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Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations
Physical Review C, 105 (2022), 5; 055801. https://doi.org/10.1103/PhysRevC.105.055801

Giraud, S.; Zegers, R. G. T.; Brown, B. A.; Gabler, J.-M.; Lesniak, J.; Rebenstock, J.; Ney, E. M.; Engel, J.; Ravlić, Ante; Paar, Nils

Citirajte ovaj rad

Giraud, S., Zegers, R. G. T., Brown, B. A., Gabler, J. M., Lesniak, J., Rebenstock, J. ... Paar, N. (2022). Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations. Physical Review C, 105. (5). doi: 10.1103/PhysRevC.105.055801

Giraud, S., et al. "Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations." Physical Review C, vol. 105, br. 5, 2022. https://doi.org/10.1103/PhysRevC.105.055801

Giraud, S., R. G. T. Zegers, B. A. Brown, J. M. Gabler, J. Lesniak, J. Rebenstock, E. M. Ney, J. Engel, Ante Ravlić i Nils Paar. "Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations." Physical Review C 105, br. 5 (2022). https://doi.org/10.1103/PhysRevC.105.055801

Giraud, S., et al. (2022) 'Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations', Physical Review C, 105(5). doi: 10.1103/PhysRevC.105.055801

Giraud S, Zegers RGT, Brown BA, Gabler JM, Lesniak J, Rebenstock J, i sur.. Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations. Physical Review C [Internet]. 2022. [pristupljeno 04.10.2024.];105(5). doi: 10.1103/PhysRevC.105.055801

S. Giraud, et al., "Finite-temperature electron-capture rates for neutron-rich nuclei near N=50 and effects on core-collapse supernova simulations", Physical Review C, vol. 105, br. 5, 2022. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:756684. [Citirano: 04.10.2024.]

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