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Astrophysically Important Reaction Rates For Novae And X-ray Bursts From Proton Breakup At Intermediate Energies

We discuss the use of one-nucleon removal reactions of loosely bound nuclei at intermediate energies as an indirect method in nuclear astrophysics. The breakup reactions are proved to be good spectroscopic tools and can be used to study a large number of loosely bound proton- or neutron-rich nuclei...

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Main Authors: Banu, A., Trache, L., National Institute of Physics and Nuclear Engineering, 'Horia Hulubei', Carstoiu, F., Negoita, F., Rotaru, F., Orr, N. A., Achouri, N. L., Laurent, B., Bonaccorso, A., Catford, W. N., Patterson, N., Thomas, J. S., Chartier, M., Fernandez-Dominguez, B., Paschalis, S., Pietras, B., Freer, M., Gaudefroy, L., Roussel-Chomaz, P., Horoi, M.
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creator Banu, A.
Trache, L.
National Institute of Physics and Nuclear Engineering, 'Horia Hulubei'
Carstoiu, F.
Negoita, F.
Rotaru, F.
Orr, N. A.
Achouri, N. L.
Laurent, B.
Bonaccorso, A.
Catford, W. N.
Patterson, N.
Thomas, J. S.
Chartier, M.
Fernandez-Dominguez, B.
Paschalis, S.
Pietras, B.
Freer, M.
Gaudefroy, L.
Roussel-Chomaz, P.
Horoi, M.
description We discuss the use of one-nucleon removal reactions of loosely bound nuclei at intermediate energies as an indirect method in nuclear astrophysics. The breakup reactions are proved to be good spectroscopic tools and can be used to study a large number of loosely bound proton- or neutron-rich nuclei over a wide range of beam energies. As peripheral processes, they can be used to extract asymptotic normalization coefficients (ANCs) from which non-resonant capture reaction rates of astrophysical interest can be calculated parameter free. In this talk, we present results of a proton-breakup experiment carried out at GANIL (France) with a cocktail beam centered around {sup 23}Al at 50 MeV/nucleon. Momentum distributions of the breakup fragments, inclusive and in coincidence with gamma rays detected by EXOGAM Germanium clover array, were measured in the focal plan of SPEG energy-loss spectrometer. We present in particular the investigations of reaction rates for {sup 22}Mg(p,{gamma}){sup 23}Al and {sup 23}Al(p,{gamma}){sup 24}Si important for novae and X-ray bursts, respectively.
doi_str_mv 10.1063/1.3527219
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A. ; Achouri, N. L. ; Laurent, B. ; Bonaccorso, A. ; Catford, W. N. ; Patterson, N. ; Thomas, J. S. ; Chartier, M. ; Fernandez-Dominguez, B. ; Paschalis, S. ; Pietras, B. ; Freer, M. ; Gaudefroy, L. ; Roussel-Chomaz, P. ; Horoi, M.</creator><creatorcontrib>Banu, A. ; Trache, L. ; National Institute of Physics and Nuclear Engineering, 'Horia Hulubei' ; Carstoiu, F. ; Negoita, F. ; Rotaru, F. ; Orr, N. A. ; Achouri, N. L. ; Laurent, B. ; Bonaccorso, A. ; Catford, W. N. ; Patterson, N. ; Thomas, J. S. ; Chartier, M. ; Fernandez-Dominguez, B. ; Paschalis, S. ; Pietras, B. ; Freer, M. ; Gaudefroy, L. ; Roussel-Chomaz, P. ; Horoi, M.</creatorcontrib><description>We discuss the use of one-nucleon removal reactions of loosely bound nuclei at intermediate energies as an indirect method in nuclear astrophysics. The breakup reactions are proved to be good spectroscopic tools and can be used to study a large number of loosely bound proton- or neutron-rich nuclei over a wide range of beam energies. As peripheral processes, they can be used to extract asymptotic normalization coefficients (ANCs) from which non-resonant capture reaction rates of astrophysical interest can be calculated parameter free. In this talk, we present results of a proton-breakup experiment carried out at GANIL (France) with a cocktail beam centered around {sup 23}Al at 50 MeV/nucleon. Momentum distributions of the breakup fragments, inclusive and in coincidence with gamma rays detected by EXOGAM Germanium clover array, were measured in the focal plan of SPEG energy-loss spectrometer. 