Relative Production Rates of 6He, 9Be, 12C in Astrophysical Environments

R. de Diego; E. Garrido; Dmitri Vladimir Fedorov; A.S. Jensen

doi:10.1007/s00601-010-0162-0

Relative Production Rates of ⁶He, ⁹Be, ¹²C in Astrophysical Environments

R. de Diego, E. Garrido, Dmitri Vladimir Fedorov, A.S. Jensen

Institut for Fysik og Astronomi

Publikation: Bidrag til tidsskrift/Konferencebidrag i tidsskrift /Bidrag til avis › Konferenceartikel › Forskning › peer review

1 Citationer (Scopus)

Abstract

We assume an environment of neutrons and α-particles of given density and temperature where nuclear syntheses into He, Be, and C are possible. The resulting relative abundance as a function of density and temperature is investigated.

Originalsprog	Engelsk
Tidsskrift	Few-Body Systems
Vol/bind	50
Nummer	1-4
Sider (fra-til)	331-333
Antal sider	3
ISSN	0177-7963
DOI	https://doi.org/10.1007/s00601-010-0162-0
Status	Udgivet - 2011
Begivenhed	21st European Conference on Few-Body Problems in Physics - Salamanca, Spanien Varighed: 30 aug. 2010 → 3 sep. 2010

Konference

Konference	21st European Conference on Few-Body Problems in Physics
Land/Område	Spanien
By	Salamanca
Periode	30/08/2010 → 03/09/2010

Adgang til dokumentet

10.1007/s00601-010-0162-0

Andre filer og links

Link to publication in Scopus

Citationsformater

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title = "Relative Production Rates of 6He, 9Be, 12C in Astrophysical Environments",

abstract = "We assume an environment of neutrons and α-particles of given density and temperature where nuclear syntheses into He, Be, and C are possible. The resulting relative abundance as a function of density and temperature is investigated.",

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language = "English",

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AU - de Diego, R.

AU - Garrido, E.

AU - Fedorov, Dmitri Vladimir

AU - Jensen, A.S.

PY - 2011

Y1 - 2011

N2 - We assume an environment of neutrons and α-particles of given density and temperature where nuclear syntheses into He, Be, and C are possible. The resulting relative abundance as a function of density and temperature is investigated.

AB - We assume an environment of neutrons and α-particles of given density and temperature where nuclear syntheses into He, Be, and C are possible. The resulting relative abundance as a function of density and temperature is investigated.

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U2 - 10.1007/s00601-010-0162-0

DO - 10.1007/s00601-010-0162-0

M3 - Conference article

AN - SCOPUS:79955132376

SN - 0177-7963

VL - 50

SP - 331

EP - 333

JO - Few-Body Systems

JF - Few-Body Systems

IS - 1-4

T2 - 21st European Conference on Few-Body Problems in Physics

Y2 - 30 August 2010 through 3 September 2010

ER -