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Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes
Classical novae are thermonuclear explosions in stellar binary systems, and important sources of 26 Al and 22 Na. While γ rays from the decay of the former radioisotope have been observed throughout the Galaxy, 22 Na remains untraceable. Its half-life (2.6 yr) would allow the observation of its 1.27...
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Published in: | Nature communications 2023-09, Vol.14 (1), p.4536-4536, Article 4536 |
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creator | Fougères, Chloé de Oliveira Santos, François José, Jordi Michelagnoli, Caterina Clément, Emmanuel Kim, Yung Hee Lemasson, Antoine Guimarães, Valdir Barrientos, Diego Bemmerer, Daniel Benzoni, Giovanna Boston, Andrew J. Böttger, Roman Boulay, Florent Bracco, Angela Čeliković, Igor Cederwall, Bo Ciemala, Michał Delafosse, Clément Domingo-Pardo, César Dudouet, Jérémie Eberth, Jürgen Fülöp, Zsolt González, Vicente Gottardo, Andrea Goupil, Johan Hess, Herbert Jungclaus, Andrea Kaşkaş, Ayşe Korichi, Amel Lenzi, Silvia M. Leoni, Silvia Li, Hongjie Ljungvall, Joa Lopez-Martens, Araceli Menegazzo, Roberto Mengoni, Daniele Million, Benedicte Mrázek, Jaromír Napoli, Daniel R. Navin, Alahari Nyberg, Johan Podolyák, Zsolt Pullia, Alberto Quintana, Begoña Ralet, Damien Redon, Nadine Reiter, Peter Rezynkina, Kseniia Saillant, Frédéric Salsac, Marie-Delphine Sánchez-Benítez, Angel M. Sanchis, Enrique Şenyiğit, Menekşe Siciliano, Marco Smirnova, Nadezda A. Sohler, Dorottya Stanoiu, Mihai Theisen, Christophe Valiente-Dobón, Jose J. Ujić, Predrag Zielińska, Magdalena |
description | Classical novae are thermonuclear explosions in stellar binary systems, and important sources of
26
Al and
22
Na. While
γ
rays from the decay of the former radioisotope have been observed throughout the Galaxy,
22
Na remains untraceable. Its half-life (2.6 yr) would allow the observation of its 1.275 MeV
γ
-ray line from a cosmic source. However, the prediction of such an observation requires good knowledge of its nucleosynthesis. The
22
Na(
p
,
γ
)
23
Mg reaction remains the only source of large uncertainty about the amount of
22
Na ejected. Its rate is dominated by a single resonance on the short-lived state at 7785.0(7) keV in
23
Mg. Here, we propose a combined analysis of particle-particle correlations and velocity-difference profiles to measure femtosecond nuclear lifetimes. The application of this method to the study of the
23
Mg states, places strong limits on the amount of
22
Na produced in novae and constrains its detectability with future space-borne observatories.
The authors report a particle-particle correlation and velocity-difference profile method to measure nuclear lifetime. The results obtained for excited states of 23Mg are used to constrain the production of 22Na in the astrophysical novae explosions. |
doi_str_mv | 10.1038/s41467-023-40121-3 |
format | article |
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26
Al and
22
Na. While
γ
rays from the decay of the former radioisotope have been observed throughout the Galaxy,
22
Na remains untraceable. Its half-life (2.6 yr) would allow the observation of its 1.275 MeV
γ
-ray line from a cosmic source. However, the prediction of such an observation requires good knowledge of its nucleosynthesis. The
22
Na(
p
,
γ
)
23
Mg reaction remains the only source of large uncertainty about the amount of
22
Na ejected. Its rate is dominated by a single resonance on the short-lived state at 7785.0(7) keV in
23
Mg. Here, we propose a combined analysis of particle-particle correlations and velocity-difference profiles to measure femtosecond nuclear lifetimes. The application of this method to the study of the
23
Mg states, places strong limits on the amount of
22
Na produced in novae and constrains its detectability with future space-borne observatories.