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A.</creatorcontrib><creatorcontrib>Achouri, N. L.</creatorcontrib><creatorcontrib>Laurent, B.</creatorcontrib><creatorcontrib>Bonaccorso, A.</creatorcontrib><creatorcontrib>Catford, W. N.</creatorcontrib><creatorcontrib>Patterson, N.</creatorcontrib><creatorcontrib>Thomas, J. S.</creatorcontrib><creatorcontrib>Chartier, M.</creatorcontrib><creatorcontrib>Fernandez-Dominguez, B.</creatorcontrib><creatorcontrib>Paschalis, S.</creatorcontrib><creatorcontrib>Pietras, B.</creatorcontrib><creatorcontrib>Freer, M.</creatorcontrib><creatorcontrib>Gaudefroy, L.</creatorcontrib><creatorcontrib>Roussel-Chomaz, P.</creatorcontrib><creatorcontrib>Horoi, M.</creatorcontrib><title>Astrophysically Important Reaction Rates For Novae And X-ray Bursts From Proton Breakup At Intermediate Energies</title><title>AIP conference proceedings</title><description>We discuss the use of one-nucleon removal reactions of loosely bound nuclei at intermediate energies as an indirect method in nuclear astrophysics. The breakup reactions are proved to be good spectroscopic tools and can be used to study a large number of loosely bound proton- or neutron-rich nuclei over a wide range of beam energies. As peripheral processes, they can be used to extract asymptotic normalization coefficients (ANCs) from which non-resonant capture reaction rates of astrophysical interest can be calculated parameter free. In this talk, we present results of a proton-breakup experiment carried out at GANIL (France) with a cocktail beam centered around {sup 23}Al at 50 MeV/nucleon. Momentum distributions of the breakup fragments, inclusive and in coincidence with gamma rays detected by EXOGAM Germanium clover array, were measured in the focal plan of SPEG energy-loss spectrometer. We present in particular the investigations of reaction rates for {sup 22}Mg(p,{gamma}){sup 23}Al and {sup 23}Al(p,{gamma}){sup 24}Si important for novae and X-ray bursts, respectively.</description><subject>ACCELERATORS</subject><subject>ALKALINE EARTH ISOTOPES</subject><subject>ALUMINIUM 23</subject><subject>ALUMINIUM ISOTOPES</subject><subject>BARYON REACTIONS</subject><subject>BARYONS</subject><subject>BEAMS</subject><subject>BETA DECAY RADIOISOTOPES</subject><subject>BETA-MINUS DECAY RADIOISOTOPES</subject><subject>BETA-PLUS DECAY RADIOISOTOPES</subject><subject>BINARY STARS</subject><subject>BREAKUP REACTIONS</subject><subject>CAPTURE</subject><subject>CHARGED-PARTICLE REACTIONS</subject><subject>COSMIC RADIATION</subject><subject>COSMIC RAY SOURCES</subject><subject>COSMIC X-RAY BURSTS</subject><subject>COSMIC X-RAY SOURCES</subject><subject>CYCLIC ACCELERATORS</subject><subject>CYCLOTRONS</subject><subject>DECAY</subject><subject>ELECTROMAGNETIC RADIATION</subject><subject>ELEMENTARY PARTICLES</subject><subject>ENERGY LEVELS</subject><subject>ENERGY LOSSES</subject><subject>ENERGY RANGE</subject><subject>ERUPTIVE VARIABLE STARS</subject><subject>EVEN-EVEN NUCLEI</subject><subject>EXCITED STATES</subject><subject>FERMIONS</subject><subject>GAMMA DECAY</subject><subject>GAMMA RADIATION</subject><subject>GANIL CYCLOTRON</subject><subject>HADRON REACTIONS</subject><subject>HADRONS</subject><subject>HEAVY ION ACCELERATORS</subject><subject>IONIZING RADIATIONS</subject><subject>ISOCHRONOUS CYCLOTRONS</subject><subject>ISOTOPES</subject><subject>KINETICS</subject><subject>LIGHT NUCLEI</subject><subject>LOSSES</subject><subject>MAGNESIUM 22</subject><subject>MAGNESIUM ISOTOPES</subject><subject>MEASURING INSTRUMENTS</subject><subject>MEV RANGE</subject><subject>MEV RANGE 10-100</subject><subject>MILLISECONDS LIVING RADIOISOTOPES</subject><subject>NEUTRON-RICH