Accessing High Pressure States Relevant to Core Conditions in the Giant Planets

Details Accessing High Pressure States Relevant to Core Conditions in the Giant Planets Accessing High Pressure States Relevant to Core Conditions in the Giant Planets

Jul 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.298..235r&link_type=abstract

Astrophysics and Space Science, Volume 298, Issue 1-2, pp. 235-240

Astronomy and Astrophysics

Astrophysics

4

Laboratory Astrophysics, Giant Planets, Planetary Core Conditions, Isentropic Compression, National Ignition Facility

Scientific paper

We have designed an experimental technique to use on the National Ignition Facility (NIF) laser to achieve very high pressure (P max > 10 Mbar = 1000 GPa), dense states of matter at moderate temperatures (T < 0.5 eV = 6000 K), relevant to the core conditions of the giant planets. A discussion of the conditions in the interiors of the giant planets is given, and an experimental design that can approach those conditions is described.

Affiliated with

Also associated with

No associations

Rating

Accessing High Pressure States Relevant to Core Conditions in the Giant Planets 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 Accessing High Pressure States Relevant to Core Conditions in the Giant Planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accessing High Pressure States Relevant to Core Conditions in the Giant Planets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1433505