Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective

Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separato...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Jenkins, D. G. [verfasserIn] Lister, C. J. Janssens, R. V. F. Khoo, T. L. Moore, E. F. Rehm, K. E. Seweryniak, D. Wuosmaa, A. H. Davinson, T. Woods, P. J. Jokinen, A. Penttila, H. Martınez-Pinedo, G. Jose, J.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2006

Anmerkung:	© Società Italiana di Fisica and Springer-Verlag 2006

Übergeordnetes Werk:	Enthalten in: The European physical journal / A - Società Italiana di Fisica, 1998, 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121
Übergeordnetes Werk:	volume:27 ; year:2006 ; number:Suppl 1 ; day:24 ; month:02 ; pages:117-121

Links:	Volltext

DOI / URN:	10.1140/epja/i2006-08-016-7

Katalog-ID:	OLC2051744262

Internformat


LEADER	01000caa a22002652 4500
001	OLC2051744262
003	DE-627
005	20230502161855.0
007	tu
008	200819s2006 xx \|\|\|\|\| 00\| \|\|eng c
024	7		\|a 10.1140/epja/i2006-08-016-7 \|2 doi
035			\|a (DE-627)OLC2051744262
035			\|a (DE-He213)i2006-08-016-7-p
040			\|a DE-627 \|b ger \|c DE-627 \|e rakwb
041			\|a eng
082	0	4	\|a 530 \|q VZ
082	0	4	\|a 530 \|q VZ
100	1		\|a Jenkins, D. G. \|e verfasserin \|4 aut
245	1	0	\|a Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
264		1	\|c 2006
336			\|a Text \|b txt \|2 rdacontent
337			\|a ohne Hilfsmittel zu benutzen \|b n \|2 rdamedia
338			\|a Band \|b nc \|2 rdacarrier
500			\|a © Società Italiana di Fisica and Springer-Verlag 2006
520			\|a Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented.
700	1		\|a Lister, C. J. \|4 aut
700	1		\|a Janssens, R. V. F. \|4 aut
700	1		\|a Khoo, T. L. \|4 aut
700	1		\|a Moore, E. F. \|4 aut
700	1		\|a Rehm, K. E. \|4 aut
700	1		\|a Seweryniak, D. \|4 aut
700	1		\|a Wuosmaa, A. H. \|4 aut
700	1		\|a Davinson, T. \|4 aut
700	1		\|a Woods, P. J. \|4 aut
700	1		\|a Jokinen, A. \|4 aut
700	1		\|a Penttila, H. \|4 aut
700	1		\|a Martınez-Pinedo, G. \|4 aut
700	1		\|a Jose, J. \|4 aut
773	0	8	\|i Enthalten in \|t The European physical journal / A \|d Società Italiana di Fisica, 1998 \|g 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 \|w (DE-627)239430387 \|w (DE-600)1413603-X \|w (DE-576)064448398 \|x 1434-6001 \|7 nnns
773	1	8	\|g volume:27 \|g year:2006 \|g number:Suppl 1 \|g day:24 \|g month:02 \|g pages:117-121
856	4	1	\|u https://doi.org/10.1140/epja/i2006-08-016-7 \|z lizenzpflichtig \|3 Volltext
912			\|a GBV_USEFLAG_A
912			\|a SYSFLAG_A
912			\|a GBV_OLC
912			\|a SSG-OLC-PHY
912			\|a GBV_ILN_11
912			\|a GBV_ILN_20
912			\|a GBV_ILN_22
912			\|a GBV_ILN_30
912			\|a GBV_ILN_40
912			\|a GBV_ILN_62
912			\|a GBV_ILN_70
912			\|a GBV_ILN_105
912			\|a GBV_ILN_267
912			\|a GBV_ILN_2002
912			\|a GBV_ILN_2003
912			\|a GBV_ILN_2006
912			\|a GBV_ILN_2018
912			\|a GBV_ILN_4029
912			\|a GBV_ILN_4082
912			\|a GBV_ILN_4116
912			\|a GBV_ILN_4277
912			\|a GBV_ILN_4307
951			\|a AR
952			\|d 27 \|j 2006 \|e Suppl 1 \|b 24 \|c 02 \|h 117-121