ISOTOPES</subject><subject>NOVAE</subject><subject>NUCLEAR DECAY</subject><subject>NUCLEAR PHYSICS AND RADIATION PHYSICS</subject><subject>NUCLEAR REACTIONS</subject><subject>NUCLEI</subject><subject>NUCLEON REACTIONS</subject><subject>NUCLEONS</subject><subject>ODD-EVEN NUCLEI</subject><subject>PRIMARY COSMIC RADIATION</subject><subject>PROTON REACTIONS</subject><subject>PROTONS</subject><subject>RADIATIONS</subject><subject>RADIOISOTOPES</subject><subject>REACTION KINETICS</subject><subject>SECONDS LIVING RADIOISOTOPES</subject><subject>SILICON 24</subject><subject>SILICON ISOTOPES</subject><subject>SPECTROMETERS</subject><subject>STARS</subject><subject>VARIABLE STARS</subject><subject>X RADIATION</subject><issn>0094-243X</issn><issn>1551-7616</issn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2010</creationdate><recordtype>conference_proceeding</recordtype><recordid>eNotj01LAzEYhIMoWKsH_0HA89Z87G42x21ptVBUikJvJZu8a1fbZEneCvvvXdDTHGaeYYaQe85mnJXykc9kIZTg-oJMeFHwTJW8vCQTxnSeiVzurslNSl-MCa1UNSF9nTCG_jCkzprjcaDrUx8iGo90C8ZiFzzdGoREVyHSl_BjgNbe0V0WzUDn55hwtGI40bcYcAzPI5jvc09rpGuPEE_gupGnSw_xs4N0S65ac0xw969T8rFavi-es83r03pRb7LDOB4z63TeFtYpmbe54CAqZ6BtVWNzJaERSlvruFSClZVUDTDNTSkrIQpjxqtaTsnDX29I2O2T7RDswQbvweJe8GLkSiF_AUtkW0Q</recordid><startdate>20100101</startdate><enddate>20100101</enddate><creator>Banu, A.</creator><creator>Trache, L.</creator><creator>National Institute of Physics and Nuclear Engineering, 'Horia Hulubei'</creator><creator>Carstoiu, F.</creator><creator>Negoita, F.</creator><creator>Rotaru, F.</creator><creator>Orr, N. 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S.</au><au>Chartier, M.</au><au>Fernandez-Dominguez, B.</au><au>Paschalis, S.</au><au>Pietras, B.</au><au>Freer, M.</au><au>Gaudefroy, L.</au><au>Roussel-Chomaz, P.</au><au>Horoi, M.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Astrophysically Important Reaction Rates For Novae And X-ray Bursts From Proton Breakup At Intermediate Energies</atitle><btitle>AIP conference proceedings</btitle><date>2010-01-01</date><risdate>2010</risdate><volume>1304</volume><issue>1</issue><issn>0094-243X</issn><eissn>1551-7616</eissn><abstract>We discuss the use of one-nucleon removal reactions of loosely bound nuclei at intermediate energies as an indirect method in nuclear astrophysics. The breakup reactions are proved to be good spectroscopic tools and can be used to study a large number of loosely bound proton- or neutron-rich nuclei over a wide range of beam energies. 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subjects ACCELERATORS
ALKALINE EARTH ISOTOPES
ALUMINIUM 23
ALUMINIUM ISOTOPES
BARYON REACTIONS
BARYONS
BEAMS
BETA DECAY RADIOISOTOPES
BETA-MINUS DECAY RADIOISOTOPES
BETA-PLUS DECAY RADIOISOTOPES
BINARY STARS
BREAKUP REACTIONS
CAPTURE
CHARGED-PARTICLE REACTIONS
COSMIC RADIATION
COSMIC RAY SOURCES
COSMIC X-RAY BURSTS
COSMIC X-RAY SOURCES
CYCLIC ACCELERATORS
CYCLOTRONS
DECAY
ELECTROMAGNETIC RADIATION
ELEMENTARY PARTICLES
ENERGY LEVELS
ENERGY LOSSES
ENERGY RANGE
ERUPTIVE VARIABLE STARS
EVEN-EVEN NUCLEI
EXCITED STATES
FERMIONS
GAMMA DECAY
GAMMA RADIATION
GANIL CYCLOTRON
HADRON REACTIONS
HADRONS
HEAVY ION ACCELERATORS
IONIZING RADIATIONS
ISOCHRONOUS CYCLOTRONS
ISOTOPES
KINETICS
LIGHT NUCLEI
LOSSES
MAGNESIUM 22
MAGNESIUM ISOTOPES
MEASURING INSTRUMENTS
MEV RANGE
MEV RANGE 10-100
MILLISECONDS LIVING RADIOISOTOPES
NEUTRON-RICH ISOTOPES
NOVAE
NUCLEAR DECAY
NUCLEAR PHYSICS AND RADIATION PHYSICS
NUCLEAR REACTIONS
NUCLEI
NUCLEON REACTIONS
NUCLEONS
ODD-EVEN NUCLEI
PRIMARY COSMIC RADIATION
PROTON REACTIONS
PROTONS
RADIATIONS
RADIOISOTOPES
REACTION KINETICS
SECONDS LIVING RADIOISOTOPES
SILICON 24
SILICON ISOTOPES
SPECTROMETERS
STARS
VARIABLE STARS
X RADIATION
title Astrophysically Important Reaction Rates For Novae And X-ray Bursts From Proton Breakup At Intermediate Energies
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