Properties of dense fluid hydrogen and helium and implications for giant gas planets

J. Vorberger; I. Tamblyn; S. A. Bonev; B. Militzer; W. B. Hubbard

Properties of dense fluid hydrogen and helium and implications for giant gas planets

J. Vorberger, I. Tamblyn, S. A. Bonev, B. Militzer, W. B. Hubbard

Lunar and Planetary Lab

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Original language	English (US)
Title of host publication	34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts
Pages	219-222
Number of pages	4
Edition	1
State	Published - 2007
Event	34th European Physical Society Conference on Plasma Physics 2007, EPS 2007 - Warsaw, Poland Duration: Jul 2 2007 → Jul 6 2007

Publication series

Name	34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts
Number	1
Volume	31

Other

Other	34th European Physical Society Conference on Plasma Physics 2007, EPS 2007
Country/Territory	Poland
City	Warsaw
Period	7/2/07 → 7/6/07

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics

Cite this

Vorberger, J., Tamblyn, I., Bonev, S. A., Militzer, B., & Hubbard, W. B. (2007). Properties of dense fluid hydrogen and helium and implications for giant gas planets. In 34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts (1 ed., pp. 219-222). (34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts; Vol. 31, No. 1).

Properties of dense fluid hydrogen and helium and implications for giant gas planets. / Vorberger, J.; Tamblyn, I.; Bonev, S. A. et al.
34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts. 1. ed. 2007. p. 219-222 (34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts; Vol. 31, No. 1).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Vorberger, J, Tamblyn, I, Bonev, SA, Militzer, B & Hubbard, WB 2007, Properties of dense fluid hydrogen and helium and implications for giant gas planets. in 34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts. 1 edn, 34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts, no. 1, vol. 31, pp. 219-222, 34th European Physical Society Conference on Plasma Physics 2007, EPS 2007, Warsaw, Poland, 7/2/07.

@inproceedings{8059eb1af2a443edad8309cb6364ab88,

title = "Properties of dense fluid hydrogen and helium and implications for giant gas planets",

author = "J. Vorberger and I. Tamblyn and Bonev, {S. A.} and B. Militzer and Hubbard, {W. B.}",

year = "2007",

language = "English (US)",

isbn = "9781622763344",

series = "34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts",

number = "1",

pages = "219--222",

booktitle = "34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts",

edition = "1",

note = "34th European Physical Society Conference on Plasma Physics 2007, EPS 2007 ; Conference date: 02-07-2007 Through 06-07-2007",

}

TY - GEN

T1 - Properties of dense fluid hydrogen and helium and implications for giant gas planets

AU - Vorberger, J.

AU - Tamblyn, I.

AU - Bonev, S. A.

AU - Militzer, B.

AU - Hubbard, W. B.

PY - 2007

Y1 - 2007

UR - http://www.scopus.com/inward/record.url?scp=84873829749&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84873829749&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84873829749

SN - 9781622763344

T3 - 34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts

SP - 219

EP - 222

BT - 34th EPS Conference on Plasma Physics 2007, EPS 2007 - Europhysics Conference Abstracts

T2 - 34th European Physical Society Conference on Plasma Physics 2007, EPS 2007

Y2 - 2 July 2007 through 6 July 2007

ER -

Properties of dense fluid hydrogen and helium and implications for giant gas planets

Publication series

Other

ASJC Scopus subject areas

Other files and links

Cite this