Indexfelder

author_variant	d g j dg dgj c j l cj cjl r v f j rvf rvfj t l k tl tlk e f m ef efm k e r ke ker d s ds a h w ah ahw t d td p j w pj pjw a j aj h p hp g m p gmp j j jj
matchkey_str	article:14346001:2006----::evlaigecinaerlvntnvncesnhssrmnc
hierarchy_sort_str	2006
publishDate	2006
allfields	10.1140/epja/i2006-08-016-7 doi (DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Jenkins, D. G. verfasserin aut Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2006 Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. Lister, C. J. aut Janssens, R. V. F. aut Khoo, T. L. aut Moore, E. F. aut Rehm, K. E. aut Seweryniak, D. aut Wuosmaa, A. H. aut Davinson, T. aut Woods, P. J. aut Jokinen, A. aut Penttila, H. aut Martınez-Pinedo, G. aut Jose, J. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121 https://doi.org/10.1140/epja/i2006-08-016-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 27 2006 Suppl 1 24 02 117-121
spelling	10.1140/epja/i2006-08-016-7 doi (DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Jenkins, D. G. verfasserin aut Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2006 Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. Lister, C. J. aut Janssens, R. V. F. aut Khoo, T. L. aut Moore, E. F. aut Rehm, K. E. aut Seweryniak, D. aut Wuosmaa, A. H. aut Davinson, T. aut Woods, P. J. aut Jokinen, A. aut Penttila, H. aut Martınez-Pinedo, G. aut Jose, J. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121 https://doi.org/10.1140/epja/i2006-08-016-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 27 2006 Suppl 1 24 02 117-121
allfields_unstemmed	10.1140/epja/i2006-08-016-7 doi (DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Jenkins, D. G. verfasserin aut Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2006 Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. Lister, C. J. aut Janssens, R. V. F. aut Khoo, T. L. aut Moore, E. F. aut Rehm, K. E. aut Seweryniak, D. aut Wuosmaa, A. H. aut Davinson, T. aut Woods, P. J. aut Jokinen, A. aut Penttila, H. aut Martınez-Pinedo, G. aut Jose, J. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121 https://doi.org/10.1140/epja/i2006-08-016-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 27 2006 Suppl 1 24 02 117-121
allfieldsGer	10.1140/epja/i2006-08-016-7 doi (DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Jenkins, D. G. verfasserin aut Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2006 Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. Lister, C. J. aut Janssens, R. V. F. aut Khoo, T. L. aut Moore, E. F. aut Rehm, K. E. aut Seweryniak, D. aut Wuosmaa, A. H. aut Davinson, T. aut Woods, P. J. aut Jokinen, A. aut Penttila, H. aut Martınez-Pinedo, G. aut Jose, J. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121 https://doi.org/10.1140/epja/i2006-08-016-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 27 2006 Suppl 1 24 02 117-121
allfieldsSound	10.1140/epja/i2006-08-016-7 doi (DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Jenkins, D. G. verfasserin aut Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Società Italiana di Fisica and Springer-Verlag 2006 Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. Lister, C. J. aut Janssens, R. V. F. aut Khoo, T. L. aut Moore, E. F. aut Rehm, K. E. aut Seweryniak, D. aut Wuosmaa, A. H. aut Davinson, T. aut Woods, P. J. aut Jokinen, A. aut Penttila, H. aut Martınez-Pinedo, G. aut Jose, J. aut Enthalten in The European physical journal / A Società Italiana di Fisica, 1998 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 (DE-627)239430387 (DE-600)1413603-X (DE-576)064448398 1434-6001 nnns volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121 https://doi.org/10.1140/epja/i2006-08-016-7 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307 AR 27 2006 Suppl 1 24 02 117-121
language	English
source	Enthalten in The European physical journal / A 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121
sourceStr	Enthalten in The European physical journal / A 27(2006), Suppl 1 vom: 24. Feb., Seite 117-121 volume:27 year:2006 number:Suppl 1 day:24 month:02 pages:117-121
format_phy_str_mv	Article
institution	findex.gbv.de
dewey-raw	530
isfreeaccess_bool	false
container_title	The European physical journal / A
authorswithroles_txt_mv	Jenkins, D. G. @@aut@@ Lister, C. J. @@aut@@ Janssens, R. V. F. @@aut@@ Khoo, T. L. @@aut@@ Moore, E. F. @@aut@@ Rehm, K. E. @@aut@@ Seweryniak, D. @@aut@@ Wuosmaa, A. H. @@aut@@ Davinson, T. @@aut@@ Woods, P. J. @@aut@@ Jokinen, A. @@aut@@ Penttila, H. @@aut@@ Martınez-Pinedo, G. @@aut@@ Jose, J. @@aut@@
publishDateDaySort_date	2006-02-24T00:00:00Z
hierarchy_top_id	239430387
dewey-sort	3530
id	OLC2051744262
language_de	englisch
