Effect of Photon Vortex Generated in Extremely Strong Magnetic Fields on Stellar Nucleosynthesis
Abstract It is thought that photon vortices are predominantly produced in extremely strong magnetic fields in the Universe. Because the photon vortex may cause significant large angular momentum transfer in interactions with atomic nuclei, stellar nucleosynthesis in such astrophysical environments is affected. In the present study, we calculate the ratios of the photon absorption transition probabilities of photon vortices with Bessel wave to photons described by the plane wave. The result shows enhancement of excitation of states with large total angular momentum by optimization of the divergence angle of the incident photon vortex in momentum space. However, the average cross section for the photon vortex turns out to be identical with that for the plane wave. Therefore, even when Bessel photons are predominantly produced in astrophysical environments, the isotopic abundances of the synthesized elements are not changed.
Authors
- Tomoyuki Maruyama (ORCID: https://orcid.org/0000-0002-6691-998X)
- Toshitaka Kajino (ORCID: https://orcid.org/0000-0003-1856-4173)
- Myung-Ki Cheoun (ORCID: https://orcid.org/0000-0001-7810-5134)
- Takehito Hayakawa (ORCID: https://orcid.org/0000-0001-5286-8395)
Institutions
- Nihon University (JP)
- Soongsil University (KR)
- National Institutes for Quantum Science and Technology (JP)
- National Astronomical Observatory of Japan (JP)
- Tokyo Metropolitan University (JP)
- The University of Tokyo (JP)
- Beihang University (CN)
- The University of Osaka (JP)
Publication Details
- Journal
- The Astrophysical Journal
- Published
- 2024-10-24
- DOI
- https://doi.org/10.3847/1538-4357/ad77a4
- Citations
- 2
- Primary Topic
- Stellar, planetary, and galactic studies
- Type
- article
- Field-Weighted Citation Impact
- 0.66
Funders
- National Research Foundation
- National Natural Science Foundation of China
- National Research Foundation of Korea
- Japan Society for the Promotion of Science
- National Key Research and Development Program of China
- National Natural Science Foundation of China-Guangdong Joint Fund