The authors report a particle-particle correlation and velocity-difference profile method to measure nuclear lifetime. The results obtained for excited states of 23Mg are used to constrain the production of 22Na in the astrophysical novae explosions.</description><identifier>ISSN: 2041-1723</identifier><identifier>EISSN: 2041-1723</identifier><identifier>DOI: 10.1038/s41467-023-40121-3</identifier><identifier>PMID: 37669984</identifier><language>eng</language><publisher>London: Nature Publishing Group UK</publisher><subject>639/766/387/1126 ; 639/766/387/1127 ; ASTRONOMY AND ASTROPHYSICS ; Binary stars ; Charged particles ; Energy ; Explosions ; Humanities and Social Sciences ; Lifetime ; Measurement methods ; multidisciplinary ; Novae ; Nuclear fusion ; NUCLEAR PHYSICS AND RADIATION PHYSICS ; Observatories ; Profile method (forecasting) ; Radioisotopes ; Science ; Science (multidisciplinary) ; Sodium 22 ; Thermonuclear explosions ; Velocity</subject><ispartof>Nature communications, 2023-09, Vol.14 (1), p.4536-4536, Article 4536</ispartof><rights>This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply 2023</rights><rights>This is a U.S. Government work and not under copyright protection in the US; foreign copyright protection may apply 2023. 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Hee</creatorcontrib><creatorcontrib>Lemasson, Antoine</creatorcontrib><creatorcontrib>Guimarães, Valdir</creatorcontrib><creatorcontrib>Barrientos, Diego</creatorcontrib><creatorcontrib>Bemmerer, Daniel</creatorcontrib><creatorcontrib>Benzoni, Giovanna</creatorcontrib><creatorcontrib>Boston, Andrew J.</creatorcontrib><creatorcontrib>Böttger, Roman</creatorcontrib><creatorcontrib>Boulay, Florent</creatorcontrib><creatorcontrib>Bracco, Angela</creatorcontrib><creatorcontrib>Čeliković, Igor</creatorcontrib><creatorcontrib>Cederwall, Bo</creatorcontrib><creatorcontrib>Ciemala, Michał</creatorcontrib><creatorcontrib>Delafosse, Clément</creatorcontrib><creatorcontrib>Domingo-Pardo, César</creatorcontrib><creatorcontrib>Dudouet, Jérémie</creatorcontrib><creatorcontrib>Eberth, Jürgen</creatorcontrib><creatorcontrib>Fülöp, Zsolt</creatorcontrib><creatorcontrib>González, Vicente</creatorcontrib><creatorcontrib>Gottardo, Andrea</creatorcontrib><creatorcontrib>Goupil, Johan</creatorcontrib><creatorcontrib>Hess, Herbert</creatorcontrib><creatorcontrib>Jungclaus, Andrea</creatorcontrib><creatorcontrib>Kaşkaş, Ayşe</creatorcontrib><creatorcontrib>Korichi, Amel</creatorcontrib><creatorcontrib>Lenzi, Silvia M.</creatorcontrib><creatorcontrib>Leoni, Silvia</creatorcontrib><creatorcontrib>Li, Hongjie</creatorcontrib><creatorcontrib>Ljungvall, Joa</creatorcontrib><creatorcontrib>Lopez-Martens, Araceli</creatorcontrib><creatorcontrib>Menegazzo, Roberto</creatorcontrib><creatorcontrib>Mengoni, Daniele</creatorcontrib><creatorcontrib>Million, Benedicte</creatorcontrib><creatorcontrib>Mrázek, Jaromír</creatorcontrib><creatorcontrib>Napoli, Daniel R.</creatorcontrib><creatorcontrib>Navin, Alahari</creatorcontrib><creatorcontrib>Nyberg, Johan</creatorcontrib><creatorcontrib>Podolyák, Zsolt</creatorcontrib><creatorcontrib>Pullia, Alberto</creatorcontrib><creatorcontrib>Quintana, Begoña</creatorcontrib><creatorcontrib>Ralet, Damien</creatorcontrib><creatorcontrib>Redon, Nadine</creatorcontrib><creatorcontrib>Reiter, Peter</creatorcontrib><creatorcontrib>Rezynkina, Kseniia</creatorcontrib><creatorcontrib>Saillant, Frédéric</creatorcontrib><creatorcontrib>Salsac, Marie-Delphine</creatorcontrib><creatorcontrib>Sánchez-Benítez, Angel M.</creatorcontrib><creatorcontrib>Sanchis, Enrique</creatorcontrib><creatorcontrib>Şenyiğit, Menekşe</creatorcontrib><creatorcontrib>Siciliano, Marco</creatorcontrib><creatorcontrib>Smirnova, Nadezda A.