Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions

Fujita Y; Adachi T; Blank B; von Brentano P; Berg GPA; Fujita H; Fujita K; Hatanaka K; Nakanishi K; Negret A; Lucia Popescu; Rubio B; Shimbara Y; Shimizu Y; Tameshinge Y; Tamii A; Yosoi M; Zell KO; Dieter Pauwels

Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions

Fujita Y
, Adachi T
, Blank B
, von Brentano P
, Berg GPA
, Fujita H
, Fujita K
, Hatanaka K
, Nakanishi K
, Negret A
, Lucia Popescu
, Rubio B
, Shimbara Y
, Shimizu Y
, Tameshinge Y
, Tamii A
, Yosoi M
, Zell KO
, Dieter Pauwels

Research output › peer-review

Abstract

The rp-process nucleosynthesis proceeds through nuclei near the proton drip-line, in which Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei play important roles. In the beta-decay study of these nuclei, half-lives can be measured rather accurately. On the other hand, in the high-resolution (3He,t) charge-exchange reactions on mirror nuclei, individual GT transitions can be studied up to high excitations. For the accurate study of the GT transition strengths in the A = 52, T = 2 system, we compare and combine the beta-decay study of the proton-rich nucleus 52Ni and the 52Cr(3He,t) measurement assuming the isospin symmetry of the Tz = +/- 2 -> +/- 1 transitions.

Original language	English
Title of host publication	The 10th International Symposium on Origin of Matter and Evolutions of Galaxies : OMEG—2010
Place of Publication	Melville, New York, United States
Pages	436-438
Volume	1
State	Published - Oct 2010
Event	The 10th International Symposium on Origin of Matter and Evolution of Galaxies: OMEG - 2010 - Osaka Duration: 8 Mar 2010 → 10 Mar 2010

Publication series

Name	AIP Conference Proceedings
Number	1269

Conference

Conference	The 10th International Symposium on Origin of Matter and Evolution of Galaxies: OMEG - 2010
Country/Territory	Japan
City	Osaka
Period	2010-03-08 → 2010-03-10

Cite this

Y, F., T, A., B, B., P, V. B., GPA, B., H, F., K, F., K, H., K, N., A, N., Popescu, L., B, R., Y, S., Y, S., Y, T., A, T., M, Y., KO, Z., & Pauwels, D. (2010). Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions. In The 10th International Symposium on Origin of Matter and Evolutions of Galaxies : OMEG—2010 (Vol. 1, pp. 436-438). (AIP Conference Proceedings; No. 1269)..

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title = "Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions",

abstract = "The rp-process nucleosynthesis proceeds through nuclei near the proton drip-line, in which Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei play important roles. In the beta-decay study of these nuclei, half-lives can be measured rather accurately. On the other hand, in the high-resolution (3He,t) charge-exchange reactions on mirror nuclei, individual GT transitions can be studied up to high excitations. For the accurate study of the GT transition strengths in the A = 52, T = 2 system, we compare and combine the beta-decay study of the proton-rich nucleus 52Ni and the 52Cr(3He,t) measurement assuming the isospin symmetry of the Tz = +/- 2 -> +/- 1 transitions.",

keywords = "nuclear structure, symmetry, decay, RCNP, weak interaction",

author = "Fujita Y and Adachi T and Blank B and P, \{von Brentano\} and Berg GPA and Fujita H and Fujita K and Hatanaka K and Nakanishi K and Negret A and Lucia Popescu and Rubio B and Shimbara Y and Shimizu Y and Tameshinge Y and Tamii A and Yosoi M and Zell KO and Dieter Pauwels",

year = "2010",

month = oct,

language = "English",

isbn = "978-0-7354-0819-7",

volume = "1",

series = "AIP Conference Proceedings",

number = "1269",

pages = "436--438",

booktitle = "The 10th International Symposium on Origin of Matter and Evolutions of Galaxies : OMEG—2010",

note = "The 10th International Symposium on Origin of Matter and Evolution of Galaxies: OMEG - 2010 ; Conference date: 08-03-2010 Through 10-03-2010",

}

Y, F, T, A, B, B, P, VB, GPA, B, H, F, K, F, K, H, K, N, A, N, Popescu, L, B, R, Y, S, Y, S, Y, T, A, T, M, Y, KO, Z & Pauwels, D 2010, Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions. in The 10th International Symposium on Origin of Matter and Evolutions of Galaxies : OMEG—2010. vol. 1, AIP Conference Proceedings, no. 1269, Melville, New York, United States, pp. 436-438, The 10th International Symposium on Origin of Matter and Evolution of Galaxies: OMEG - 2010, Osaka, Japan, 2010-03-08.

TY - GEN

T1 - Gamow-Teller Transitions in Proton Rich Exotic pf-shell Nuclei Deduced from Mirror Transitions

AU - Y, Fujita

AU - T, Adachi

AU - B, Blank

AU - P, von Brentano

AU - GPA, Berg

AU - H, Fujita

AU - K, Fujita

AU - K, Hatanaka

AU - K, Nakanishi

AU - A, Negret

AU - Popescu, Lucia

AU - B, Rubio

AU - Y, Shimbara

AU - Y, Shimizu

AU - Y, Tameshinge

AU - A, Tamii

AU - M, Yosoi

AU - KO, Zell

A2 - Pauwels, Dieter

PY - 2010/10

Y1 - 2010/10

N2 - The rp-process nucleosynthesis proceeds through nuclei near the proton drip-line, in which Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei play important roles. In the beta-decay study of these nuclei, half-lives can be measured rather accurately. On the other hand, in the high-resolution (3He,t) charge-exchange reactions on mirror nuclei, individual GT transitions can be studied up to high excitations. For the accurate study of the GT transition strengths in the A = 52, T = 2 system, we compare and combine the beta-decay study of the proton-rich nucleus 52Ni and the 52Cr(3He,t) measurement assuming the isospin symmetry of the Tz = +/- 2 -> +/- 1 transitions.

AB - The rp-process nucleosynthesis proceeds through nuclei near the proton drip-line, in which Gamow-Teller (GT) transitions starting from unstable pf-shell nuclei play important roles. In the beta-decay study of these nuclei, half-lives can be measured rather accurately. On the other hand, in the high-resolution (3He,t) charge-exchange reactions on mirror nuclei, individual GT transitions can be studied up to high excitations. For the accurate study of the GT transition strengths in the A = 52, T = 2 system, we compare and combine the beta-decay study of the proton-rich nucleus 52Ni and the 52Cr(3He,t) measurement assuming the isospin symmetry of the Tz = +/- 2 -> +/- 1 transitions.

KW - nuclear structure

KW - symmetry

KW - decay

KW - RCNP

KW - weak interaction

UR - http://ecm.sckcen.be/OTCS/llisapi.dll/open/ezp_116117

UR - http://knowledgecentre.sckcen.be/so2/bibref/8341

M3 - In-proceedings paper

SN - 978-0-7354-0819-7

VL - 1

T3 - AIP Conference Proceedings

SP - 436

EP - 438

BT - The 10th International Symposium on Origin of Matter and Evolutions of Galaxies : OMEG—2010

CY - Melville, New York, United States

T2 - The 10th International Symposium on Origin of Matter and Evolution of Galaxies: OMEG - 2010

Y2 - 8 March 2010 through 10 March 2010

ER -