fullrecord	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2051744262</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502161855.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2006 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1140/epja/i2006-08-016-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2051744262</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)i2006-08-016-7-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Jenkins, D. G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2006</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Società Italiana di Fisica and Springer-Verlag 2006</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lister, C. J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Janssens, R. V. F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Khoo, T. L.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Moore, E. F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rehm, K. E.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Seweryniak, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wuosmaa, A. H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Davinson, T.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Woods, P. J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jokinen, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Penttila, H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martınez-Pinedo, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jose, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The European physical journal / A</subfield><subfield code="d">Società Italiana di Fisica, 1998</subfield><subfield code="g">27(2006), Suppl 1 vom: 24. Feb., Seite 117-121</subfield><subfield code="w">(DE-627)239430387</subfield><subfield code="w">(DE-600)1413603-X</subfield><subfield code="w">(DE-576)064448398</subfield><subfield code="x">1434-6001</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:27</subfield><subfield code="g">year:2006</subfield><subfield code="g">number:Suppl 1</subfield><subfield code="g">day:24</subfield><subfield code="g">month:02</subfield><subfield code="g">pages:117-121</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1140/epja/i2006-08-016-7</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_30</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_267</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2003</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4029</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4116</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4277</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">27</subfield><subfield code="j">2006</subfield><subfield code="e">Suppl 1</subfield><subfield code="b">24</subfield><subfield code="c">02</subfield><subfield code="h">117-121</subfield></datafield></record></collection>
author	Jenkins, D. G.
spellingShingle	Jenkins, D. G. ddc 530 Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
authorStr	Jenkins, D. G.
ppnlink_with_tag_str_mv	@@773@@(DE-627)239430387
format	Article
dewey-ones	530 - Physics
delete_txt_mv	keep
author_role	aut aut aut aut aut aut aut aut aut aut aut aut aut aut
collection	OLC
remote_str	false
illustrated	Not Illustrated
issn	1434-6001
topic_title	530 VZ Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
topic	ddc 530
topic_unstemmed	ddc 530
topic_browse	ddc 530
format_facet	Aufsätze Gedruckte Aufsätze
format_main_str_mv	Text Zeitschrift/Artikel
carriertype_str_mv	nc
hierarchy_parent_title	The European physical journal / A
hierarchy_parent_id	239430387
dewey-tens	530 - Physics
hierarchy_top_title	The European physical journal / A
isfreeaccess_txt	false
familylinks_str_mv	(DE-627)239430387 (DE-600)1413603-X (DE-576)064448398
title	Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
ctrlnum	(DE-627)OLC2051744262 (DE-He213)i2006-08-016-7-p
title_full	Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
author_sort	Jenkins, D. G.
journal	The European physical journal / A
journalStr	The European physical journal / A
lang_code	eng
isOA_bool	false
dewey-hundreds	500 - Science
recordtype	marc
publishDateSort	2006
contenttype_str_mv	txt
container_start_page	117
author_browse	Jenkins, D. G. Lister, C. J. Janssens, R. V. F. Khoo, T. L. Moore, E. F. Rehm, K. E. Seweryniak, D. Wuosmaa, A. H. Davinson, T. Woods, P. J. Jokinen, A. Penttila, H. Martınez-Pinedo, G. Jose, J.
container_volume	27
class	530 VZ
format_se	Aufsätze
author-letter	Jenkins, D. G.
doi_str_mv	10.1140/epja/i2006-08-016-7
dewey-full	530
title_sort	re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
title_auth	Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
abstract	Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. © Società Italiana di Fisica and Springer-Verlag 2006
abstractGer	Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. © Società Italiana di Fisica and Springer-Verlag 2006
abstract_unstemmed	Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented. © Società Italiana di Fisica and Springer-Verlag 2006
collection_details	GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_62 GBV_ILN_70 GBV_ILN_105 GBV_ILN_267 GBV_ILN_2002 GBV_ILN_2003 GBV_ILN_2006 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4082 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4307
container_issue	Suppl 1
title_short	Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective
url	https://doi.org/10.1140/epja/i2006-08-016-7
remote_bool	false
author2	Lister, C. J. Janssens, R. V. F. Khoo, T. L. Moore, E. F. Rehm, K. E. Seweryniak, D. Wuosmaa, A. H. Davinson, T. Woods, P. J. Jokinen, A. Penttila, H. Martınez-Pinedo, G. Jose, J.
