Transport Properties of Laser Plasma and H-Rich White Dwarf Stars

Details Transport Properties of Laser Plasma and H-Rich White Dwarf Stars Transport Properties of Laser Plasma and H-Rich White Dwarf Stars

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aps..dppbp8093p&link_type=abstract

American Physical Society, 49th Annual Meeting of the Division of Plasma Physics, November 12-16, 2007, abstract #BP8.093

Physics

Plasma Physics

Scientific paper

An extended survey of spectroscopic observations of hydrogen-rich white dwarf stars indicates existence of magnetic fields of 10kG-10MG [1]. High intensity laser interactions with matter generates magnetic fields of several 100s MG [2]. In both laboratory laser plasma as well as astrophysical plasmas, weakly Landau quantization may be present. We consider transport properties of such plasmas following work of Potekhin [3]. With some simplification, estimate of transport coefficients can be made without evaluation of elaborate integration. This research was performed in Laser Plasma Branch, Plasma Physics Division, Naval Research Laboratory and was supported by DOE/NNSA. [1] A. Kawka et. al., ApJ, 654, 499, 2007 [2] S. Eliezer et. al., Phys. Plasmas, 12, 052115, 2005 [3] A. Y. Potekhin, Astron. Astrophys., 346, 345, 1999

Affiliated with

Also associated with

No associations

Rating

Transport Properties of Laser Plasma and H-Rich White Dwarf Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Transport Properties of Laser Plasma and H-Rich White Dwarf Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Transport Properties of Laser Plasma and H-Rich White Dwarf Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1697333