Articles Citing

Super heavy dark matter origin of the PeV neutrino event: KM3-230213A

Kazunori Kohri ^1,2,3,*, Partha Kumar Paul ^4,†, and Narendra Sahu ^4,‡

¹Division of Science, National Astronomical Observatory of Japan (NAOJ), and SOKENDAI, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
²Theory Center, IPNS, and QUP (WPI), KEK, 1-1 Oho, Tsukuba, Ibaraki 305-0801, Japan
³Kavli IPMU (WPI), UTIAS, The University of Tokyo, Kashiwa, Chiba 277-8583, Japan
⁴Department of Physics, Indian Institute of Technology Hyderabad, Kandi, Sangareddy, Telangana-502285, India

^*Contact author: kazunori.kohri@gmail.com
^†Contact author: ph22resch11012@iith.ac.in
^‡Contact author: nsahu@phy.iith.ac.in

Dark matter

Marco Cirelli, Alessandro Strumia, and Jure Zupan

SciPost Phys. Rev. 1 (2026)

Could a Primordial Black Hole Explosion Explain the Extremely High-Energy KM3NeT Neutrino Event?

Lua F. T. Airoldi, Gustavo F. S. Alves, Yuber F. Perez-Gonzalez, Gabriel M. Salla, and Renata Zukanovich Funchal

Phys. Rev. Lett. 136 041002 (2026)

Tackling transient sources with neutrino telescopes

Lua F. T. Airoldi, Gustavo F. S. Alves, Yuber F. Perez-Gonzalez, Gabriel M. Salla, and Renata Zukanovich Funchal

Phys. Rev. D 113 023052 (2026)

Implications of the KM3NeT ultrahigh-energy event on neutrino self-interactions

Yuxuan He, Jia Liu, Xiao-Ping Wang, and Yi-Ming Zhong

Phys. Rev. D 113 043022 (2026)

Constraining superheavy dark matter with the KM3-230213A neutrino event

Roberto Aloisio, Antonio Ambrosone, and Carmelo Evoli

Phys. Rev. D 113 043024 (2026)

Neutrino transition dipole moments in light of the KM3NeT event

Alejandro Muñoz-Ovalle and Stefan Vogl

Phys. Rev. D 113 055004 (2026)

Neutron portal to ultrahigh-energy neutrinos

Gustavo F. S. Alves, Matheus Hostert, and Maxim Pospelov

Phys. Rev. D 113 075035 (2026)

KM3-230213A and IceCube neutrino events from metastable dark matter of primordial black hole origin

Prabhav Singh, Mansi Dhuria, and Nathanael Varghese Job

Phys. Rev. D 113 103014 (2026)

Highest-energy neutrino event constrains dark matter-neutrino interactions

Toni Bertólez-Martínez, Gonzalo Herrera, Pablo Martínez-Miravé, and Jorge Terol Calvo

Phys. Rev. D 113 103052 (2026)

Exploring ultra-high energy neutrino experiments through the lens of the transport equation

Stefano Palmisano, Diego Redigolo, Michele Tammaro, and Andrea Tesi

J. High Energ. Phys. 2026 223 (2026)

Superluminal constraints from ultra-high-energy neutrino events

J.M. Carmona, J.L. Cortés, and M.A. Reyes

J. Cosmol. Astropart. Phys. 2026 023 (2026)

Explaining the KM3-230213A detection without gamma-ray emission: cosmic-ray dark radiation

Yuma Narita and Wen Yin

J. Cosmol. Astropart. Phys. 2026 030 (2026)

Decaying vector dark matter with low reheating temperature for KM3NeT signal and its impact on gravitational waves

Sarif Khan, Jongkuk Kim, and Hyun Min Lee

J. Cosmol. Astropart. Phys. 2026 083 (2026)

Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from a Cosmic-Ray Transient

Sovan Boxi, Saikat Das, and Nayantara Gupta

ApJL 997 L3 (2026)

Implications of a Cosmogenic Origin of KM3-230213A for Ultra-high-energy Protons

Abdulrahman Alhebsi, Arjen van Vliet, Domenik Ehlert, and Satyendra Thoudam

ApJ 1003 235 (2026)

