TY - JOUR
T1 - Synchrotron maser from weakly magnetised neutron stars as the emission mechanism of fast radio bursts
AU - Long, Killian
AU - Pe'Er, Asaf
N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0).
PY - 2019
Y1 - 2019
N2 - The origin of Fast Radio Bursts (FRBs) is still mysterious. All FRBs to date show extremely high brightness temperatures, requiring a coherent emission mechanism. Using constraints derived from the physics of one of these mechanisms, the synchrotron maser, as well as observations, we show that accretion induced explosions of neutron stars with surface magnetic fields of B∗ . 1011 G are favoured as FRB progenitors.
AB - The origin of Fast Radio Bursts (FRBs) is still mysterious. All FRBs to date show extremely high brightness temperatures, requiring a coherent emission mechanism. Using constraints derived from the physics of one of these mechanisms, the synchrotron maser, as well as observations, we show that accretion induced explosions of neutron stars with surface magnetic fields of B∗ . 1011 G are favoured as FRB progenitors.
UR - http://www.scopus.com/inward/record.url?scp=85081135292&partnerID=8YFLogxK
M3 - مقالة من مؤنمر
SN - 1824-8039
VL - 354
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 048
T2 - 7th High Energy Phenomena in Relativistic Outflows, HEPRO 2019
Y2 - 9 July 2019 through 12 July 2019
ER -