activity
19922009
most citedDouble Decimation and Sliding Vacua in the Nuclear Many-Body System

83 citations · 548 across the 34 of their papers we have counts for

collaborators

34 papers

nucl-th2009★ 30 cited

Low-momentum NN interactions and all-order summation of ring diagrams of symmetric nuclear matter

L. -W. Siu, J. W. Holt, T. T. S. Kuo +1

We study the equation of state for symmetric nuclear matter using a ring-diagram approach in which the particle-particle hole-hole () ring diagrams within a momentum model sp…

astro-ph2008★ 37 cited

The Case for Hypercritical Accretion in M33 X-7

E. Moreno Mendez, G. E. Brown, C. -H. Lee +1

The spin parameter of the black hole in M33 X-7 has recently been measured to be a*=0.77+-0.05 (Liu et al. 2008). It has been proposed that the spin of the 15.65 M_sun black hole i…

astro-ph2008★ 10 cited

LMC X-3 May Be a Relic of a GRB Similar to Cosmological GRBs

G. E. Brown, C. -H. Lee, E. Moreno Mendez

The present scenario for high-luminosity long gamma-ray bursts is strongly influenced by the paper of Fruchter et al. (2006). Whereas the main contention of this paper that these G…

nucl-th2007★ 66 cited

Shell model description of the 14C dating beta decay with Brown-Rho-scaled NN interactions

J. W. Holt, G. E. Brown, T. T. S. Kuo +2

We present shell model calculations for the beta-decay of the 14C ground state to the 14N ground state, treating the states of the A=14 multiplet as two 0p holes in an 16O core. We…

astro-ph2007★ 20 cited

GRBs and Hypernova Explosions of Some Galactic Sources

G. E. Brown, C. -H. Lee, E. Moreno Mendez

Knowing the Kerr parameters we can make quantitative calculations of the rotational energy of black holes. We show that Nova Sco (GRO J1655 - 40), Il Lupi (4U 1543 - 47), XTE J1550…

astro-ph2006★ 2 cited

Kerr Parameters for Stellar Mass Black Holes and Their Consequences for GRBs and Hypernovae

E. Moreno Mendez, G. E. Brown, C. -H. Lee +1

Recent measurements of the Kerr parameters a* for two black-hole binaries in our Galaxy (Shafee et al. 2006), GRO J1655-40 and 4U 1543-47 of a*=0.65-0.75 and a*=0.75-0.85, respecti…