Grant: Subatomic Physics Envelope - Project
TRIUMF
$26,000.00
Nuclear astrophysics with nucleonic ejectiles
FY 2012-13
Summary
There are many reactions in nuclear physics and astrophysics in which heavy particles are emitted after the reaction has occurred. These are of the type (alpha,p) and (p,alpha) for direct stellar reactions. In addition, nuclear transfer reactions like (^6Li,d) and (^3He,d), as well as the measurement of elastic scattering can provide useful nuclear information to derive stellar reaction rates. In all cases, the detection of charged light ejectiles is required. A special case are (alpha,n) reactions where we plan not to detect the neutron but the heavy reaction partner. For all these types of reactions we have two detector facilities available: Tuda and Tactic. Tuda is a sophisticated vacuum chamber that allows the placement of various kinds of silicon detectors. This year has seen infrastructure at ISAC II been set in place that allows Tuda to be moved between ISAC I for low energy experiments and ISAC II for high energy experiments. In the past three years, we also have developed a gas based time projection chamber named Tactic. This chamber has a non beam-sensible zone in the centre and no windows toward the outer detecting zone. Thus heavy ions from reactions that occur in the central region can be detected with high efficiency once they scatter into the detection region. Frequently, the emission of charged particles is followed by the emission of gamma rays. We have employed the Dragon BGO array. However, the existing BGO array has too few detectors to allow coverage of the Tactic detector. We therefore request the acquisition of two LaBr detectors for test purposes. LaBr detectors have very good time resolution, as well as good energy resolution combined with a high efficiency. Among the reactions we plan to measure with Tuda are those concerning the breakout from the hot CNO cycle via 18Ne. An indirect measurement of the 14C(a,g)18O stellar rate is planned (AV canum veneticorum stars). We also will provide some support for groups coming to Tuda from abroad. For Tactic a measurement of 8Li(a,n)11B reaction is planned. Also measurements of the 7(Be(p,p)7Be and 7Li(3He,a)6Li reactions are planned. The latter reaction requires a separation of the beam and the detection zone in Tactic and thus another gas handling system.
Program
Subatomic Physics Envelope - Project
Recipient
Location
British Columbia, Canada
Recipient Type
Not-for-profit organization or charity
Type
Grant
Source
NSERC's Awards Data
As published
Application id
217035-2010
Name nom
Buchmann, Lothar
Department département
Science Division
Organization id
8
Institution établissement
TRIUMF
Province en
British Columbia
Province fr
Colombie-Britannique
Country en
CANADA
Country fr
CANADA
Fiscal year exercice financier
2012
Competition year année de concours
2010
Award amount
26000
Program id
SAPPJ
Program name en
Subatomic Physics Envelope - Project
Program name fr
Enveloppe de physique subatomique - De projet
Group en
Discovery grants programs
Group fr
Programmes de subventions à la découverte
Committee code
19
Committee name en
Subatomic Physics
Committee name fr
Physique subatomique
Area of application code
1200
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Advancement of knowledge
Area of application fr
Avancement des connaissances
Research subject code
3103
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Nuclear reactions and scattering
Research subject fr
Réactions nucléaires et dispersion
Partie
3
Nb partie
3
Application title
Nuclear astrophysics with nucleonic ejectiles
Keyword
NSERC
Application summary
There are many reactions in nuclear physics and astrophysics in which heavy particles are emitted after the reaction has occurred. These are of the type (alpha,p) and (p,alpha) for direct stellar reactions. In addition, nuclear transfer reactions like (^6Li,d) and (^3He,d), as well as the measurement of elastic scattering can provide useful nuclear information to derive stellar reaction rates. In all cases, the detection of charged light ejectiles is required. A special case are (alpha,n) reactions where we plan not to detect the neutron but the heavy reaction partner. For all these types of reactions we have two detector facilities available: Tuda and Tactic. Tuda is a sophisticated vacuum chamber that allows the placement of various kinds of silicon detectors. This year has seen infrastructure at ISAC II been set in place that allows Tuda to be moved between ISAC I for low energy experiments and ISAC II for high energy experiments. In the past three years, we also have developed a gas based time projection chamber named Tactic. This chamber has a non beam-sensible zone in the centre and no windows toward the outer detecting zone. Thus heavy ions from reactions that occur in the central region can be detected with high efficiency once they scatter into the detection region. Frequently, the emission of charged particles is followed by the emission of gamma rays. We have employed the Dragon BGO array. However, the existing BGO array has too few detectors to allow coverage of the Tactic detector. We therefore request the acquisition of two LaBr detectors for test purposes. LaBr detectors have very good time resolution, as well as good energy resolution combined with a high efficiency. Among the reactions we plan to measure with Tuda are those concerning the breakout from the hot CNO cycle via 18Ne. An indirect measurement of the 14C(a,g)18O stellar rate is planned (AV canum veneticorum stars). We also will provide some support for groups coming to Tuda from abroad. For Tactic a measurement of 8Li(a,n)11B reaction is planned. Also measurements of the 7(Be(p,p)7Be and 7Li(3He,a)6Li reactions are planned. The latter reaction requires a separation of the beam and the detection zone in Tactic and thus another gas handling system.