skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Fast Radio Bursts’ Emission Mechanism: Implication from Localization

Abstract

We argue that the localization of the repeating fast radio bursts (FRBs) at ∼1 Gpc excludes a rotationally powered type of radio emission (e.g., analogs of Crab’s giant pulses coming from very young energetic pulsars) as the origin of FRBs.

Authors:
 [1]
  1. Department of Physics and Astronomy, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907-2036 (United States)
Publication Date:
OSTI Identifier:
22654507
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal Letters; Journal Volume: 838; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; EMISSION; NEUTRONS; PULSARS; SOLAR RADIO BURSTS; STARS

Citation Formats

Lyutikov, Maxim. Fast Radio Bursts’ Emission Mechanism: Implication from Localization. United States: N. p., 2017. Web. doi:10.3847/2041-8213/AA62FA.
Lyutikov, Maxim. Fast Radio Bursts’ Emission Mechanism: Implication from Localization. United States. doi:10.3847/2041-8213/AA62FA.
Lyutikov, Maxim. Mon . "Fast Radio Bursts’ Emission Mechanism: Implication from Localization". United States. doi:10.3847/2041-8213/AA62FA.
@article{osti_22654507,
title = {Fast Radio Bursts’ Emission Mechanism: Implication from Localization},
author = {Lyutikov, Maxim},
abstractNote = {We argue that the localization of the repeating fast radio bursts (FRBs) at ∼1 Gpc excludes a rotationally powered type of radio emission (e.g., analogs of Crab’s giant pulses coming from very young energetic pulsars) as the origin of FRBs.},
doi = {10.3847/2041-8213/AA62FA},
journal = {Astrophysical Journal Letters},
number = 1,
volume = 838,
place = {United States},
year = {Mon Mar 20 00:00:00 EDT 2017},
month = {Mon Mar 20 00:00:00 EDT 2017}
}