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Regulated NiCu Cycles with the New 57 Cu(p, γ ) 58 Zn Reaction Rate and the Influence on Type-I X-Ray Bursts: GS 1826–24 Clocked Burster
In Type-I X-ray bursts (XRBs), the rapid-proton capture (rp-) process passes through the NiCu and ZnGa cycles before reaching the region above Ge and Se isotopes that hydrogen burning actively powers the XRBs. The sensitivity study performed by Cyburt et al . [1] shows that the 57 Cu(p, γ ) 58 Zn re...
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Published in: | EPJ Web of conferences 2022, Vol.260, p.11023 |
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Main Authors: | , , , , , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | In Type-I X-ray bursts (XRBs), the rapid-proton capture (rp-) process passes through the NiCu and ZnGa cycles before reaching the region above Ge and Se isotopes that hydrogen burning actively powers the XRBs. The sensitivity study performed by Cyburt
et al
. [1] shows that the
57
Cu(p,
γ
)
58
Zn reaction in the NiCu cycles is the fifth most important rp-reaction influencing the burst light curves. Langer
et al
. [2] precisely measured some low-lying energy levels of
58
Zn to deduce the
57
Cu(p,
γ
)
58
Zn reaction rate. Nevertheless, the order of the 1
+
1
and 2
+
3
resonance states that dominate at 0:2 ≲
T
(GK) ≲ 0:8 is not confirmed. The 1
+
2
resonance state, which dominates at the XRB sensitive temperature regime 0:8 ≲
T
(GK) ≲ 2 was not detected. Using isobaric-multipletmass equation (IMME), we estimate the order of the 1
+
1
and 2
+
3
resonance states and estimate the lower limit of the 1
+
2
resonance energy. We then determine the
57
Cu(p,
γ
)
58
Zn reaction rate using the full
pf
-model space shell model calculations. The new rate is up to a factor of four lower than the Forstner
et al
. [3] rate recommended by JINA REACLIBv2.2. Using the present
57
Cu(p,
γ
)
58
Zn, the latest
56
Ni(p,
γ
)
57
Cu and
55
Ni(p,
γ
)
56
Cu reaction rates, and 1D implicit hydrodynamic K
epler
code, we model the thermonuclear XRBs of the clocked burster GS 1826–24. We find that the new rates regulate the reaction flow in the NiCu cycles and strongly influence the burst-ash composition. The
59
Cu(p,
γ
)
56
Ni and
59
Cu(p,
α
)
60
Zn reactions suppress the influence of the
57
Cu(p,
γ
)
58
Zn reaction. They strongly diminish the impact of the nuclear reaction flow that bypasses the
56
Ni waiting point induced by the
55
Ni(p,
γ
)
56
Cu reaction on burst light curve. |
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ISSN: | 2100-014X 2100-014X |
DOI: | 10.1051/epjconf/202226011023 |