</creatorcontrib><creatorcontrib>Sohler, Dorottya</creatorcontrib><creatorcontrib>Stanoiu, Mihai</creatorcontrib><creatorcontrib>Theisen, Christophe</creatorcontrib><creatorcontrib>Valiente-Dobón, Jose J.</creatorcontrib><creatorcontrib>Ujić, Predrag</creatorcontrib><creatorcontrib>Zielińska, Magdalena</creatorcontrib><creatorcontrib>Argonne National Laboratory (ANL), Argonne, IL (United States)</creatorcontrib><title>Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes</title><title>Nature communications</title><addtitle>Nat Commun</addtitle><description>Classical novae are thermonuclear explosions in stellar binary systems, and important sources of
26
Al and
22
Na. While
γ
rays from the decay of the former radioisotope have been observed throughout the Galaxy,
22
Na remains untraceable. Its half-life (2.6 yr) would allow the observation of its 1.275 MeV
γ
-ray line from a cosmic source. However, the prediction of such an observation requires good knowledge of its nucleosynthesis. The
22
Na(
p
,
γ
)
23
Mg reaction remains the only source of large uncertainty about the amount of
22
Na ejected. Its rate is dominated by a single resonance on the short-lived state at 7785.0(7) keV in
23
Mg. Here, we propose a combined analysis of particle-particle correlations and velocity-difference profiles to measure femtosecond nuclear lifetimes. The application of this method to the study of the
23
Mg states, places strong limits on the amount of
22
Na produced in novae and constrains its detectability with future space-borne observatories.
The authors report a particle-particle correlation and velocity-difference profile method to measure nuclear lifetime. The results obtained for excited states of 23Mg are used to constrain the production of 22Na in the astrophysical novae explosions.</description><subject>639/766/387/1126</subject><subject>639/766/387/1127</subject><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Binary stars</subject><subject>Charged particles</subject><subject>Energy</subject><subject>Explosions</subject><subject>Humanities and Social Sciences</subject><subject>Lifetime</subject><subject>Measurement methods</subject><subject>multidisciplinary</subject><subject>Novae</subject><subject>Nuclear fusion</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>Observatories</subject><subject>Profile method (forecasting)</subject><subject>Radioisotopes</subject><subject>Science</subject><subject>Science (multidisciplinary)</subject><subject>Sodium 22</subject><subject>Thermonuclear explosions</subject><subject>Velocity</subject><issn>2041-1723</issn><issn>2041-1723</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>PIMPY</sourceid><sourceid>DOA</sourceid><recordid>eNp9kk1v1DAQhi0EotXSP8DJgguXgL8SxyeEKj4qVXAAzsaxJ7teJXGwnUr99zibqrQc8MWj8eN3xq8HoZeUvKWEt--SoKKRFWG8EoQyWvEn6JwRQSsqGX_6ID5DFykdSVlc0VaI5-iMy6ZRqhXn6Nd3MNEecB8iZuyrwX7CU7gxgNMyzyFmcLi7xWZNwoBHyIfgTvQIJi3RT3vcw5hDAhsmh6fFDkURD76H7EdIL9Cz3gwJLu72Hfr56eOPyy_V9bfPV5cfrisrZJ0ryiTp2tpKXhtqGG-lAtX0kveWCaEIb0xNnSOKQmsUo84yKQ10DYNWOcr5Dl1tui6Yo56jH0281cF4fUqEuNcmZl-60z2FriW1tasdAKzUNQJ6p0yJJWNF6_2mNS_dCM7ClKMZHok-Ppn8Qe_DjaZEtIRKVRRebQohZa-T9RnsoRg0gc2aiYKJukBv7srE8HuBlPXok4VhMBOEJWnWNrQRgpfX79Drf9BjWOJUDD1RhBeQFoptlI0hpQj9fcuU6HVq9DY1ukyNPk2NXo3j26U0r78J8a_0f279AelowjU</recordid><startdate>20230905</startdate><enddate>20230905</enddate><creator>Fougères, Chloé</creator><creator>de Oliveira Santos, François</creator><creator>José, 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Rezynkina, Kseniia ; Saillant, Frédéric ; Salsac, Marie-Delphine ; Sánchez-Benítez, Angel M. ; Sanchis, Enrique ; Şenyiğit, Menekşe ; Siciliano, Marco ; Smirnova, Nadezda A. ; Sohler, Dorottya ; Stanoiu, Mihai ; Theisen, Christophe ; Valiente-Dobón, Jose J. ; Ujić, Predrag ; Zielińska, Magdalena</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c475t-1270b85c735a1a23879e96f73fc2449036a51dd091e8a921dc277aeb62e89d133</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>639/766/387/1126</topic><topic>639/766/387/1127</topic><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>Binary stars</topic><topic>Charged particles</topic><topic>Energy</topic><topic>Explosions</topic><topic>Humanities and Social Sciences</topic><topic>Lifetime</topic><topic>Measurement methods</topic><topic>multidisciplinary</topic><topic>Novae</topic><topic>Nuclear fusion</topic><topic>NUCLEAR PHYSICS AND 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titles)</collection><collection>Directory of Open Access Journals</collection><jtitle>Nature communications</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Fougères, Chloé</au><au>de Oliveira Santos, François</au><au>José, Jordi</au><au>Michelagnoli, Caterina</au><au>Clément, Emmanuel</au><au>Kim, Yung Hee</au><au>Lemasson, Antoine</au><au>Guimarães, Valdir</au><au>Barrientos, Diego</au><au>Bemmerer, Daniel</au><au>Benzoni, Giovanna</au><au>Boston, Andrew J.</au><au>Böttger, Roman</au><au>Boulay, Florent</au><au>Bracco, Angela</au><au>Čeliković, Igor</au><au>Cederwall, Bo</au><au>Ciemala, Michał</au><au>Delafosse, Clément</au><au>Domingo-Pardo, César</au><au>Dudouet, Jérémie</au><au>Eberth, Jürgen</au><au>Fülöp, Zsolt</au><au>González, Vicente</au><au>Gottardo, Andrea</au><au>Goupil, Johan</au><au>Hess, Herbert</au><au>Jungclaus, Andrea</au><au>Kaşkaş, Ayşe</au><au>Korichi, Amel</au><au>Lenzi, Silvia M.</au><au>Leoni, Silvia</au><au>Li, Hongjie</au><au>Ljungvall, Joa</au><au>Lopez-Martens, Araceli</au><au>Menegazzo, Roberto</au><au>Mengoni, Daniele</au><au>Million, Benedicte</au><au>Mrázek, Jaromír</au><au>Napoli, Daniel R.</au><au>Navin, Alahari</au><au>Nyberg, Johan</au><au>Podolyák, Zsolt</au><au>Pullia, Alberto</au><au>Quintana, Begoña</au><au>Ralet, Damien</au><au>Redon, Nadine</au><au>Reiter, Peter</au><au>Rezynkina, Kseniia</au><au>Saillant, Frédéric</au><au>Salsac, Marie-Delphine</au><au>Sánchez-Benítez, Angel M.</au><au>Sanchis, Enrique</au><au>Şenyiğit, Menekşe</au><au>Siciliano, Marco</au><au>Smirnova, Nadezda A.</au><au>Sohler, Dorottya</au><au>Stanoiu, Mihai</au><au>Theisen, Christophe</au><au>Valiente-Dobón, Jose J.</au><au>Ujić, Predrag</au><au>Zielińska, Magdalena</au><aucorp>Argonne National Laboratory (ANL), Argonne, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes</atitle><jtitle>Nature communications</jtitle><stitle>Nat Commun</stitle><date>2023-09-05</date><risdate>2023</risdate><volume>14</volume><issue>1</issue><spage>4536</spage><epage>4536</epage><pages>4536-4536</pages><artnum>4536</artnum><issn>2041-1723</issn><eissn>2041-1723</eissn><abstract>Classical novae are thermonuclear explosions in stellar binary systems, and important sources of
26
Al and
22
Na. While
γ
rays from the decay of the former radioisotope have been observed throughout the Galaxy,
22
Na remains untraceable. Its half-life (2.6 yr) would allow the observation of its 1.275 MeV
γ
-ray line from a cosmic source. However, the prediction of such an observation requires good knowledge of its nucleosynthesis. The
22
Na(
p
,
γ
)
23
Mg reaction remains the only source of large uncertainty about the amount of
22
Na ejected. Its rate is dominated by a single resonance on the short-lived state at 7785.0(7) keV in
23
Mg. Here, we propose a combined analysis of particle-particle correlations and velocity-difference profiles to measure femtosecond nuclear lifetimes. The application of this method to the study of the
23
Mg states, places strong limits on the amount of
22
Na produced in novae and constrains its detectability with future space-borne observatories.
