Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process

U. Bosch; W. D. Schmidt-Ott; P. Tidemand-Petersson; E. Runte; W. Hillebrandt; M. Lechle; F. K. Thielemann; R. Kirchner; O. Klepper; E. Roeckl; K. Rykaczewski; D. Schardt; N. Kaffrell; M. Bernas; Ph Dessagne; W. Kurcewicz

doi:10.1016/0370-2693(85)90023-1

Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process

U. Bosch
, W. D. Schmidt-Ott
, P. Tidemand-Petersson
, E. Runte
, W. Hillebrandt
, M. Lechle
, F. K. Thielemann
, R. Kirchner
, O. Klepper
, E. Roeckl
, K. Rykaczewski
, D. Schardt
, N. Kaffrell
, M. Bernas
, Ph Dessagne
, W. Kurcewicz

Nuclear Structure and Nuclear Astrophysi

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

51 Scopus citations

Abstract

Beta-decay studies of the new neutron-rich isotopes ^58,59Cr, ⁶³Mn, ^66,67Co and ⁶⁹Ni, yielding distinctly shorter half-lives than the corresponding theoretical predictions, are presented. The influence of the short half-lives on the r-process calculations of nuclear abundances is discussed. It is concluded that a significantly higher neutron density than the one obtained from explosive helium burning in supernovae is need to reproduce the observe abundances around A=80.

Original language	English
Pages (from-to)	22-26
Number of pages	5
Journal	Physics Letters B
Volume	164
Issue number	1-3
DOIs	https://doi.org/10.1016/0370-2693(85)90023-1
State	Published - Dec 5 1985

Access to Document

10.1016/0370-2693(85)90023-1

Cite this

Bosch, U., Schmidt-Ott, W. D., Tidemand-Petersson, P., Runte, E., Hillebrandt, W., Lechle, M., Thielemann, F. K., Kirchner, R., Klepper, O., Roeckl, E., Rykaczewski, K., Schardt, D., Kaffrell, N., Bernas, M., Dessagne, P., & Kurcewicz, W. (1985). Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process. Physics Letters B, 164(1-3), 22-26. https://doi.org/10.1016/0370-2693(85)90023-1

@article{605154184d6d4acc95248ab71576c577,

title = "Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process",

abstract = "Beta-decay studies of the new neutron-rich isotopes 58,59Cr, 63Mn, 66,67Co and 69Ni, yielding distinctly shorter half-lives than the corresponding theoretical predictions, are presented. The influence of the short half-lives on the r-process calculations of nuclear abundances is discussed. It is concluded that a significantly higher neutron density than the one obtained from explosive helium burning in supernovae is need to reproduce the observe abundances around A=80.",

author = "U. Bosch and Schmidt-Ott, \{W. D.\} and P. Tidemand-Petersson and E. Runte and W. Hillebrandt and M. Lechle and Thielemann, \{F. K.\} and R. Kirchner and O. Klepper and E. Roeckl and K. Rykaczewski and D. Schardt and N. Kaffrell and M. Bernas and Ph Dessagne and W. Kurcewicz",

year = "1985",

month = dec,

day = "5",

doi = "10.1016/0370-2693(85)90023-1",

language = "English",

volume = "164",

pages = "22--26",

journal = "Physics Letters B",

issn = "0370-2693",

publisher = "Elsevier",

number = "1-3",

}

Bosch, U, Schmidt-Ott, WD, Tidemand-Petersson, P, Runte, E, Hillebrandt, W, Lechle, M, Thielemann, FK, Kirchner, R, Klepper, O, Roeckl, E, Rykaczewski, K, Schardt, D, Kaffrell, N, Bernas, M, Dessagne, P & Kurcewicz, W 1985, 'Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process', Physics Letters B, vol. 164, no. 1-3, pp. 22-26. https://doi.org/10.1016/0370-2693(85)90023-1

TY - JOUR

T1 - Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process

AU - Bosch, U.

AU - Schmidt-Ott, W. D.

AU - Tidemand-Petersson, P.

AU - Runte, E.

AU - Hillebrandt, W.

AU - Lechle, M.

AU - Thielemann, F. K.

AU - Kirchner, R.

AU - Klepper, O.

AU - Roeckl, E.

AU - Rykaczewski, K.

AU - Schardt, D.

AU - Kaffrell, N.

AU - Bernas, M.

AU - Dessagne, Ph

AU - Kurcewicz, W.

PY - 1985/12/5

Y1 - 1985/12/5

N2 - Beta-decay studies of the new neutron-rich isotopes 58,59Cr, 63Mn, 66,67Co and 69Ni, yielding distinctly shorter half-lives than the corresponding theoretical predictions, are presented. The influence of the short half-lives on the r-process calculations of nuclear abundances is discussed. It is concluded that a significantly higher neutron density than the one obtained from explosive helium burning in supernovae is need to reproduce the observe abundances around A=80.

AB - Beta-decay studies of the new neutron-rich isotopes 58,59Cr, 63Mn, 66,67Co and 69Ni, yielding distinctly shorter half-lives than the corresponding theoretical predictions, are presented. The influence of the short half-lives on the r-process calculations of nuclear abundances is discussed. It is concluded that a significantly higher neutron density than the one obtained from explosive helium burning in supernovae is need to reproduce the observe abundances around A=80.

UR - https://www.scopus.com/pages/publications/0002438023

U2 - 10.1016/0370-2693(85)90023-1

DO - 10.1016/0370-2693(85)90023-1

M3 - Article

AN - SCOPUS:0002438023

SN - 0370-2693

VL - 164

SP - 22

EP - 26

JO - Physics Letters B

JF - Physics Letters B

IS - 1-3

ER -

Beta-decay half-lives of new neutron-rich chromium-to-nickel isotopes and their consequences for the astrophysical r-process

Abstract

Access to Document

Other files and links

Fingerprint

Cite this