NucleoSynthesis of Galactic 26 Al 25 Al+p Resonances Peter Parker, Yale University

Preview:

DESCRIPTION

NucleoSynthesis of Galactic 26 Al 25 Al+p Resonances Peter Parker, Yale University Catherine Deibel, Rachel Lewis, Anuj Parikh, Christopher Wrede Jac Caggiano, Jason Clark. ORNL - 23 Oct.’06. 26 Al (1809 keV) map of our Galaxy GRO-Comptel. 25 Al Branch Point :. - PowerPoint PPT Presentation

Citation preview

NucleoSynthesis of Galactic 26Al

25Al+p Resonances

Peter Parker, Yale UniversityCatherine Deibel, Rachel Lewis, Anuj Parikh, Christopher Wrede

Jac Caggiano, Jason Clark

ORNL - 23 Oct.’06

26Al (1809 keV) map of our GalaxyGRO-Comptel

24Mg 25Mg Mg*26

25Al26 g.s.Al

26S i

26 mAl

Mg26 g.s.

1.809-

MeV ray

(p,)26Si()26mAl()26MgGS24Mg(p,)25Al

()25Mg(p,)26Al()26*Mg(26MgGS

25Al Branch Point:

25Al(p,)26Si Resonance Searches: 29Si(3He,6He)26Si (Caggiano)

24Mg(3He,n)26Si (Parpottas)

28Si(p,t)26Si (Bardayan)

[ 26Al(3He,t)26Si(p)25Al ] (Yale)

TRIUMF E1071 (C. Deibel)

TRIUMF DRAGON E922 (A. Chen)Direct Measurement:

29Si(3He,6He)27Si (Yale): Caggiano, et al. Phys.Rev.C 65,055801(2002)

24Mg(3He,n)26Si (Ohio Univ.): Parpottas, et al. Phys.Rev.C 70,065805(2004).

28Si(p,t)26Si (ORNL): Bardayan, et al. Phys.Rev.C 74,045804(2006).

28Si(p,t)26Si (ORNL): Bardayan, et al. Phys.Rev.C 74,045804(2006).

25Al(p,)26Si: Parpottas, et al. Phys.Rev.C 73,049907(E) (2006).

26Al Implanted Target: (TRIUMF-ISAC Proposal E1071)

HRMS 41010 26Al/sec at an energy of 51 keV

1017 26Al/cm2 rastered into a 3-mm diameter circle in 4 to 7 days, into a 40 μg/cm2 carbon foil Contamination: About 1 to 10% 26Na(-)26Mg,But no 27Al

With this target, in conjunction with the Yale split-pole spectrograph and the YLSA silicon array,

we project a 26Al(3He,t)26Si*(p)25Al coincidence rate of 1/hour.

500-thick Silicon5 Sectors; 16 strips eachCovering 131°lab166°80-energy and 80-time signals

Yale LampShade Array - YLSA

26Al(3He,t)26Si*(p)25Al E YLSA vs. Focal Plane

0

0.2

0.4

0.6

0.8

1

1.2

1.4

1.6

1.8

2

5.566.577.58

FP excitation energy (MeV)

YLSA

ene

rgy

26Al(3He,t)26Si(p)25Al(g.s.)

26Mg(3He,t)26Al(p)25Mg

26Al(3He,t)26Si(p)25Al*

27Al(3He,t)27Si*(p)26Al

27Al(3He,t)27Si*(p)26Al

Yale – Nuclear Astrophysics Group

Faculty and Post Doc: Peter Parker Jason ClarkCurrent Graduate Students: Christopher Wrede (4th year) Catherine Deibel (5th year)Most Recent PhDs: Anuj Parikh (’06), PostDoc @ Barcelona Rachel Lewis (‘05), PostDoc @ Univ.of York Dale Visser (’03), Microsoft, Seattle Alan Chen (’00), Faculty @ McMaster Dan Bardayan (’99DNP), Wigner Fellow @ ORNL

Recent PostDocs: Jac Caggiano @ Hanford Lab, Richland, WA

Will Bradfield-Smith @ Univ.Western Ontario

Recommended