Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy

J. Hu; H. Yamaguchi; Y. H. Lam; A. Heger; D. Kahl; A. M. Jacobs; Z. Johnston; S. W. Xu; N. T. Zhang; S. B. Ma; L. H. Ru; E. Q. Liu; T. Liu; S. Hayakawa; L. Yang; H. Shimizu; C. B. Hamill; A. St J. Murphy; J. Su; X. Fang; K. Y. Chae; M. S. Kwag; S. M. Cha; N. N. Duy; N. K. Uyen; D. H. Kim; R. G. Pizzone; M. La Cognata; S. Cherubini; S. Romano; A. Tumino; J. Liang; A. Psaltis; M. Sferrazza; D. Kim; Y. Y. Li; S. Kubono

doi:10.1103/PhysRevLett.127.172701

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy

J. Hu
, H. Yamaguchi
, Y. H. Lam
, A. Heger
, D. Kahl
, A. M. Jacobs
, Z. Johnston
, S. W. Xu
, N. T. Zhang
, S. B. Ma
, L. H. Ru
, E. Q. Liu
, T. Liu
, S. Hayakawa
, L. Yang
, H. Shimizu
, C. B. Hamill
, A. St J. Murphy
, J. Su
, X. Fang

K. Y. Chae, M. S. Kwag, S. M. Cha, N. N. Duy, N. K. Uyen, D. H. Kim, R. G. Pizzone, M. La Cognata, S. Cherubini, S. Romano, A. Tumino, J. Liang, A. Psaltis, M. Sferrazza, D. Kim, Y. Y. Li, S. Kubono

Department of Physics

CAS - Institute of Modern Physics
University of Chinese Academy of Sciences
The University of Tokyo
National Astronomical Observatory of Japan (NAOJ)
Monash University
Center of Excellence for Astrophysics in Three Dimensions (ASTRO-3D)
Michigan State University
Horia Hulubei National Institute of Physics and Nuclear Engineering
University of Edinburgh
Beijing Normal University
Sun Yat-Sen University
Sungkyunkwan University
Duy Tan University
National Institute for Nuclear Physics
University of Catania
CSFNSM
Kore University of Enna
McMaster University
Université libre de Bruxelles
Ewha Womans University
RIKEN

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

21 Scopus citations

Abstract

We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in contributing to the reaction at type I x-ray burst energies. We measured spin-parities of four resonances above the threshold of that are found to strongly impact the rate. The new rate advances a state-of-the-art model to remarkably reproduce light curves of the GS clocked burster with mean deviation and permits us to discover a strong correlation between the He abundance in the accreting envelope of the photospheric radius expansion burster and the dominance of branch.

Original language	English
Article number	172701
Journal	Physical Review Letters
Volume	127
Issue number	17
DOIs	https://doi.org/10.1103/PhysRevLett.127.172701
State	Published - 22 Oct 2021

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10.1103/PhysRevLett.127.172701

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Hu, J., Yamaguchi, H., Lam, Y. H., Heger, A., Kahl, D., Jacobs, A. M., Johnston, Z., Xu, S. W., Zhang, N. T., Ma, S. B., Ru, L. H., Liu, E. Q., Liu, T., Hayakawa, S., Yang, L., Shimizu, H., Hamill, C. B., Murphy, A. S. J., Su, J., ... Kubono, S. (2021). Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy. Physical Review Letters, 127(17), Article 172701. https://doi.org/10.1103/PhysRevLett.127.172701

@article{e4ecf69c58034b93b3a360098855f320,

title = "Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy",

abstract = "We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in contributing to the reaction at type I x-ray burst energies. We measured spin-parities of four resonances above the threshold of that are found to strongly impact the rate. The new rate advances a state-of-the-art model to remarkably reproduce light curves of the GS clocked burster with mean deviation and permits us to discover a strong correlation between the He abundance in the accreting envelope of the photospheric radius expansion burster and the dominance of branch.",

