Measurement of the 26Mg(p, n)26 Alg (7.2 × 105) yr cross section via accelerator mass spectrometry

M. Paul; W. Henning; W. Kutschera; E. J. Stephenson; J. L. Yntema

doi:10.1016/0370-2693(80)90883-7

Measurement of the ²⁶Mg(p, n)²⁶ Al^g (7.2 × 10⁵) yr cross section via accelerator mass spectrometry

M. Paul, W. Henning, W. Kutschera, E. J. Stephenson, J. L. Yntema

Argonne National Laboratory

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

35 Scopus citations

Abstract

The new technique of accelerator mass spectrometry was successfully applied to measure the ²⁶Mg(p, n)²⁶ Al^g (7.2 × 10⁵ yr) cross section for proton energies E_p = 5.2−6.9 MeV. This cross section thar threshold is of astrophysical interest because of the recently observed ²⁶Mg excess in meteoritic material and its bearing on the early solar system.

Original language	English
Pages (from-to)	303-306
Number of pages	4
Journal	Physics Letters B
Volume	94
Issue number	3
DOIs	https://doi.org/10.1016/0370-2693(80)90883-7
State	Published - 1980
Externally published	Yes

Access to Document

10.1016/0370-2693(80)90883-7

Cite this

@article{92647d79468646be8077bf2c425b4e74,

title = "Measurement of the 26Mg(p, n)26 Alg (7.2 × 105) yr cross section via accelerator mass spectrometry",

abstract = "The new technique of accelerator mass spectrometry was successfully applied to measure the 26Mg(p, n)26 Alg (7.2 × 105 yr) cross section for proton energies Ep = 5.2−6.9 MeV. This cross section thar threshold is of astrophysical interest because of the recently observed 26Mg excess in meteoritic material and its bearing on the early solar system.",

author = "M. Paul and W. Henning and W. Kutschera and Stephenson, {E. J.} and Yntema, {J. L.}",

year = "1980",

doi = "10.1016/0370-2693(80)90883-7",

language = "English",

volume = "94",

pages = "303--306",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier B.V.",

number = "3",

}

TY - JOUR

T1 - Measurement of the 26Mg(p, n)26 Alg (7.2 × 105) yr cross section via accelerator mass spectrometry

AU - Paul, M.

AU - Henning, W.

AU - Kutschera, W.

AU - Stephenson, E. J.

AU - Yntema, J. L.

PY - 1980

Y1 - 1980

N2 - The new technique of accelerator mass spectrometry was successfully applied to measure the 26Mg(p, n)26 Alg (7.2 × 105 yr) cross section for proton energies Ep = 5.2−6.9 MeV. This cross section thar threshold is of astrophysical interest because of the recently observed 26Mg excess in meteoritic material and its bearing on the early solar system.

AB - The new technique of accelerator mass spectrometry was successfully applied to measure the 26Mg(p, n)26 Alg (7.2 × 105 yr) cross section for proton energies Ep = 5.2−6.9 MeV. This cross section thar threshold is of astrophysical interest because of the recently observed 26Mg excess in meteoritic material and its bearing on the early solar system.

UR - http://www.scopus.com/inward/record.url?scp=85014077413&partnerID=8YFLogxK

U2 - 10.1016/0370-2693(80)90883-7

DO - 10.1016/0370-2693(80)90883-7

M3 - Article

AN - SCOPUS:85014077413

SN - 0370-2693

VL - 94

SP - 303

EP - 306

JO - Physics Letters B

JF - Physics Letters B

IS - 3

ER -

Measurement of the ²⁶Mg(p, n)²⁶ Al^g (7.2 × 10⁵) yr cross section via accelerator mass spectrometry

Abstract

Access to Document

Other files and links

Fingerprint

Cite this