The authors report a particle-particle correlation and velocity-difference profile method to measure nuclear lifetime. The results obtained for excited states of 23Mg are used to constrain the production of 22Na in the astrophysical novae explosions.</abstract><cop>London</cop><pub>Nature Publishing Group UK</pub><pmid>37669984</pmid><doi>10.1038/s41467-023-40121-3</doi><tpages>1</tpages><orcidid>https://orcid.org/0000-0001-5717-2426</orcidid><orcidid>https://orcid.org/0000-0001-9985-6228</orcidid><orcidid>https://orcid.org/0000-0003-3016-8210</orcidid><orcidid>https://orcid.org/0000-0001-6996-7605</orcidid><orcidid>https://orcid.org/0000-0002-7221-058X</orcidid><orcidid>https://orcid.org/0000-0002-5767-0342</orcidid><orcidid>https://orcid.org/0000-0001-6014-2586</orcidid><orcidid>https://orcid.org/0000-0002-9299-6962</orcidid><orcidid>https://orcid.org/0000-0002-9434-8520</orcidid><orcidid>https://orcid.org/0000-0002-6094-9520</orcidid><orcidid>https://orcid.org/0000-0002-4598-0298</orcidid><orcidid>https://orcid.org/0000-0002-7069-4533</orcidid><orcidid>https://orcid.org/0000-0002-9689-9131</orcidid><orcidid>https://orcid.org/0000-0002-6393-747X</orcidid><orcidid>https://orcid.org/0000-0002-9018-6763</orcidid><orcidid>https://orcid.org/0000-0002-9937-2685</orcidid><orcidid>https://orcid.org/0000-0003-3715-0726</orcidid><orcidid>https://orcid.org/0000-0002-8509-1022</orcidid><orcidid>https://orcid.org/0000-0001-8496-1586</orcidid><orcidid>https://orcid.org/0000-0002-0344-0525</orcidid><orcidid>https://orcid.org/0000-0002-3060-5276</orcidid><orcidid>https://orcid.org/0000-0002-4666-8431</orcidid><orcidid>https://orcid.org/0000-0001-5328-720X</orcidid><orcidid>https://orcid.org/0000-0001-7988-9911</orcidid><orcidid>https://orcid.org/0000-0002-3691-0749</orcidid><orcidid>https://orcid.org/0000-0003-0470-8367</orcidid><orcidid>https://orcid.org/0000-0002-2661-6562</orcidid><orcidid>https://orcid.org/0000-0002-9250-135X</orcidid><orcidid>https://orcid.org/0000-0003-1771-2656</orcidid><orcidid>https://orcid.org/0000-0002-0390-5767</orcidid><orcidid>https://orcid.org/0000-0003-4539-5985</orcidid><orcidid>https://orcid.org/0000-0002-2408-4419</orcidid><orcidid>https://orcid.org/0000-0002-9992-9463</orcidid><orcidid>https://orcid.org/0000-0001-9693-2942</orcidid><orcidid>https://orcid.org/0000-0002-5642-4393</orcidid><orcidid>https://orcid.org/0000-0002-1236-4739</orcidid><orcidid>https://orcid.org/0000000160142586</orcidid><orcidid>https://orcid.org/000000027221058X</orcidid><orcidid>https://orcid.org/0000000203905767</orcidid><orcidid>https://orcid.org/0000000246668431</orcidid><orcidid>https://orcid.org/0000000299929463</orcidid><orcidid>https://orcid.org/0000000294348520</orcidid><orcidid>https://orcid.org/0000000292996962</orcidid><orcidid>https://orcid.org/0000000260949520</orcidid><orcidid>https://orcid.org/0000000212364739</orcidid><orcidid>https://orcid.org/0000000299372685</orcidid><orcidid>https://orcid.org/0000000169967605</orcidid><orcidid>https://orcid.org/0000000330168210</orcidid><orcidid>https://orcid.org/0000000157172426</orcidid><orcidid>https://