Published December 12, 2022 | Version 1.0.0
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XRB_LightCurves_Ashes

Creators

  • 1. CAS Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, 730000, China; School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing, 100049, China
  • 2. GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, Darmstadt, 64291, Germany
  • 3. Institute of Nuclear and Particle Physics, Department of Physics and Astronomy, Ohio University, Athens, Ohio, 45701, USA
  • 4. Max-Planck-Institut fu ̈r Kernphysik, Saupfercheckweg 1, Heidelberg, 69117, Germany
  • 5. CAS Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, 730000, China; School of Nuclear Science and Technology, University of Chinese Academy of Sciences, Beijing, 100049, China; NuGrid Collaboration, http://www.nugridstars.org
  • 6. CAS Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, 730000, China
  • 7. CAS Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, 730000, China; GSI Helmholtzzentrum fu ̈r Schwerionenforschung, Planckstraße 1, Darmstadt, 64291, Germany
  • 8. Key Laboratory of Beam Technology of Ministry of Education, College of Nuclear Science and Technology, Beijing Normal University, Beijing, 100875, China
  • 9. Advanced Energy Science and Technology Guangdong Laboratory, Huizhou, 516007, China; CAS Key Laboratory of High Precision Nuclear Spectroscopy, Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou, 730000, China
  • 10. School of Nuclear Science and Technology, Lanzhou University, Lanzhou, 730000, China
  • 11. State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing, 100871, China
  • 12. School of Nuclear Science and Engineering, East China University of Technology, Nanchang, 330013, China

Description

Results of multi-zone x-ray burst simulations with new masses measured at the storage ring CSRe in Institute of Modern Physics, Chinese Academy of Sciences by employing the newly developed Br-IMS technique [1]. These data sets supplement dedicated publication, where they are cited, illustrated and interpreted. 

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XRB_Asches_Var16_Prof41.txt

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Additional details

References

  • M. Wang et al., Bρ-defined isochronous mass spectrometry: An approach for high-precision mass measurements of short-lived nuclei , Physical Review C 106 (2022) L051301, doi: 10.1103/PhysRevC.106.L051301
  • T. Yamaguchi et al., Masses of exotic nuclei, Progress in Particle and Nuclear Physics 120 (2021) 103882, doi: 10.1016/j.ppnp.2021.103882
  • B. Paxton et al., Modules for experiments in stellar astrophysics (MESA), Astrophys. J. Suppl. Ser. 192, 3 (2011), doi: 10.1088/0067-0049/192/1/3
  • B. Paxton et al., Modules for experiments in stellar astrophysics (MESA): planets, oscillations, rotation, and massive stars, Astrophys. J. Suppl. Ser. 208, 4 (2013), doi: 10.1088/0067-0049/208/1/4
  • B. Paxton et al., Modules for experiments in stellar astrophysics (MESA): binaries, pulsations, and explosions, Astrophys. J. Suppl. Ser. 220, 15 (2015). https://doi.org/10.1088/0067-0049/220/1/15. Erra- tum, Astrophys. J. Suppl. Ser. 223, 18 (2016), doi: 10.3847/ 0067-0049/223/1/18
  • Z. Meisel, Consistent modeling of GS 1826-24 x-ray bursts for multiple accretion rates demonstrates the possibility of constraining rp-process reaction rates, The Astrophysical Journal 860(2), 147 (2018), doi: 10.3847/1538-4357/aac3d3
  • H. Schatz et al., rp-process nucleosynthesis at extreme temperature and density conditions, Physics Reports 294(4), 167–263 (1998), doi: 10.1016/S0370-1573(97)00048-3