What KM3-230213A event may tell us about the neutrino mass and dark matter

Basabendu Barman, Arindam Das, and Prantik Sarmah

Phys. Rev. D 112 075014 (2025)

Ultrahigh-energy neutrino event KM3-230213A as a signal of electroweak vacuum turbulence in merging black hole binaries

Alexander S. Sakharov, Rostislav Konoplich, and Merab Gogberashvili

Phys. Rev. D 112 083061 (2025)

Superheavy supersymmetric dark matter as the origin of the KM3NeT ultrahigh energy signal

Yongsoo Jho, Seong Chan Park, and Chang Sub Shin

Phys. Rev. D 112 115004 (2025)

Astrophysical flux of dark particles as a solution to the KM3NeT and IceCube tension over KM3-230213A

Yasaman Farzan and Matheus Hostert

J. High Energ. Phys. 2025 208 (2025)

Looking for the gamma-Ray cascades of the KM3-230213A neutrino source

Milena Crnogorčević, Carlos Blanco, and Tim Linden

J. Cosmol. Astropart. Phys. 2025 009 (2025)

Linking the KM3-230213A neutrino event to dark matter decay and gravitational wave signals

Sarif Khan, Jongkuk Kim, and Pyungwon Ko

J. Cosmol. Astropart. Phys. 2025 033 (2025)

A possible cosmological origin of the KM3-230213A event

Ki-Young Choi, Erdenebulgan Lkhagvadorj, and Satyabrata Mahapatra

J. Cosmol. Astropart. Phys. 2025 079 (2025)

Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events

Kohta Murase, Yuma Narita, and Wen Yin

J. Cosmol. Astropart. Phys. 2025 109 (2025)

Cosmic-Ray Constraints on the Flux of Ultrahigh-energy Neutrino Event KM3-230213A

Saikat Das, Bing Zhang, Soebur Razzaque, and Siyao Xu

ApJ 991 96 (2025)

Select page:

Physical Review D

Filter

Articles Citing

Super heavy dark matter origin of the PeV neutrino event: KM3-230213A

Dark matter

Could a Primordial Black Hole Explosion Explain the Extremely High-Energy KM3NeT Neutrino Event?

Tackling transient sources with neutrino telescopes

Implications of the KM3NeT ultrahigh-energy event on neutrino self-interactions

Constraining superheavy dark matter with the KM3-230213A neutrino event

Neutrino transition dipole moments in light of the KM3NeT event

Neutron portal to ultrahigh-energy neutrinos

KM3-230213A and IceCube neutrino events from metastable dark matter of primordial black hole origin

Highest-energy neutrino event constrains dark matter-neutrino interactions

Exploring ultra-high energy neutrino experiments through the lens of the transport equation

Superluminal constraints from ultra-high-energy neutrino events

Explaining the KM3-230213A detection without gamma-ray emission: cosmic-ray dark radiation

Decaying vector dark matter with low reheating temperature for KM3NeT signal and its impact on gravitational waves

Cosmogenic Origin of KM3-230213A: Delayed Gamma-Ray Emission from a Cosmic-Ray Transient

Implications of a Cosmogenic Origin of KM3-230213A for Ultra-high-energy Protons

What KM3-230213A event may tell us about the neutrino mass and dark matter

Ultrahigh-energy neutrino event KM3-230213A as a signal of electroweak vacuum turbulence in merging black hole binaries

Superheavy supersymmetric dark matter as the origin of the KM3NeT ultrahigh energy signal

Astrophysical flux of dark particles as a solution to the KM3NeT and IceCube tension over KM3-230213A

Looking for the gamma-Ray cascades of the KM3-230213A neutrino source

Linking the KM3-230213A neutrino event to dark matter decay and gravitational wave signals

A possible cosmological origin of the KM3-230213A event

Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events

Cosmic-Ray Constraints on the Flux of Ultrahigh-energy Neutrino Event KM3-230213A

Filter

Filter

Article Lookup

Enter a citation