Axion emissivity from the conversion of a neutron star into a strange star

In Saeng Suh; Chul H. Lee

doi:10.1016/S0370-2693(98)00597-8

Axion emissivity from the conversion of a neutron star into a strange star

In Saeng Suh, Chul H. Lee

Research output: Contribution to journal › Article › peer-review

3 Scopus citations

Abstract

The conversion of neutron matter into strange matter in a neutron star occurs through the non-leptonic weak-interaction process. We study the energy loss of the neutron star by the emission of axions in that process. Owing to that process, the neutron star will liberate the energy which can in no way be negligible as an axion burst.

Original language	English
Pages (from-to)	145-150
Number of pages	6
Journal	Physics Letters B
Volume	432
Issue number	1-2
DOIs	https://doi.org/10.1016/S0370-2693(98)00597-8
State	Published - Jul 23 1998
Externally published	Yes

Funding

We would like to thank Prof. N. Iwamoto and Prof. K. Choi for their encouraging comments. This work is supported in part by the Basic Science Institute Program, Korean Ministry of Education (Project No. BSRI-97-2441) and in part by the KOSEF through the Center for Theoretical Physics of Seoul National University.

Funders	Funder number
Ministry of Education	BSRI-97-2441
Korea Basic Science Institute
Korea Science and Engineering Foundation

Keywords

Astrophysics
Axions
Neutron stars
Strange star

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10.1016/S0370-2693(98)00597-8

Cite this

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abstract = "The conversion of neutron matter into strange matter in a neutron star occurs through the non-leptonic weak-interaction process. We study the energy loss of the neutron star by the emission of axions in that process. Owing to that process, the neutron star will liberate the energy which can in no way be negligible as an axion burst.",

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AU - Lee, Chul H.

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AB - The conversion of neutron matter into strange matter in a neutron star occurs through the non-leptonic weak-interaction process. We study the energy loss of the neutron star by the emission of axions in that process. Owing to that process, the neutron star will liberate the energy which can in no way be negligible as an axion burst.

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KW - Neutron stars

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ER -

Axion emissivity from the conversion of a neutron star into a strange star

Abstract

Funding

Keywords

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