Pulsar acceleration shifts from nearby supernova explosion

Kodwani Darsh; Pen Ue-Li; Yang I-Sheng

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Pulsar acceleration shifts from nearby supernova explosion

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摘要

We show that when a supernova explodes, a nearby pulsar signal goes through a very specific change. The observed period first changes smoothly, then is followed by a sudden change in the time derivative. A stable millisecond pulsar can allow us to measure such an effect. This may improve our measurement of the total energy released in neutrinos and also the orientation of the supernova-pulsar system.

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《Physical review, D》 |2016年第10期|共6页
作者
Kodwani Darsh; Pen Ue-Li; Yang I-Sheng;
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作者单位

Canadian Inst Theoret Astrophys, 60 St George St, Toronto, ON M5S 3H8, Canada;

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原文格式 PDF
正文语种英语
中图分类粒子物理学;场论;
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2. 60Fe: A Heat Source for Planetary Differentiation from a Nearby Supernova Explosion [J] . S. Mostefaoui1, G. W. Lugmair12, P. Hoppe1 The Astrophysical journal . 2005,第1期

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8. SUPERNOVA REMNANTS AND HIDDEN PULSARS, [R] . pacini, f. cavaliere, a. 1970

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Pulsar acceleration shifts from nearby supernova explosion

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