Trojan Horse particle invariance in fusion reactions

Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to ver...
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Autor*in:	Pizzone R.G. [verfasserIn] Spitaleril C. [verfasserIn] Bertulani C. [verfasserIn] Mukhamedzhanov A. [verfasserIn] Blokhintsev L. [verfasserIn] La Cognata M. [verfasserIn] Lamia L. [verfasserIn] Spartá R. [verfasserIn] Tumino A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2015

Übergeordnetes Werk:	In: EPJ Web of Conferences - EDP Sciences, 2010, 86, p 00034(2015)
Übergeordnetes Werk:	volume:86, p 00034 ; year:2015

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.1051/epjconf/20158600034

Katalog-ID:	DOAJ074813013

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allfields	10.1051/epjconf/20158600034 doi (DE-627)DOAJ074813013 (DE-599)DOAJ9caca1877ab54758ac5e7278de6e1132 DE-627 ger DE-627 rakwb eng QC1-999 Pizzone R.G. verfasserin aut Trojan Horse particle invariance in fusion reactions 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details. Physics Spitaleril C. verfasserin aut Bertulani C. verfasserin aut Mukhamedzhanov A. verfasserin aut Blokhintsev L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Spartá R. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 86, p 00034(2015) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:86, p 00034 year:2015 https://doi.org/10.1051/epjconf/20158600034 kostenfrei https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 kostenfrei http://dx.doi.org/10.1051/epjconf/20158600034 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 86, p 00034 2015
spelling	10.1051/epjconf/20158600034 doi (DE-627)DOAJ074813013 (DE-599)DOAJ9caca1877ab54758ac5e7278de6e1132 DE-627 ger DE-627 rakwb eng QC1-999 Pizzone R.G. verfasserin aut Trojan Horse particle invariance in fusion reactions 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details. Physics Spitaleril C. verfasserin aut Bertulani C. verfasserin aut Mukhamedzhanov A. verfasserin aut Blokhintsev L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Spartá R. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 86, p 00034(2015) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:86, p 00034 year:2015 https://doi.org/10.1051/epjconf/20158600034 kostenfrei https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 kostenfrei http://dx.doi.org/10.1051/epjconf/20158600034 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 86, p 00034 2015
allfields_unstemmed	10.1051/epjconf/20158600034 doi (DE-627)DOAJ074813013 (DE-599)DOAJ9caca1877ab54758ac5e7278de6e1132 DE-627 ger DE-627 rakwb eng QC1-999 Pizzone R.G. verfasserin aut Trojan Horse particle invariance in fusion reactions 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details. Physics Spitaleril C. verfasserin aut Bertulani C. verfasserin aut Mukhamedzhanov A. verfasserin aut Blokhintsev L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Spartá R. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 86, p 00034(2015) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:86, p 00034 year:2015 https://doi.org/10.1051/epjconf/20158600034 kostenfrei https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 kostenfrei http://dx.doi.org/10.1051/epjconf/20158600034 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 86, p 00034 2015
allfieldsGer	10.1051/epjconf/20158600034 doi (DE-627)DOAJ074813013 (DE-599)DOAJ9caca1877ab54758ac5e7278de6e1132 DE-627 ger DE-627 rakwb eng QC1-999 Pizzone R.G. verfasserin aut Trojan Horse particle invariance in fusion reactions 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details. Physics Spitaleril C. verfasserin aut Bertulani C. verfasserin aut Mukhamedzhanov A. verfasserin aut Blokhintsev L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Spartá R. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 86, p 00034(2015) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:86, p 00034 year:2015 https://doi.org/10.1051/epjconf/20158600034 kostenfrei https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 kostenfrei http://dx.doi.org/10.1051/epjconf/20158600034 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 86, p 00034 2015
allfieldsSound	10.1051/epjconf/20158600034 doi (DE-627)DOAJ074813013 (DE-599)DOAJ9caca1877ab54758ac5e7278de6e1132 DE-627 ger DE-627 rakwb eng QC1-999 Pizzone R.G. verfasserin aut Trojan Horse particle invariance in fusion reactions 2015 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details. Physics Spitaleril C. verfasserin aut Bertulani C. verfasserin aut Mukhamedzhanov A. verfasserin aut Blokhintsev L. verfasserin aut La Cognata M. verfasserin aut Lamia L. verfasserin aut Spartá R. verfasserin aut Tumino A. verfasserin aut In EPJ Web of Conferences EDP Sciences, 2010 86, p 00034(2015) (DE-627)647306611 (DE-600)2595425-8 2100014X nnns volume:86, p 00034 year:2015 https://doi.org/10.1051/epjconf/20158600034 kostenfrei https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 kostenfrei http://dx.doi.org/10.1051/epjconf/20158600034 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 86, p 00034 2015
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title	Trojan Horse particle invariance in fusion reactions
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title_full	Trojan Horse particle invariance in fusion reactions
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author_browse	Pizzone R.G. Spitaleril C. Bertulani C. Mukhamedzhanov A. Blokhintsev L. La Cognata M. Lamia L. Spartá R. Tumino A.
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title_sort	trojan horse particle invariance in fusion reactions
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title_auth	Trojan Horse particle invariance in fusion reactions
abstract	Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details.
abstractGer	Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details.
abstract_unstemmed	Trojan Horse method plays an important part for the measurement of several charged particle induced reactions cross sections of astrophysical interest. In order to better understand its cornerstones and the related applications to different astrophysical scenarios several tests were performed to verify all its properties and the possible future perspectives. The Trojan Horse nucleus invariance for the binary reactions d(d,p)t, 6,7Li(p,α)3,4He was therefore tested using the appropriate quasi free break- ups, respectively. In the first cases results from 6Li and 3He break up were used, while for the lithium fusion reactions break-ups of 2H and 3He were compared. The astrophysical S(E)-factors for the different processes were then extracted in the framework of the PlaneWave Approximation applied to the different break-up schemes. The obtained results are compared with direct data as well as with previous indirect investigations. The very good agreement between data coming from different break-up schemes confirms the applicability of the plane wave approximation and suggests the independence of binary indirect cross section on the chosen Trojan Horse nucleus also for the present cases. Moreover the astrophysical implications of the results will also be discussed in details.
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title_short	Trojan Horse particle invariance in fusion reactions
url	https://doi.org/10.1051/epjconf/20158600034 https://doaj.org/article/9caca1877ab54758ac5e7278de6e1132 http://dx.doi.org/10.1051/epjconf/20158600034 https://doaj.org/toc/2100-014X
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