Charles J. Horowitz

Nuclear Theory Center and Department of Physics,

Indiana University, 701 E. Third St., Bloomington, IN 47405

Swain Hall West Room 233 or Indiana University Cyclotron Facility 1215

Phone: 812 855-2959 or 855-0303

Email: horowit at Indiana dot edu   

 

 

Research

I am a theoretical nuclear physicist working on dense nuclear matter in the laboratory and in astrophysics.  Some of my publications are listed on SPIRES

 

Conferences I have co-organized in Nuclear Physics, Astrophysics, and Fundamental Symmetries.

 

Research topics:

The Equation of State (pressure versus density) of dense and or neutron rich nuclear matter.

Supernovae are giant stellar explosions.  I am interested in how supernovae depend on neutrino interactions and the properties of dense matter.

Neutron stars are collapsed stars that are the densest macroscopic objects this side of black holes.

Laboratory measurements of nuclear properties important for astrophysics, such as

Measuring the neutron radius of the heavy nucleus 208Pb via parity violating electron scattering.  This is the Pb Radius Experiment (PREX) at Jefferson lab.  

 Chemistry of neutron stars modeled for first time

A NewScientist Web article by David Shiga highlights our recent paper on phase separation in neutron star crusts.  We find, based on large scale molecular dynamics simulations, that when material falls on a neutron star and freezes, the lighter Z elements tend to remain behind in a liquid ocean.  This chemical separation may change many properties of neutron stars and could explain how carbon is concentrated until it can ignite in a great thermonuclear explosion known as a superburst.  It could also lead to a layered structure for neutron stars with larger bumps that may efficiently radiate gravitational waves.

 

See Astro-ph/0703062 Phase separation in the crust of accreting neutron stars by C. J. Horowitz, D. K. Berry, E. F. Brown, Phys Rev. E in Press.

 

A neutron star that siphons material from a partner has a solid crust of heavy elements topped by an ocean of lighter elements. Occasionally, the ocean erupts in a nuclear explosion (Illustration: Ed Brown, MSU)    

 

Teaching      

 

I organize the Indiana University Physics Journal Club.   Here graduate students make informal presentations on exciting recent papers in any area of physics.

 

In the Fall of 2007 I will teach Classical Mechanics: P521  Click here for information

I will teach in the Spring 2008 P621 Relativisatic Quantum Field Theory
I have also tought in recent years:

P110/ P120, Energy
P111, The Physics of Extraterrestrial Life and Death
P453 Quantum Mechanics
P556, Statistical Physics
P630, Nuclear Astrophysics

 

Some personal information is here