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Grant: Subatomic Physics Envelope - Individual

TRIUMF

$75,000.00

Indirect methods in nuclear astrophysics

FY 2009-10

Summary
This proposal seeks funding for my research program applying indirect methods to experimental nuclear astrophysics. The focus of this research is the experimental determination of the rates of nuclear reactions that occur in stars and astrophysical explosions. These reaction rates must be known in order to understand how energy is released in stars and stellar explosions, and to discover the origins of the chemical elements. Many of the most important reactions involve radioactive nuclei that don't occur naturally on Earth, and therefore must be created in the laboratory in order to be studied. Nuclear reaction rates can be determined directly if a beam of sufficient intensity can be produced, but such intense beams are available for only a tiny fraction of the relevant nuclei. In cases where direct study is presently impossible, indirect methods can be brought to bear. These methods, which involve the determination of the properties of the states of the compound nuclei formed in reactions of astrophysical interest, are quite powerful and often yield sufficient information to determine the nuclear reaction rates needed. One of the tools we intend to exploit at TRIUMF in the future for these studies of nuclear structure relevant to astrophysics is the recently funded ElectroMagnetic Mass Analyser (EMMA), of which I am the principal investigator. EMMA is a recoil mass spectrometer that will be used to separate the recoils of nuclear reactions from the beam used to produce them and to disperse the recoils according to their charge-to-mass ratio. We are currently building EMMA, and anticipate that it will be fully commissioned and ready for first experiments in 2011, at which point we will apply for an EMMA project grant. Until that time, it is essential that I continue to carry out my experimental program. As I am very busy with EMMA, I require a group of students and postdoctoral researchers to help me with this research. I therefore request continued funding for my research in indirect methods in experimental nuclear astrophysics via an individual discovery grant. This would support my ongoing experiments at TRIUMF, including student and postdoc salaries as well as detectors, electronics, and travel to conferences.
Program
Subatomic Physics Envelope - Individual
Recipient
Location
British Columbia, Canada
Recipient Type
Not-for-profit organization or charity
Type
Grant
Source
NSERC's Awards Data

As published

Application id
293193-2009
Name nom
Davids, Barry
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
2009
Competition year année de concours
2009
Award amount
75000
Program id
SAPIN
Program nane en
Subatomic Physics Envelope - Individual
Program name fr
Enveloppe de physique subatomique - Individuelles
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
1202
Area of application group en
Advancement of knowledge
Area of application group fr
Avancement des connaissances
Area of application en
Physical sciences
Area of application fr
Sciences physiques
Research subject code
3102
Research subject group en
Physics
Research subject group fr
Physique
Research subject en
Nuclear physics
Research subject fr
Physique nucléaire
Partie
1
Nb partie
2
Application title
Indirect methods in nuclear astrophysics
Keyword
NA
Application summary
This proposal seeks funding for my research program applying indirect methods to experimental nuclear astrophysics. The focus of this research is the experimental determination of the rates of nuclear reactions that occur in stars and astrophysical explosions. These reaction rates must be known in order to understand how energy is released in stars and stellar explosions, and to discover the origins of the chemical elements. Many of the most important reactions involve radioactive nuclei that don't occur naturally on Earth, and therefore must be created in the laboratory in order to be studied. Nuclear reaction rates can be determined directly if a beam of sufficient intensity can be produced, but such intense beams are available for only a tiny fraction of the relevant nuclei. In cases where direct study is presently impossible, indirect methods can be brought to bear. These methods, which involve the determination of the properties of the states of the compound nuclei formed in reactions of astrophysical interest, are quite powerful and often yield sufficient information to determine the nuclear reaction rates needed. One of the tools we intend to exploit at TRIUMF in the future for these studies of nuclear structure relevant to astrophysics is the recently funded ElectroMagnetic Mass Analyser (EMMA), of which I am the principal investigator. EMMA is a recoil mass spectrometer that will be used to separate the recoils of nuclear reactions from the beam used to produce them and to disperse the recoils according to their charge-to-mass ratio. We are currently building EMMA, and anticipate that it will be fully commissioned and ready for first experiments in 2011, at which point we will apply for an EMMA project grant. Until that time, it is essential that I continue to carry out my experimental program. As I am very busy with EMMA, I require a group of students and postdoctoral researchers to help me with this research. I therefore request continued funding for my research in indirect methods in experimental nuclear astrophysics via an individual discovery grant. This would support my ongoing experiments at TRIUMF, including student and postdoc salaries as well as detectors, electronics, and travel to conferences.