author = "J. Hu and H. Yamaguchi and Lam, \{Y. H.\} and A. Heger and D. Kahl and Jacobs, \{A. M.\} and Z. Johnston and Xu, \{S. W.\} and Zhang, \{N. T.\} and Ma, \{S. B.\} and Ru, \{L. H.\} and Liu, \{E. Q.\} and T. Liu and S. Hayakawa and L. Yang and H. Shimizu and Hamill, \{C. B.\} and Murphy, \{A. St J.\} and J. Su and X. Fang and Chae, \{K. Y.\} and Kwag, \{M. S.\} and Cha, \{S. M.\} and Duy, \{N. N.\} and Uyen, \{N. K.\} and Kim, \{D. H.\} and Pizzone, \{R. G.\} and \{La Cognata\}, M. and S. Cherubini and S. Romano and A. Tumino and J. Liang and A. Psaltis and M. Sferrazza and D. Kim and Li, \{Y. Y.\} and S. Kubono",

note = "Publisher Copyright: {\textcopyright} 2021 American Physical Society",

year = "2021",

month = oct,

day = "22",

doi = "10.1103/PhysRevLett.127.172701",

language = "English",

volume = "127",

journal = "Physical Review Letters",

issn = "0031-9007",

publisher = "American Physical Society",

number = "17",

}

Hu, J, Yamaguchi, H, Lam, YH, Heger, A, Kahl, D, Jacobs, AM, Johnston, Z, Xu, SW, Zhang, NT, Ma, SB, Ru, LH, Liu, EQ, Liu, T, Hayakawa, S, Yang, L, Shimizu, H, Hamill, CB, Murphy, ASJ, Su, J, Fang, X, Chae, KY, Kwag, MS, Cha, SM, Duy, NN, Uyen, NK, Kim, DH, Pizzone, RG, La Cognata, M, Cherubini, S, Romano, S, Tumino, A, Liang, J, Psaltis, A, Sferrazza, M, Kim, D, Li, YY & Kubono, S 2021, 'Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy', Physical Review Letters, vol. 127, no. 17, 172701. https://doi.org/10.1103/PhysRevLett.127.172701

TY - JOUR

T1 - Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy

AU - Hu, J.

AU - Yamaguchi, H.

AU - Lam, Y. H.

AU - Heger, A.

AU - Kahl, D.

AU - Jacobs, A. M.

AU - Johnston, Z.

AU - Xu, S. W.

AU - Zhang, N. T.

AU - Ma, S. B.

AU - Ru, L. H.

AU - Liu, E. Q.

AU - Liu, T.

AU - Hayakawa, S.

AU - Yang, L.

AU - Shimizu, H.

AU - Hamill, C. B.

AU - Murphy, A. St J.

AU - Su, J.

AU - Fang, X.

AU - Chae, K. Y.

AU - Kwag, M. S.

AU - Cha, S. M.

AU - Duy, N. N.

AU - Uyen, N. K.

AU - Kim, D. H.

AU - Pizzone, R. G.

AU - La Cognata, M.

AU - Cherubini, S.

AU - Romano, S.

AU - Tumino, A.

AU - Liang, J.

AU - Psaltis, A.

AU - Sferrazza, M.

AU - Kim, D.

AU - Li, Y. Y.

AU - Kubono, S.

PY - 2021/10/22

Y1 - 2021/10/22

N2 - We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in contributing to the reaction at type I x-ray burst energies. We measured spin-parities of four resonances above the threshold of that are found to strongly impact the rate. The new rate advances a state-of-the-art model to remarkably reproduce light curves of the GS clocked burster with mean deviation and permits us to discover a strong correlation between the He abundance in the accreting envelope of the photospheric radius expansion burster and the dominance of branch.

AB - We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in contributing to the reaction at type I x-ray burst energies. We measured spin-parities of four resonances above the threshold of that are found to strongly impact the rate. The new rate advances a state-of-the-art model to remarkably reproduce light curves of the GS clocked burster with mean deviation and permits us to discover a strong correlation between the He abundance in the accreting envelope of the photospheric radius expansion burster and the dominance of branch.

UR - https://www.scopus.com/pages/publications/85118117277

U2 - 10.1103/PhysRevLett.127.172701

DO - 10.1103/PhysRevLett.127.172701

M3 - Article

C2 - 34739292

AN - SCOPUS:85118117277

SN - 0031-9007

VL - 127

JO - Physical Review Letters

JF - Physical Review Letters

IS - 17

M1 - 172701

ER -

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New Reaction Rate Determined at the Gamow Energy

Abstract

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