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Author
dc.contributor.author
Csótó, A 
Author
dc.contributor.author
Oberhummer, H 
Author
dc.contributor.author
Schlattl, H 
Availability Date
dc.date.accessioned
2020-08-07T08:32:25Z
Availability Date
dc.date.available
2020-08-07T08:32:25Z
Release
dc.date.issued
2001
uri
dc.identifier.uri
http://hdl.handle.net/10831/49587
Abstract
dc.description.abstract
We show that the synthesis of carbon and oxygen through the triple-alpha process in red giant stars is extremely sensitive to the fine details of the nucleon-nucleon (N-N) interaction. A ±0.5% change in the strength of the N-N force would reduce either the carbon or oxygen abundance by as much as a factor of 30-1000. This result may be used to constrain some fundamental parameters of the Standard Model.
Language
dc.language
Angol
Title
dc.title
Fine-tuning the basic forces of nature through the triple-alpha process in red giant stars
Type
dc.type
folyóiratcikk
Date Change
dc.date.updated
2020-06-10T10:45:17Z
Scope
dc.format.page
560c-562c
Doi ID
dc.identifier.doi
10.1016/S0375-9474(01)00787-4
Wos ID
dc.identifier.wos
000168799300131
ID Scopus
dc.identifier.scopus
0035927306
MTMT ID
dc.identifier.mtmt
2284257
Issue Number
dc.identifier.issue
1-2
abbreviated journal
dc.identifier.jabbrev
NUCL PHYS A
Journal
dc.identifier.jtitle
NUCLEAR PHYSICS A
Volume Number
dc.identifier.volume
688
Release Date
dc.description.issuedate
2001
department of Author
dc.contributor.institution
MTA Atommagkutató Intézet
department of Author
dc.contributor.institution
Atomfizikai Tanszék
Author institution
dc.contributor.department
Atomfizikai Tanszék


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Fine-tuning the basic forces of nature through the triple-alpha process in red giant stars
 

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