Gamow-Teller transitions from 56Ni

M. Sasano; G. Perdikakis; R. G.T. Zegers; Sam M. Austin; D. Bazin; B. A. Brown; C. Caesar; A. L. Cole; J. M. Deaven; N. Ferrante; C. J. Guess; G. W. Hitt; H. Honma; R. Meharchand; F. Montes; J. Palardy; A. Prinke; L. A. Riley; H. Sakai; M. Scott; A. Stolz; T. Suzuki; L. Valdez; K. Yako

doi:10.1063/1.4763384

Gamow-Teller transitions from ⁵⁶Ni

M. Sasano, G. Perdikakis, R. G.T. Zegers, Sam M. Austin, D. Bazin, B. A. Brown, C. Caesar, A. L. Cole, J. M. Deaven, N. Ferrante, C. J. Guess, G. W. Hitt, H. Honma, R. Meharchand, F. Montes, J. Palardy, A. Prinke, L. A. Riley, H. Sakai, M. ScottA. Stolz, T. Suzuki, L. Valdez, K. Yako

Physics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

Abstract

A new technique to measure (p,n) charge-exchange reactions in inverse kinematics at intermediate energies on unstable isotopes was successfully developed and used to study the ⁵⁶Ni(p,n) reaction at 110 MeV/u. Gamow-Teller transition strengths from ⁵⁶Ni to ⁵⁶Cu were obtained and compared with shell-model predictions in the pf-shell using the KB3G and GXPF1A interactions. The calculations with the GXPF1A interaction reproduce the experimental GT strength distribution much better than the calculations that employed the KB3G interaction, indicating deficiencies in the spin-orbit and proton-neutron residual potentials for the latter. The results are important for improving the description of electron-capture rates on nuclei in the iron region, which are important for modeling the late evolution of core-collapse and thermonuclear supernovae.

Original language	English
Title of host publication	Origin of Matter and Evolution of Galaxies 2011
Pages	125-130
Number of pages	6
DOIs	https://doi.org/10.1063/1.4763384
State	Published - 2012
Event	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011 - Wako, Japan Duration: Nov 14 2011 → Nov 17 2011

Publication series

Name	AIP Conference Proceedings
Volume	1484
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011
Country/Territory	Japan
City	Wako
Period	11/14/11 → 11/17/11

Keywords

Charge-exchange reactions
Electron capture
Gamow-Teller transition
Ni

Access to Document

10.1063/1.4763384

Cite this

Sasano, M., Perdikakis, G., Zegers, R. G. T., Austin, S. M., Bazin, D., Brown, B. A., Caesar, C., Cole, A. L., Deaven, J. M., Ferrante, N., Guess, C. J., Hitt, G. W., Honma, H., Meharchand, R., Montes, F., Palardy, J., Prinke, A., Riley, L. A., Sakai, H., ... Yako, K. (2012). Gamow-Teller transitions from ⁵⁶Ni. In Origin of Matter and Evolution of Galaxies 2011 (pp. 125-130). (AIP Conference Proceedings; Vol. 1484). https://doi.org/10.1063/1.4763384

@inproceedings{6c85c5162b5f413e8493179ac1ecaf55,

title = "Gamow-Teller transitions from 56Ni",

abstract = "A new technique to measure (p,n) charge-exchange reactions in inverse kinematics at intermediate energies on unstable isotopes was successfully developed and used to study the 56Ni(p,n) reaction at 110 MeV/u. Gamow-Teller transition strengths from 56Ni to 56Cu were obtained and compared with shell-model predictions in the pf-shell using the KB3G and GXPF1A interactions. The calculations with the GXPF1A interaction reproduce the experimental GT strength distribution much better than the calculations that employed the KB3G interaction, indicating deficiencies in the spin-orbit and proton-neutron residual potentials for the latter. The results are important for improving the description of electron-capture rates on nuclei in the iron region, which are important for modeling the late evolution of core-collapse and thermonuclear supernovae.",

keywords = "Charge-exchange reactions, Electron capture, Gamow-Teller transition, Ni",

