Ultradense hydrogen in astrophysics, high-pressure metal physics and fusion studies

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, Hydrostatic Stellar Nucleosynthesis, Metal-Insulator Transitions And Other Electronic Transitions, Atomic Processes And Interactions

Scientific paper

Phase diagrams of hydrogen are constructed through first-principles calculations of the equations of state for metallic and insulator phases. On the bases of these theories of the equations of state and the electric resistivity, it is shown that the results of recent shock-metallization experiments can be consistently interpreted in terms of first-order metal-insulator transitions, involving discontinuous changes in density, entropy and enthalpy. The first-order transitions then predict a discontinuous distribution of density and resistivity near the Jovian surface, with a large magnetic Reynolds number enough to sustain prominent magnetic activities. A phase diagram for freezing and ferromagnetic transitions provides a basic account of strong magnetization observed in magnetic white dwarfs. Feasibility of a novel scheme of fusion studies in ultradense metallic hydrogen is examined in light of these experimental and theoretical developments.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Ultradense hydrogen in astrophysics, high-pressure metal physics and fusion studies 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 Ultradense hydrogen in astrophysics, high-pressure metal physics and fusion studies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ultradense hydrogen in astrophysics, high-pressure metal physics and fusion studies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1222801

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.