orcid.org/0000000285091022</orcidid><orcidid>https://orcid.org/0000000345395985</orcidid><orcidid>https://orcid.org/0000000257670342</orcidid><orcidid>https://orcid.org/0000000236910749</orcidid><orcidid>https://orcid.org/0000000184961586</orcidid><orcidid>https://orcid.org/0000000199856228</orcidid><orcidid>https://orcid.org/0000000203440525</orcidid><orcidid>https://orcid.org/0000000256424393</orcidid><orcidid>https://orcid.org/000000015328720X</orcidid><orcidid>https://orcid.org/000000029250135X</orcidid><orcidid>https://orcid.org/0000000337150726</orcidid><orcidid>https://orcid.org/0000000196932942</orcidid><orcidid>https://orcid.org/0000000296899131</orcidid><orcidid>https://orcid.org/0000000304708367</orcidid><orcidid>https://orcid.org/0000000230605276</orcidid><orcidid>https://orcid.org/0000000224084419</orcidid><orcidid>https://orcid.org/0000000179889911</orcidid><orcidid>https://orcid.org/0000000270694533</orcidid><orcidid>https://orcid.org/0000000317712656</orcidid><orcidid>https://orcid.org/0000000290186763</orcidid><orcidid>https://orcid.org/000000026393747X</orcidid><orcidid>https://orcid.org/0000000226616562</orcidid><orcidid>https://orcid.org/0000000245980298</orcidid><oa>free_for_read</oa></addata></record> |
fulltext | fulltext |
identifier | ISSN: 2041-1723 |
ispartof | Nature communications, 2023-09, Vol.14 (1), p.4536-4536, Article 4536 |
issn | 2041-1723 2041-1723 |
language | eng |
recordid | cdi_doaj_primary_oai_doaj_org_article_f1eb805cc9184ee2b85a4efd9ae2b722 |
source | Publicly Available Content Database; Nature Journals Online; PubMed Central; Springer Nature - nature.com Journals - Fully Open Access |
subjects | 639/766/387/1126 639/766/387/1127 ASTRONOMY AND ASTROPHYSICS Binary stars Charged particles Energy Explosions Humanities and Social Sciences Lifetime Measurement methods multidisciplinary Novae Nuclear fusion NUCLEAR PHYSICS AND RADIATION PHYSICS Observatories Profile method (forecasting) Radioisotopes Science Science (multidisciplinary) Sodium 22 Thermonuclear explosions Velocity |
title | Search for 22Na in novae supported by a novel method for measuring femtosecond nuclear lifetimes |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-24T12%3A46%3A03IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_doaj_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Search%20for%2022Na%20in%20novae%20supported%20by%20a%20novel%20method%20for%20measuring%20femtosecond%20nuclear%20lifetimes&rft.jtitle=Nature%20communications&rft.au=Foug%C3%A8res,%20Chlo%C3%A9&rft.aucorp=Argonne%20National%20Laboratory%20(ANL),%20Argonne,%20IL%20(United%20States)&rft.date=2023-09-05&rft.volume=14&rft.issue=1&rft.spage=4536&rft.epage=4536&rft.pages=4536-4536&rft.artnum=4536&rft.issn=2041-1723&rft.eissn=2041-1723&rft_id=info:doi/10.1038/s41467-023-40121-3&rft_dat=%3Cproquest_doaj_%3E2861644390%3C/proquest_doaj_%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c475t-1270b85c735a1a23879e96f73fc2449036a51dd091e8a921dc277aeb62e89d133%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_pqid=2861031641&rft_id=info:pmid/37669984&rfr_iscdi=true |