author = "M. Sasano and G. Perdikakis and Zegers, {R. G.T.} and Austin, {Sam M.} and D. Bazin and Brown, {B. A.} and C. Caesar and Cole, {A. L.} and Deaven, {J. M.} and N. Ferrante and Guess, {C. J.} and Hitt, {G. W.} and H. Honma and R. Meharchand and F. Montes and J. Palardy and A. Prinke and Riley, {L. A.} and H. Sakai and M. Scott and A. Stolz and T. Suzuki and L. Valdez and K. Yako",

year = "2012",

doi = "10.1063/1.4763384",

language = "English",

isbn = "9780735410961",

series = "AIP Conference Proceedings",

pages = "125--130",

booktitle = "Origin of Matter and Evolution of Galaxies 2011",

note = "null ; Conference date: 14-11-2011 Through 17-11-2011",

}

Sasano, M, Perdikakis, G, Zegers, RGT, Austin, SM, Bazin, D, Brown, BA, Caesar, C, Cole, AL, Deaven, JM, Ferrante, N, Guess, CJ, Hitt, GW, Honma, H, Meharchand, R, Montes, F, Palardy, J, Prinke, A, Riley, LA, Sakai, H, Scott, M, Stolz, A, Suzuki, T, Valdez, L & Yako, K 2012, Gamow-Teller transitions from ⁵⁶Ni. in Origin of Matter and Evolution of Galaxies 2011. AIP Conference Proceedings, vol. 1484, pp. 125-130, International Symposium on Origin of Matter and Evolutions of Galaxies 2011, OMEG 2011, Wako, Japan, 11/14/11. https://doi.org/10.1063/1.4763384

TY - GEN

T1 - Gamow-Teller transitions from 56Ni

AU - Sasano, M.

AU - Perdikakis, G.

AU - Zegers, R. G.T.

AU - Austin, Sam M.

AU - Bazin, D.

AU - Brown, B. A.

AU - Caesar, C.

AU - Cole, A. L.

AU - Deaven, J. M.

AU - Ferrante, N.

AU - Guess, C. J.

AU - Hitt, G. W.

AU - Honma, H.

AU - Meharchand, R.

AU - Montes, F.

AU - Palardy, J.

AU - Prinke, A.

AU - Riley, L. A.

AU - Sakai, H.

AU - Scott, M.

AU - Stolz, A.

AU - Suzuki, T.

AU - Valdez, L.

AU - Yako, K.

PY - 2012

Y1 - 2012

N2 - A new technique to measure (p,n) charge-exchange reactions in inverse kinematics at intermediate energies on unstable isotopes was successfully developed and used to study the 56Ni(p,n) reaction at 110 MeV/u. Gamow-Teller transition strengths from 56Ni to 56Cu were obtained and compared with shell-model predictions in the pf-shell using the KB3G and GXPF1A interactions. The calculations with the GXPF1A interaction reproduce the experimental GT strength distribution much better than the calculations that employed the KB3G interaction, indicating deficiencies in the spin-orbit and proton-neutron residual potentials for the latter. The results are important for improving the description of electron-capture rates on nuclei in the iron region, which are important for modeling the late evolution of core-collapse and thermonuclear supernovae.

AB - A new technique to measure (p,n) charge-exchange reactions in inverse kinematics at intermediate energies on unstable isotopes was successfully developed and used to study the 56Ni(p,n) reaction at 110 MeV/u. Gamow-Teller transition strengths from 56Ni to 56Cu were obtained and compared with shell-model predictions in the pf-shell using the KB3G and GXPF1A interactions. The calculations with the GXPF1A interaction reproduce the experimental GT strength distribution much better than the calculations that employed the KB3G interaction, indicating deficiencies in the spin-orbit and proton-neutron residual potentials for the latter. The results are important for improving the description of electron-capture rates on nuclei in the iron region, which are important for modeling the late evolution of core-collapse and thermonuclear supernovae.

KW - Charge-exchange reactions

KW - Electron capture

KW - Gamow-Teller transition

KW - Ni

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U2 - 10.1063/1.4763384

DO - 10.1063/1.4763384

M3 - Conference contribution

AN - SCOPUS:84874533599

SN - 9780735410961

T3 - AIP Conference Proceedings

SP - 125

EP - 130

BT - Origin of Matter and Evolution of Galaxies 2011

Y2 - 14 November 2011 through 17 November 2011

ER -