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Mass measurements show slowdown of rapid proton capture process at waiting-point nucleus 64Ge
by
Yang, J. C
, Zhou, X
, Jiao, H. Y
, Zhang, Y. H
, Xing, Y. M
, Huang, W. J
, Wang, M
, Hou, S. Q
, Sun, M. Z
, Wang, Q
, Li, H. F
, Zhou, X. H
, Li, J. G
, Zeng, Q
, Chen, R. J
, Shuai, P
, Meisel, Z
, Fu, C. Y
, Liao, T
, Niu, Y. F
, Zhang, S
, Ge, W. W
, Xu, X
, Litvinov, Yu. A
, Song, Y. N
, Yuan, Q
, Xu, H. S
, Xu, F. R
, Deng, H. Y
, Yuan, Y. J
, Yu, Y
, Shi, J. Y
, Yan, X. L
, Li, K. A
, Liu, M. L
, Zhang, M
, He, J. J
, Litvinov, S. A
, Blaum, K
in
Binary stars
/ Bursts
/ Celestial bodies
/ Companion stars
/ Deposition
/ Light curve
/ Neutron stars
/ Neutrons
/ Nuclear fusion
/ Nuclear reactions
/ Nuclides
/ Protons
/ Spaceborne telescopes
/ Stars
/ Thermonuclear explosions
2023
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Mass measurements show slowdown of rapid proton capture process at waiting-point nucleus 64Ge
by
Yang, J. C
, Zhou, X
, Jiao, H. Y
, Zhang, Y. H
, Xing, Y. M
, Huang, W. J
, Wang, M
, Hou, S. Q
, Sun, M. Z
, Wang, Q
, Li, H. F
, Zhou, X. H
, Li, J. G
, Zeng, Q
, Chen, R. J
, Shuai, P
, Meisel, Z
, Fu, C. Y
, Liao, T
, Niu, Y. F
, Zhang, S
, Ge, W. W
, Xu, X
, Litvinov, Yu. A
, Song, Y. N
, Yuan, Q
, Xu, H. S
, Xu, F. R
, Deng, H. Y
, Yuan, Y. J
, Yu, Y
, Shi, J. Y
, Yan, X. L
, Li, K. A
, Liu, M. L
, Zhang, M
, He, J. J
, Litvinov, S. A
, Blaum, K
in
Binary stars
/ Bursts
/ Celestial bodies
/ Companion stars
/ Deposition
/ Light curve
/ Neutron stars
/ Neutrons
/ Nuclear fusion
/ Nuclear reactions
/ Nuclides
/ Protons
/ Spaceborne telescopes
/ Stars
/ Thermonuclear explosions
2023
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Mass measurements show slowdown of rapid proton capture process at waiting-point nucleus 64Ge
by
Yang, J. C
, Zhou, X
, Jiao, H. Y
, Zhang, Y. H
, Xing, Y. M
, Huang, W. J
, Wang, M
, Hou, S. Q
, Sun, M. Z
, Wang, Q
, Li, H. F
, Zhou, X. H
, Li, J. G
, Zeng, Q
, Chen, R. J
, Shuai, P
, Meisel, Z
, Fu, C. Y
, Liao, T
, Niu, Y. F
, Zhang, S
, Ge, W. W
, Xu, X
, Litvinov, Yu. A
, Song, Y. N
, Yuan, Q
, Xu, H. S
, Xu, F. R
, Deng, H. Y
, Yuan, Y. J
, Yu, Y
, Shi, J. Y
, Yan, X. L
, Li, K. A
, Liu, M. L
, Zhang, M
, He, J. J
, Litvinov, S. A
, Blaum, K
in
Binary stars
/ Bursts
/ Celestial bodies
/ Companion stars
/ Deposition
/ Light curve
/ Neutron stars
/ Neutrons
/ Nuclear fusion
/ Nuclear reactions
/ Nuclides
/ Protons
/ Spaceborne telescopes
/ Stars
/ Thermonuclear explosions
2023
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Mass measurements show slowdown of rapid proton capture process at waiting-point nucleus 64Ge
Journal Article
Mass measurements show slowdown of rapid proton capture process at waiting-point nucleus 64Ge
2023
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Overview
X-ray bursts are among the brightest stellar objects frequently observed in the sky by space-based telescopes. A type-I X-ray burst is understood as a violent thermonuclear explosion on the surface of a neutron star, accreting matter from a companion star in a binary system. The bursts are powered by a nuclear reaction sequence known as the rapid proton capture process (rp process), which involves hundreds of exotic neutron-deficient nuclides. At so-called waiting-point nuclides, the process stalls until a slower β+ decay enables a bypass. One of the handful of rp process waiting-point nuclides is 64Ge, which plays a decisive role in matter flow and therefore the produced X-ray flux. Here we report precision measurements of the masses of 63Ge, 64,65As and 66,67Se—the relevant nuclear masses around the waiting-point 64Ge—and use them as inputs for X-ray burst model calculations. We obtain the X-ray burst light curve to constrain the neutron-star compactness, and suggest that the distance to the X-ray burster GS 1826–24 needs to be increased by about 6.5% to match astronomical observations. The nucleosynthesis results affect the thermal structure of accreting neutron stars, which will subsequently modify the calculations of associated observables.Rapid proton capture nucleosynthesis stalls at waiting-point nuclides, including 64Ge. Precision mass measurements in the vicinity of this nuclide influence state-of-the-art calculations of X-ray bursts from accreting neutron stars.
Publisher
Nature Publishing Group
Subject
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