Symposium on "Nuclear Equation of State used in Astrophysics Models"

August 25-26, 2004
Philadelphia, Pennsylvania, USA

Nuclear Astrophysics and the EOS

Wednesday, August 25, 2004

9:00

Introductory Remarks

9:10

From Infinite Matter to Neutron Stars
H.Lenske

9:40

Equation of State of Supernova Matter
M. W. Carmell, M. Prakash, J. M. Lattimer

10:10

Nuclear Equation of State of Compact Stars
F. Weber

10:40

Intermission.

11:00

Compact Binary Mergers: The Influence of the Equation of State
S. Rosswog

11:30

Comparative Study of Equations of State Used for Neutron Star and Supernova Collapse Models
J. R. Stone, J. C. Miller

12:00

Nuclear Physics of X-ray Bursts as Probe of Neutron Stars
H. Schatz

Experimental Characterization of the EOS

2:00

EOS of Neutron-rich Matter and Collisions of Neutron-rich Nuclei
B. Li

2:30

Heavy-ion Reaction Studies and the Nuclear Equation-of-State
S. J. Yennello, D. Shetty, A. Botvina, S. Soisson, L. Chen, C. Ko

3:00

Neutron Stars: The Richest of the Neutron-Rich Nuclei
J. Piekarewicz, C. J. Horowitz

3:50

Symmetry Energy for Excited Nuclei Produced by Multifragmentation
A. Ono

4:20

Nuclear Symmetry Energy
P. Danielewicz

4:50

Probing the EOS of Asymmetric Matter
W. G. Lynch

Nuclear Astrophysics and the EOS - Part 2

Thursday, August 26, 2004

9:00

Level Density Dependence on Excitation Energy, n-p Asymmetry, and Deformation
R. J. Charity and L. G. Sobotka

9:30

Supernovae, Neutron Stars and Dense Matter
C. J. Horowitz

10:00

Hartree-Fock-Bogoliubov Mass Formulas and the Equation of State of Neutron-Star Matter
M. Peterson

10:30

Intermission.

10:50

On-line Tools for Exploring the Nuclear Equation of State in Astrophysics
B. S. Meyer, J. S. Brown, B. Donehew

11:20

Selfconsistent Equation of State for Supernovae and Neutron Stars
W. G. Newton, J. R. Stone

11:50

R. Rutlege

Experimental Characterization of the EOS - Part 2

2:00

EOS Information from Heavy Ion Collisions between 0.1A and 2A GeV
W. Reisdorf

2:30

Multifragmentation and Supernovae phenomena: Is there a connection?
V. E. Viola

3:00

Nuclear Incompressibility from the Isoscalar Giant Dipole Resonance
U. Garg

3:30

Intermission.

4:00

Nuclear Equation of State from Neutron Star Structure
J. M. Lattimer

4:30

Panel Discussion.

5:15

Concluding Remarks





archive.jinaweb.org      Oct. 26, 2004