scholarly journals High-energy Neutrinos and Gamma Rays from Nonrelativistic Shock-powered Transients

2020 ◽  
Vol 904 (1) ◽  
pp. 4
Author(s):  
Ke Fang ◽  
Brian D. Metzger ◽  
Indrek Vurm ◽  
Elias Aydi ◽  
Laura Chomiuk
2019 ◽  
Author(s):  
Paola Alvarez Hurtado ◽  
Nissim Fraija ◽  
Antonio Galván ◽  
Antonio Marinelli

2005 ◽  
Vol 22 (2) ◽  
pp. 157-161 ◽  
Author(s):  
Qinghuan Luo

AbstractPulsars may be born with a short rotation period of milliseconds with the magnetic field amplified through dynamo processes up to ∼1015–1016 G. Such millisecond magnetars spin down rapidly, emitting bursts of high-energy neutrinos and gamma rays. Specifically, acceleration of ions in both the polar gap (as in a normal pulsar) and the relativistic magnetar wind is considered. In both cases ions can be accelerated to ultra-high energies and these energetic ions can lead to production of high-energy neutrinos and gamma rays through interaction with thermal radiation from the hot neutron star or the heated inner boundary region of the stellar envelope as the result of the deposition of energy by the magnetar wind. The detectability of the neutrino flux by a kilometre-scale neutrino detector such as the planned IceCube neutrino observatory is discussed.


2019 ◽  
Author(s):  
Fabian Schüssler ◽  
H. Ashkar ◽  
M. Backes ◽  
Kathrin Egberts ◽  
F. Brun ◽  
...  

2021 ◽  
Author(s):  
Susumu Inoue ◽  
Matteo Cerruti ◽  
Kohta Murase ◽  
Ruo-Yu Liu

1964 ◽  
Vol 83 (5) ◽  
pp. 3-34 ◽  
Author(s):  
F.R. Arutyunyan ◽  
V.A. Tumanyan

2021 ◽  
Author(s):  
Tiebin Yang ◽  
Feng Li ◽  
Rongkun Zheng

Perovskite halides hold great potential for high-energy radiation detection. Recent advancements in detecting alpha-, beta-, X-, and gamma-rays by perovskite halides are reviewed and an outlook on the device performance optimization is provided.


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