Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling
| Autor(a) principal: | |
|---|---|
| Data de Publicação: | 2022 |
| Outros Autores: | , , , , |
| Tipo de documento: | Artigo |
| Idioma: | eng |
| Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
| Texto Completo: | http://hdl.handle.net/10362/134359 |
Resumo: | R.F.S acknowledges the support from the ChETEC COST Action( CA16117) during his short-term scientific mission at GSI. A.F. Publisher Copyright: © 2022 by the authors. Licensee MDPI, Basel, Switzerland. |
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Structure Calculations in Nd III and U III Relevant for Kilonovae ModellingAtomic dataKilonovaeNeutron starsOpacityOscillator strengthsAtomic and Molecular Physics, and OpticsNuclear and High Energy PhysicsCondensed Matter PhysicsR.F.S acknowledges the support from the ChETEC COST Action( CA16117) during his short-term scientific mission at GSI. A.F. Publisher Copyright: © 2022 by the authors. Licensee MDPI, Basel, Switzerland.The detection of gravitational waves and electromagnetic signals from the neutron star merger GW170817 has provided evidence that these astrophysical events are sites where the r-process nucleosynthesis operates. The electromagnetic signal, commonly known as kilonova, is powered by the radioactive decay of freshly synthesized nuclei. However, its luminosity, colour and spectra depend on the atomic opacities of the produced elements. In particular, opacities of lanthanides and actinides elements, due to their large density of bound–bound transitions, are fundamental. The current work focuses on atomic structure calculations for lanthanide and actinide ions, which are important in kilonovae modelling of ejecta spectra. Calculations for Nd III and U III, two representative rare-earth ions, were achieved. Our aim is to provide valuable insights for future opacity calculations for all heavy elements. We noticed that the opacity of U III is about an order of magnitude greater than the opacity of Nd III due to a higher density of levels in the case of the actinide.DF – Departamento de FísicaLIBPhys-UNLRUNSilva, Ricardo F.Sampaio, Jorge M.Amaro, PedroFlörs, AndreasMartínez-Pinedo, GabrielMarques, José P.2022-03-11T23:23:38Z2022-032022-03-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10362/134359eng2218-2004PURE: 42310426https://doi.org/10.3390/atoms10010018info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-03-11T05:12:51Zoai:run.unl.pt:10362/134359Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:48:05.028380Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse |
| dc.title.none.fl_str_mv |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| title |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| spellingShingle |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling Silva, Ricardo F. Atomic data Kilonovae Neutron stars Opacity Oscillator strengths Atomic and Molecular Physics, and Optics Nuclear and High Energy Physics Condensed Matter Physics |
| title_short |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| title_full |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| title_fullStr |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| title_full_unstemmed |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| title_sort |
Structure Calculations in Nd III and U III Relevant for Kilonovae Modelling |
| author |
Silva, Ricardo F. |
| author_facet |
Silva, Ricardo F. Sampaio, Jorge M. Amaro, Pedro Flörs, Andreas Martínez-Pinedo, Gabriel Marques, José P. |
| author_role |
author |
| author2 |
Sampaio, Jorge M. Amaro, Pedro Flörs, Andreas Martínez-Pinedo, Gabriel Marques, José P. |
| author2_role |
author author author author author |
| dc.contributor.none.fl_str_mv |
DF – Departamento de Física LIBPhys-UNL RUN |
| dc.contributor.author.fl_str_mv |
Silva, Ricardo F. Sampaio, Jorge M. Amaro, Pedro Flörs, Andreas Martínez-Pinedo, Gabriel Marques, José P. |
| dc.subject.por.fl_str_mv |
Atomic data Kilonovae Neutron stars Opacity Oscillator strengths Atomic and Molecular Physics, and Optics Nuclear and High Energy Physics Condensed Matter Physics |
| topic |
Atomic data Kilonovae Neutron stars Opacity Oscillator strengths Atomic and Molecular Physics, and Optics Nuclear and High Energy Physics Condensed Matter Physics |
| description |
R.F.S acknowledges the support from the ChETEC COST Action( CA16117) during his short-term scientific mission at GSI. A.F. Publisher Copyright: © 2022 by the authors. Licensee MDPI, Basel, Switzerland. |
| publishDate |
2022 |
| dc.date.none.fl_str_mv |
2022-03-11T23:23:38Z 2022-03 2022-03-01T00:00:00Z |
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info:eu-repo/semantics/publishedVersion |
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info:eu-repo/semantics/article |
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article |
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publishedVersion |
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http://hdl.handle.net/10362/134359 |
| url |
http://hdl.handle.net/10362/134359 |
| dc.language.iso.fl_str_mv |
eng |
| language |
eng |
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2218-2004 PURE: 42310426 https://doi.org/10.3390/atoms10010018 |
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info:eu-repo/semantics/openAccess |
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openAccess |
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application/pdf |
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reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação instacron:RCAAP |
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Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
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RCAAP |
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Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
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