona, wind, and outflow regions in a TDE have been examined and shown to produce…

High Energy Astrophysical Phenomena · Physics 2026-01-30 Mainak Mukhopadhyay , Patrick Wusinich , Kohta Murase

We report on a search for electromagnetic and/or hadronic showers (cascades) induced by a diffuse flux of neutrinos with energies between 5 TeV and 300 TeV from extraterrestrial sources. Cascades may be produced by matter interactions of…

Astrophysics · Physics 2011-08-31 J. Ahrens

Tidal disruptions are extremely powerful phenomena that have been designated as candidate sources of ultra-high-energy cosmic rays. The disruption of a star by a black hole can naturally provide protons and heavier nuclei, which can be…

High Energy Astrophysical Phenomena · Physics 2022-02-09 Claire Guépin , Kumiko Kotera , Enrico Barausse , Ke Fang , Kohta Murase

We introduce neutrino astronomy starting from the observational fact that Nature accelerates protons and photons to energies in excess of 10^{20} and 10^{13} eV, respectively. Although the discovery of cosmic rays dates back a century, we…

Astrophysics · Physics 2007-05-23 F. Halzen

Three Tidal Disruption Event (TDE) candidates (AT2019dsg, AT2019fdr, AT2019aalc) have been associated with high energy astrophysical neutrinos in multi-messenger follow-ups. In all cases, the neutrino observation occurred O(100) days after…

High Energy Astrophysical Phenomena · Physics 2023-05-08 Walter Winter , Cecilia Lunardini

High-energy neutrinos, arising from decays of mesons that were produced through the cosmic rays collisions with air nuclei, form unavoidable background noise in the astrophysical neutrino detection problem. The atmospheric neutrino flux…

High Energy Astrophysical Phenomena · Physics 2010-10-13 S. I. Sinegovsky , A. A. Kochanov , T. S. Sinegovskaya

Ultra-high energy cosmic rays interacting with the radiation fields in the universe cause electromagnetic cascades resulting in a flux of extragalactic gamma rays, detectable to some 100 GeV. Recent precise measurements of the extragalactic…

High Energy Astrophysical Phenomena · Physics 2015-06-19 A. D. Erlykin , A. W. Wolfendale
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