Shell model spin and parity dependent nuclear level densities for nuclear reaction rates

Mihai Horoi

Shell model spin and parity dependent nuclear level densities for nuclear reaction rates

Physics

Research output: Contribution to journal › Conference article › peer-review

Abstract

We present a recently developed strategy [Nucl. Phys. A 785C, 142 (2005), Phys. Rev. C 69, 041307(R) (2004), Phys. Rev. C 67, 054309 (2003)] of calculating the spin and parity dependent shell model level density for application to astrophysics reaction rates. We also present an exact method for removing the spurious contribution to the nuclear level density in shell model spaces that are factorizable in center-of-mass (CoM) and intrinsic components.

Original language	English
Journal	Proceedings of Science
State	Published - 2006
Event	9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 - Geneva, Switzerland Duration: Jun 25 2006 → Jun 30 2006

Cite this

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title = "Shell model spin and parity dependent nuclear level densities for nuclear reaction rates",

abstract = "We present a recently developed strategy [Nucl. Phys. A 785C, 142 (2005), Phys. Rev. C 69, 041307(R) (2004), Phys. Rev. C 67, 054309 (2003)] of calculating the spin and parity dependent shell model level density for application to astrophysics reaction rates. We also present an exact method for removing the spurious contribution to the nuclear level density in shell model spaces that are factorizable in center-of-mass (CoM) and intrinsic components.",

author = "Mihai Horoi",

year = "2006",

language = "English",

journal = "Proceedings of Science",

issn = "1824-8039",

note = "9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 ; Conference date: 25-06-2006 Through 30-06-2006",

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T1 - Shell model spin and parity dependent nuclear level densities for nuclear reaction rates

AU - Horoi, Mihai

PY - 2006

Y1 - 2006

N2 - We present a recently developed strategy [Nucl. Phys. A 785C, 142 (2005), Phys. Rev. C 69, 041307(R) (2004), Phys. Rev. C 67, 054309 (2003)] of calculating the spin and parity dependent shell model level density for application to astrophysics reaction rates. We also present an exact method for removing the spurious contribution to the nuclear level density in shell model spaces that are factorizable in center-of-mass (CoM) and intrinsic components.

AB - We present a recently developed strategy [Nucl. Phys. A 785C, 142 (2005), Phys. Rev. C 69, 041307(R) (2004), Phys. Rev. C 67, 054309 (2003)] of calculating the spin and parity dependent shell model level density for application to astrophysics reaction rates. We also present an exact method for removing the spurious contribution to the nuclear level density in shell model spaces that are factorizable in center-of-mass (CoM) and intrinsic components.

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M3 - Conference article

AN - SCOPUS:84887458274

SN - 1824-8039

JO - Proceedings of Science

JF - Proceedings of Science

T2 - 9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006

Y2 - 25 June 2006 through 30 June 2006

ER -

Shell model spin and parity dependent nuclear level densities for nuclear reaction rates

Abstract

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