Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 42 min ago
PreprintCC BY 4.0arXiv

Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain

Abstract

Nucleosynthesis simulations of the r-process require neutron capture rates for neutron-rich nuclei, many of which lie beyond experimental reach. Predicting these rates relies on theoretical calculations of the low-energy electric dipole (E1) strength near the neutron threshold. We present the first ab initio computation of the E1 strength along the nickel isotopic chain, for 58Ni and the even-even isotopes 68−80Ni. The E1 strength is obtained with the Lorentz integral transform coupled-cluster (LIT-CC) method, extended to axially symmetric reference states to reach open-shell nuclei, using two- and three-nucleon interactions from chiral effective field theory. The approach is benchmarked against the measured photoabsorption cross section of 58Ni and the E1 strength of 68Ni. Along the chain we find low-lying E1 strength above the neutron threshold that grows with neutron number. Including it in the reaction code TALYS enhances the neutron capture rates forming 68−78Ni between 3 and 10 GK, with an effect that increases with temperature and neutron number and an uncertainty dominated by the inversion of the integral transform. For 80Ni, where strong pygmy dipole strength lies just above threshold, the enhancement sets in already around 0.5 GK. Together, these results open the way to ab initio input for neutron capture rates along isotopic chains far from stability.

Related

  1. Bayesian inference of neutron star crust properties using an ab initio-benchmarked meta-model
    S Burrello, F Gulminelli, M Antonelli +2
    Physical Review CPeer-reviewedCC BY 4.0Full text7 citedGeneral astronomyNuclear physicsHAL
  2. Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates
    Suprovo Ghosh, Alexander Haber, Nils Andersson +1
    arXivPreprintCC BY-NC-SA 4.0Full textHigh-energy astrophysicsGravitation & general relativityarXiv
  3. Impact of Eccentricity on the Population Properties of Neutron Star–Black Hole Mergers
    Gonzalo Morras, Geraint Pratten, Patricia Schmidt
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textHigh-energy astrophysicsCrossref
  4. Impact of neutron captures on the r-process: I. Propagation of statistical model uncertainties
    Yu An, Jan Kuske, Almudena Arcones
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsNuclear physicsarXiv
  5. The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation
    John Ming Ngo, Charlee Amason, Sharon M. Morsink
    arXivPreprintCC BY-SA 4.0Full textHigh-energy astrophysicsarXiv
BibTeX
@misc{bonaiti2026impact,
  title = {{Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain}},
  author = {Francesca Bonaiti and Joanna E. Sobczyk},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.13868},
  eprint = {2610.13868},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.13868},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Impact of ab initio E1 strength on neutron capture rates along the nickel isotopic chain
AU  - Francesca Bonaiti
AU  - Joanna E. Sobczyk
PY  - 2026
DA  - 2026/10/09
PB  - arXiv
DO  - 10.48550/arxiv.2610.13868
UR  - https://arxiv.org/abs/2610.13868
AB  - Nucleosynthesis simulations of the r-process require neutron capture rates for neutron-rich nuclei, many of which lie beyond experimental reach. Predicting these rates relies on theoretical calculations of the low-energy electric dipole (E1) strength near the neutron threshold. We present the first ab initio computation of the E1 strength along the nickel isotopic chain, for ^58Ni and the even-even isotopes ^68−80Ni. The E1 strength is obtained with the Lorentz integral transform coupled-cluster (LIT-CC) method, extended to axially symmetric reference states to reach open-shell nuclei, using two- and three-nucleon interactions from chiral effective field theory. The approach is benchmarked against the measured photoabsorption cross section of ^58Ni and the E1 strength of ^68Ni. Along the chain we find low-lying E1 strength above the neutron threshold that grows with neutron number. Including it in the reaction code TALYS enhances the neutron capture rates forming ^68−78Ni between 3 and 10 GK, with an effect that increases with temperature and neutron number and an uncertainty dominated by the inversion of the integral transform. For ^80Ni, where strong pygmy dipole strength lies just above threshold, the enhancement sets in already around 0.5 GK. Together, these results open the way to ab initio input for neutron capture rates along isotopic chains far from stability.
ER  -