Thermonclear origin of rare neutron-rich isotopes

W. Michael Howard; W. David Arnett; Donald D. Clayton; Stanford E. Woosley

doi:10.1103/PhysRevLett.27.1607

Thermonclear origin of rare neutron-rich isotopes

W. Michael Howard, W. David Arnett, Donald D. Clayton, Stanford E. Woosley

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

2 Scopus citations

Abstract

Many rare neutron-rich isotopes in the range 16<34 can be synthesized from seed nuclei exposed to explosive carbon burning. This process, which involves no new astrophysical parameters, can solve most of the outstanding problems in the thermonuclear synthesis of elements in the range 34.

Original language	English (US)
Pages (from-to)	1607-1610
Number of pages	4
Journal	Physical review letters
Volume	27
Issue number	23
DOIs	https://doi.org/10.1103/PhysRevLett.27.1607
State	Published - 1971
Externally published	Yes

ASJC Scopus subject areas

General Physics and Astronomy

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10.1103/PhysRevLett.27.1607

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title = "Thermonclear origin of rare neutron-rich isotopes",

abstract = "Many rare neutron-rich isotopes in the range 16<34 can be synthesized from seed nuclei exposed to explosive carbon burning. This process, which involves no new astrophysical parameters, can solve most of the outstanding problems in the thermonuclear synthesis of elements in the range 34.",

author = "Howard, {W. Michael} and Arnett, {W. David} and Clayton, {Donald D.} and Woosley, {Stanford E.}",

year = "1971",

doi = "10.1103/PhysRevLett.27.1607",

language = "English (US)",

volume = "27",

pages = "1607--1610",

journal = "Physical review letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "23",

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T1 - Thermonclear origin of rare neutron-rich isotopes

AU - Howard, W. Michael

AU - Arnett, W. David

AU - Clayton, Donald D.

AU - Woosley, Stanford E.

PY - 1971

Y1 - 1971

N2 - Many rare neutron-rich isotopes in the range 16<34 can be synthesized from seed nuclei exposed to explosive carbon burning. This process, which involves no new astrophysical parameters, can solve most of the outstanding problems in the thermonuclear synthesis of elements in the range 34.

AB - Many rare neutron-rich isotopes in the range 16<34 can be synthesized from seed nuclei exposed to explosive carbon burning. This process, which involves no new astrophysical parameters, can solve most of the outstanding problems in the thermonuclear synthesis of elements in the range 34.

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U2 - 10.1103/PhysRevLett.27.1607

DO - 10.1103/PhysRevLett.27.1607

M3 - Article

AN - SCOPUS:35949033240

SN - 0031-9007

VL - 27

SP - 1607

EP - 1610

JO - Physical review letters

JF - Physical review letters

IS - 23

ER -

Thermonclear origin of rare neutron-rich isotopes

Abstract

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