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Title: Properties of hydrogen, helium, and silicon dioxide mixtures in giant planet interiors

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4978618· OSTI ID:1465731

Recent observations of Jupiter and Saturn provided by spacecraft missions, such as Juno and Cassini, compel us to revise and improve our models of giant planet interiors. Even though hydrogen and helium are by far the dominant species in these planets, heavy elements can play a significant role in the structure and evolution of the planet.

Research Organization:
Univ. of California, Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Grant/Contract Number:
SC0010517; SC0016248
OSTI ID:
1465731
Alternate ID(s):
OSTI ID: 1373965
Journal Information:
Physics of Plasmas, Vol. 24, Issue 4; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 26 works
Citation information provided by
Web of Science

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Cited By (13)

How cores grow by pebble accretion: I. Direct core growth journal March 2018
The static local field correction of the warm dense electron gas: An ab initio path integral Monte Carlo study and machine learning representation journal November 2019
Quantum molecular dynamics study on the proton exchange, ionic structures, and transport properties of warm dense hydrogen-deuterium mixtures journal June 2018
Simple scaling laws for the transport coefficients calculated by density-functional theory molecular dynamics journal June 2019
Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution journal January 2020
Path integral Monte Carlo simulations of dense carbon-hydrogen plasmas journal March 2018
Explaining the low luminosity of Uranus: A self-consistent thermal and structural evolution text January 2019
The interiors of Uranus and Neptune: current understanding and open questions
  • Helled, Ravit; Fortney, Jonathan J.
  • Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, Vol. 378, Issue 2187 https://doi.org/10.1098/rsta.2019.0474
journal November 2020
Ab initio Path Integral Monte Carlo Results for the Dynamic Structure Factor of Correlated Electrons: From the Electron Liquid to Warm Dense Matter journal December 2018
Explaining the low luminosity of Uranus: a self-consistent thermal and structural evolution text January 2020
Permutation blocking path integral Monte Carlo simulations of degenerate electrons at finite temperature journal January 2019
How cores grow by pebble accretion: I. Direct core growth ( Corrigendum ) journal December 2018
The exoplanet handbook: Book Review journal March 2012

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