Towards a parity-dependent level density for astrophysics

D. Mocelj; T. Rauscher; Friedrich-Karl Thielemann; G. Martinez-Pinedo; K. Langanke; L. Pacearescu; A. Fassler

doi:10.1088/0954-3899/31/10/103

Towards a parity-dependent level density for astrophysics

D. Mocelj, T. Rauscher, Friedrich-Karl Thielemann, G. Martinez-Pinedo, K. Langanke, L. Pacearescu, A. Fassler

Research output: Contribution to journal › Article › peer-review

3 Citations (Scopus)

Abstract

Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.

Original language	English
Pages (from-to)	S1927-S1930
Number of pages	4
Journal	Journal of Physics G: Nuclear and Particle Physics
Volume	31
Issue number	10
DOIs	https://doi.org/10.1088/0954-3899/31/10/103
Publication status	Published - Oct 2005
Event	1st International Conference on Nuclear, Structure, Astrophysics and Reactions (NUSTAR 05) - Guildford Duration: 5 Jan 2005 → 8 Jan 2005

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10.1088/0954-3899/31/10/103

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title = "Towards a parity-dependent level density for astrophysics",

abstract = "Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.",

author = "D. Mocelj and T. Rauscher and Friedrich-Karl Thielemann and G. Martinez-Pinedo and K. Langanke and L. Pacearescu and A. Fassler",

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TY - JOUR

T1 - Towards a parity-dependent level density for astrophysics

AU - Mocelj, D.

AU - Rauscher, T.

AU - Thielemann, Friedrich-Karl

AU - Martinez-Pinedo, G.

AU - Langanke, K.

AU - Pacearescu, L.

AU - Fassler, A.

PY - 2005/10

Y1 - 2005/10

N2 - Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.

AB - Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal.

U2 - 10.1088/0954-3899/31/10/103

DO - 10.1088/0954-3899/31/10/103

M3 - Article

SN - 0954-3899

VL - 31

SP - S1927-S1930

JO - Journal of Physics G: Nuclear and Particle Physics

JF - Journal of Physics G: Nuclear and Particle Physics

IS - 10

T2 - 1st International Conference on Nuclear, Structure, Astrophysics and Reactions (NUSTAR 05)

Y2 - 5 January 2005 through 8 January 2005

ER -

Towards a parity-dependent level density for astrophysics

Abstract

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