ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case

The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirr...
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Autor*in:	D’Agata G. [verfasserIn] Kilic A. I. [verfasserIn] Burjan V. [verfasserIn] Mrázek J. [verfasserIn] Glagolev V. [verfasserIn] Kroha V. [verfasserIn] Cassisa A. [verfasserIn] Guardo G. L. [verfasserIn] La Cognata M. [verfasserIn] Lamia L. [verfasserIn] Palmerini S. [verfasserIn] Pizzone R. G. [verfasserIn] Rapisarda G. G. [verfasserIn] Romano S. [verfasserIn] Sergi M. L. [verfasserIn] Spartà R. [verfasserIn] Spitaleri C. [verfasserIn] Tumino A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2023

Übergeordnetes Werk:	In: EPJ Web of Conferences - EDP Sciences, 2010, 279, p 02002(2023)
Übergeordnetes Werk:	volume:279, p 02002 ; year:2023

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1051/epjconf/202327902002

Katalog-ID:	DOAJ089069935

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allfields	10.1051/epjconf/202327902002 doi (DE-627)DOAJ089069935 (DE-599)DOAJ8b7cb998a19549f99ecc970c1664481d DE-627 ger DE-627 rakwb eng QC1-999 D’Agata G. verfasserin aut ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed. Physics Kilic A. I. verfasserin aut Burjan V. verfasserin aut Mrázek J. verfasserin aut Glagolev V. verfasserin aut Kroha V. verfasserin aut Cassisa A. verfasserin aut Guardo G. L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Palmerini S. verfasserin aut Pizzone R. G. verfasserin aut Rapisarda G. G. verfasserin aut Romano S. verfasserin aut Sergi M. L. verfasserin aut Spartà R. verfasserin aut Spitaleri C. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 279, p 02002(2023) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:279, p 02002 year:2023 https://doi.org/10.1051/epjconf/202327902002 kostenfrei https://doaj.org/article/8b7cb998a19549f99ecc970c1664481d kostenfrei https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_02002.pdf kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 279, p 02002 2023
spelling	10.1051/epjconf/202327902002 doi (DE-627)DOAJ089069935 (DE-599)DOAJ8b7cb998a19549f99ecc970c1664481d DE-627 ger DE-627 rakwb eng QC1-999 D’Agata G. verfasserin aut ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed. Physics Kilic A. I. verfasserin aut Burjan V. verfasserin aut Mrázek J. verfasserin aut Glagolev V. verfasserin aut Kroha V. verfasserin aut Cassisa A. verfasserin aut Guardo G. L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Palmerini S. verfasserin aut Pizzone R. G. verfasserin aut Rapisarda G. G. verfasserin aut Romano S. verfasserin aut Sergi M. L. verfasserin aut Spartà R. verfasserin aut Spitaleri C. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 279, p 02002(2023) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:279, p 02002 year:2023 https://doi.org/10.1051/epjconf/202327902002 kostenfrei https://doaj.org/article/8b7cb998a19549f99ecc970c1664481d kostenfrei https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_02002.pdf kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 279, p 02002 2023
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allfieldsGer	10.1051/epjconf/202327902002 doi (DE-627)DOAJ089069935 (DE-599)DOAJ8b7cb998a19549f99ecc970c1664481d DE-627 ger DE-627 rakwb eng QC1-999 D’Agata G. verfasserin aut ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed. Physics Kilic A. I. verfasserin aut Burjan V. verfasserin aut Mrázek J. verfasserin aut Glagolev V. verfasserin aut Kroha V. verfasserin aut Cassisa A. verfasserin aut Guardo G. L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Palmerini S. verfasserin aut Pizzone R. G. verfasserin aut Rapisarda G. G. verfasserin aut Romano S. verfasserin aut Sergi M. L. verfasserin aut Spartà R. verfasserin aut Spitaleri C. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 279, p 02002(2023) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:279, p 02002 year:2023 https://doi.org/10.1051/epjconf/202327902002 kostenfrei https://doaj.org/article/8b7cb998a19549f99ecc970c1664481d kostenfrei https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_02002.pdf kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 279, p 02002 2023
allfieldsSound	10.1051/epjconf/202327902002 doi (DE-627)DOAJ089069935 (DE-599)DOAJ8b7cb998a19549f99ecc970c1664481d DE-627 ger DE-627 rakwb eng QC1-999 D’Agata G. verfasserin aut ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case 2023 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed. Physics Kilic A. I. verfasserin aut Burjan V. verfasserin aut Mrázek J. verfasserin aut Glagolev V. verfasserin aut Kroha V. verfasserin aut Cassisa A. verfasserin aut Guardo G. L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Palmerini S. verfasserin aut Pizzone R. G. verfasserin aut Rapisarda G. G. verfasserin aut Romano S. verfasserin aut Sergi M. L. verfasserin aut Spartà R. verfasserin aut Spitaleri C. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 279, p 02002(2023) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:279, p 02002 year:2023 https://doi.org/10.1051/epjconf/202327902002 kostenfrei https://doaj.org/article/8b7cb998a19549f99ecc970c1664481d kostenfrei https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_02002.pdf kostenfrei https://doaj.org/toc/2100-014X Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_206 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2005 GBV_ILN_2009 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2055 GBV_ILN_2111 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 279, p 02002 2023
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callnumber-first	Q - Science
author	D’Agata G.
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topic_title	QC1-999 ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case
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title	ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case
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title_full	ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case
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author_browse	D’Agata G. Kilic A. I. Burjan V. Mrázek J. Glagolev V. Kroha V. Cassisa A. Guardo G. L. La Cognata M. Lamia L. Palmerini S. Pizzone R. G. Rapisarda G. G. Romano S. Sergi M. L. Spartà R. Spitaleri C. Tumino A.
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title_sort	anc experiments for nuclear astrophysics: the 26si(p, γ)27p case
callnumber	QC1-999
title_auth	ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case
abstract	The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed.
abstractGer	The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed.
abstract_unstemmed	The Asymptotic Normalization Coefficient (ANC) method has proven to be useful in retrieving the direct part of the radiative capture cross section for a number of reactions of astrophysical interest. In this work, the study of the 26Si(p, γ)27P reaction, studied via the ANC in its extension for mirror nuclei will be discussed.
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title_short	ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case
url	https://doi.org/10.1051/epjconf/202327902002 https://doaj.org/article/8b7cb998a19549f99ecc970c1664481d https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_02002.pdf https://doaj.org/toc/2100-014X
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author2	Kilic A. I. Burjan V. Mrázek J. Glagolev V. Kroha V. Cassisa A. Guardo G. L. La Cognata M. Lamia L. Palmerini S. Pizzone R. G. Rapisarda G. G. Romano S. Sergi M. L. Spartà R. Spitaleri C. Tumino A.
author2Str	Kilic A. I. Burjan V. Mrázek J. Glagolev V. Kroha V. Cassisa A. Guardo G. L. La Cognata M. Lamia L. Palmerini S. Pizzone R. G. Rapisarda G. G. Romano S. Sergi M. L. Spartà R. Spitaleri C. Tumino A.
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up_date	2024-07-03T21:05:16.071Z
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ANC experiments for nuclear astrophysics: The 26Si(p, γ)27P case

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