Statistical Mechanics of Light Elements at High Pressure. III. Molecular Hydrogen

1973 ◽  
Vol 181 ◽  
pp. 1031 ◽  
Author(s):  
Wayne L. Slattery ◽  
W. B. Hubbard
Keyword(s):  
High Pressure ◽  
Statistical Mechanics ◽  
Molecular Hydrogen ◽  
Light Elements

Statistical mechanics of light elements at high pressure. V Three-dimensional Thomas-Fermi-Dirac theory

1983 ◽  
Vol 272 ◽  
pp. 301 ◽  
Author(s):  
J. J. Macfarlane ◽  
W. B. Hubbard
Keyword(s):  
High Pressure ◽  
Statistical Mechanics ◽  
Three Dimensional ◽  
Light Elements ◽  
Dirac Theory ◽  
Thomas Fermi

Statistical Mechanics of Light Elements at High Pressure. II. Hydrogen and Helium Alloys

1972 ◽  
Vol 176 ◽  
pp. 525 ◽  
Author(s):  
W. B. Hubbard
Keyword(s):  
High Pressure ◽  
Statistical Mechanics ◽  
Light Elements

Statistical mechanics of light elements at high pressure. IV - A model free energy for the metallic phase

1976 ◽  
Vol 205 ◽  
pp. 295 ◽  
Author(s):  
H. E. Dewitt ◽  
W. B. Hubbard
Keyword(s):  
High Pressure ◽  
Free Energy ◽  
Statistical Mechanics ◽  
Metallic Phase ◽  
Light Elements ◽  
Model Free

Effects of high pressure molecular hydrogen in a-Si:H

1985 ◽  
Vol 77-78 ◽  
pp. 201-212 ◽  
Author(s):  
Y.J Chabal ◽  
C.K.N Patel
Keyword(s):  
High Pressure ◽  
Molecular Hydrogen

scholarly journals Cold Molecular Gas as Baryonic Dark Matter

2004 ◽  
Vol 220 ◽  
pp. 241-248 ◽  
Author(s):  
Daniel Pfenniger
Keyword(s):  
High Pressure ◽  
Dark Matter ◽  
Radiation Field ◽  
Molecular Hydrogen ◽  
Solar Neighbourhood ◽  
Molecular Gas ◽  
Stability Problems ◽  
New Variant ◽  
Uv Excitation ◽  
Baryonic Dark Matter

We review the different cold dark gas models that have been proposed in the literature, as well as a new variant which addresses their principal stability problems by taking into account the property of molecular hydrogen to become solid or liquid below 33 K and at sufficiently high pressure. This new physical ingredient provides the possibility to stabilise cold gas globules by a core of condensed molecular hydrogen. Such loosely bound cold globules behave in a galaxy as a collisionless ensemble of matter, and form a reservoir of gas easily liberated through, e.g., UV excitation. the cold condensed cores survive the longest, of order a Gyr in the solar neighbourhood radiation field, and much longer in spiral outer HI disks.

Neutron spectroscopy of fullerite hydrogenated under high pressure; evidence for interstitial molecular hydrogen

1997 ◽  
Vol 9 (13) ◽  
pp. 2831-2838 ◽  
Author(s):  
A I Kolesnikov ◽  
V E Antonov ◽  
I O Bashkin ◽  
G Grosse ◽  
A P Moravsky ◽  
...  
Keyword(s):  
High Pressure ◽  
Molecular Hydrogen ◽  
Neutron Spectroscopy
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