author2Str	Lister, C. J. Janssens, R. V. F. Khoo, T. L. Moore, E. F. Rehm, K. E. Seweryniak, D. Wuosmaa, A. H. Davinson, T. Woods, P. J. Jokinen, A. Penttila, H. Martınez-Pinedo, G. Jose, J.
ppnlink	239430387
mediatype_str_mv	n
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1140/epja/i2006-08-016-7
up_date	2024-07-04T05:11:46.365Z
_version_	1803624022125051904
fullrecord_marcxml	<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2051744262</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230502161855.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2006 xx \|\|\|\|\| 00\| \|\|eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1140/epja/i2006-08-016-7</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2051744262</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)i2006-08-016-7-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Jenkins, D. G.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2006</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Società Italiana di Fisica and Springer-Verlag 2006</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract. Conventionally, reaction rates relevant to nova nucleosynthesis are determined by performing the relevant proton capture reactions directly for stable species, or as has become possible more recently in inverse kinematics using short-lived accelerated radioactive beams with recoil separators. A secondary approach is to compile information on the properties of levels in the Gamow window using transfer reactions. We present a complementary technique where the states of interest are populated in a heavy-ion fusion reaction and their gamma decay studied with a state-of-the-art array of high-purity germanium detectors. The advantages of this approach, including the ability to determine resonance energies with high precision and the possibility of determining spins and parities from gamma-ray angular distributions are discussed. Two specific examples related to the 22Na(p,γ) and 30P(p,γ) reactions are presented.</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Lister, C. J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Janssens, R. V. F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Khoo, T. L.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Moore, E. F.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Rehm, K. E.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Seweryniak, D.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Wuosmaa, A. H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Davinson, T.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Woods, P. J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jokinen, A.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Penttila, H.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Martınez-Pinedo, G.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Jose, J.</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The European physical journal / A</subfield><subfield code="d">Società Italiana di Fisica, 1998</subfield><subfield code="g">27(2006), Suppl 1 vom: 24. Feb., Seite 117-121</subfield><subfield code="w">(DE-627)239430387</subfield><subfield code="w">(DE-600)1413603-X</subfield><subfield code="w">(DE-576)064448398</subfield><subfield code="x">1434-6001</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:27</subfield><subfield code="g">year:2006</subfield><subfield code="g">number:Suppl 1</subfield><subfield code="g">day:24</subfield><subfield code="g">month:02</subfield><subfield code="g">pages:117-121</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">https://doi.org/10.1140/epja/i2006-08-016-7</subfield><subfield code="z">lizenzpflichtig</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_11</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_20</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_22</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_30</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_40</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_62</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_105</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_267</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2002</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2003</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2006</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_2018</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4029</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4082</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4116</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4277</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_4307</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">27</subfield><subfield code="j">2006</subfield><subfield code="e">Suppl 1</subfield><subfield code="b">24</subfield><subfield code="c">02</subfield><subfield code="h">117-121</subfield></datafield></record></collection>
score	7.400401

Nicht das Richtige dabei?

Schreiben Sie uns!

Re-evaluating reaction rates relevant to nova nucleosynthesis from a nuclear structure perspective

Nicht das Richtige dabei?

Zugang & Verfügbarkeit

Vorhandene Bände

Nicht das Richtige dabei?