Sangeeta, A; Ghosh, T.; Maheshwari, B.; Saxena, G.; Agrawal, B. K.
Cite this document
Sangeeta, A., Ghosh, T., Maheshwari, B., Saxena, G. & Agrawal, B. K. (2022). Astrophysical reaction rates with realistic nuclear level densities. Physical Review C, 105. (4). doi: 10.1103/PhysRevC.105.044320
Sangeeta, A, et al. "Astrophysical reaction rates with realistic nuclear level densities." Physical Review C, vol. 105, no. 4, 2022. https://doi.org/10.1103/PhysRevC.105.044320
Sangeeta, A, T. Ghosh, B. Maheshwari, G. Saxena and B. K. Agrawal. "Astrophysical reaction rates with realistic nuclear level densities." Physical Review C 105, no. 4 (2022). https://doi.org/10.1103/PhysRevC.105.044320
Sangeeta, A., et al. (2022) 'Astrophysical reaction rates with realistic nuclear level densities', Physical Review C, 105(4). doi: 10.1103/PhysRevC.105.044320
Sangeeta A, Ghosh T, Maheshwari B, Saxena G, Agrawal BK. Astrophysical reaction rates with realistic nuclear level densities. Physical Review C [Internet]. 2022 [cited 2024 October 05];105(4). doi: 10.1103/PhysRevC.105.044320
A. Sangeeta, T. Ghosh, B. Maheshwari, G. Saxena and B. K. Agrawal, "Astrophysical reaction rates with realistic nuclear level densities", Physical Review C, vol. 105, no. 4, 2022. [Online]. Available at: https://urn.nsk.hr/urn:nbn:hr:217:244322. [Accessed: 05 October 2024]