Neutrinos from the Galactic Center Hosting a Hypernova Remnant

He, Hao-Ning; Lee, Shiu-Hang; Nagataki, Shigehiro; Kusenko, Alexander

doi:10.3847/1538-4357/ab7749

Title: Neutrinos from the Galactic Center Hosting a Hypernova Remnant

Journal Article · Wed Mar 18 00:00:00 EDT 2020 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/ab7749· OSTI ID:1801945

^[1]; Lee, Shiu-Hang ^[2];

^[3]; Kusenko, Alexander ^[4]

Inst. of Physical and Chemical Research (RIKEN), Wako (Japan); Chinese Academy of Sciences (CAS), Nanjing (China)
Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI); Kyoto Univ. (Japan)
RIKEN, Saitama (Japan)
Univ. of California, Los Angeles, CA (United States); Univ. of Tokyo (Japan)

Similar to star-forming galaxies or starburst galaxies, star-forming regions in our Galaxy can host cosmic-ray (CR) accelerators and rich gas as targets of hadronuclear interaction. By our estimations, the IceCube neutrino observatory might detect muon neutrinos from a CR accelerator associated with a molecular cloud complex in our Galaxy. The associated high-energy gamma-ray emission might be observed by the Cherenkov Telescope Array (CTA), High-Altitude Water Cherenkov Gamma-Ray Observatory (HAWC), and Large High Altitude Air Shower Observatory (LHAASO). Furthermore, taking the Galactic Center (GC) region as an example, we assume that a hypernova exploded in the past in the GC. We simulate the acceleration of CRs in the hypernova remnant (HNR) as well as their confinement and escape. The high-energy protons escape from the HNR, diffuse around the GC, interact with molecular clouds, and then produce gamma-rays and neutrinos. In the optimal cases, the GC would be a promising 100 TeV gamma-ray source for LHAASO’s one-month observation. We propose that neutrino-induced searching for starting track-like and high-energy starting events (HESEs) observed by IceCube, from the GC region with a radius of 1°.8, would help us discover the particle accelerator in the GC or constrain our models. Under the constraint from high-energy gamma-ray observations by the H.E.S.S. telescope, we estimate the exposure time needed to make a significant discovery for the optimal cases. The analysis combining observations of IceCube and ANTARES, starting track-like events and HESEs, future observations by neutrino detectors IceCube-Gen2 and KM3net, and gamma-ray telescopes CTA, HAWC, and LHAASO would help to constrain our models.

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Research Organization:: Univ. of California, Los Angeles, CA (United States)

Sponsoring Organization:: USDOE Office of Science (SC)

Grant/Contract Number:: SC0009937

OSTI ID:: 1801945

Journal Information:: The Astrophysical Journal (Online), Vol. 891, Issue 2; ISSN 1538-4357

Publisher:: IOP PublishingCopyright Statement

Country of Publication:: United States

Language:: English

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