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researcher

S. Muller

8 papers hereh-index 441 citations12 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author6
  • last author2

Across the 8 of 8 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP6
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • S. Muller — 86 papers, h 34
  • S. Muller — 23 papers, h 13
  • S. Muller — 20 papers, h 24
  • S. Muller — 19 papers, h 4
  • S. Muller — 10 papers, h 7
  • S. Muller — 7 papers, h 19

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20232026
most citedEvolution of Jupiter and Saturn with helium rain

35 citations · 56 across the 8 of their papers we have counts for

collaborators
Showing 2024Show all

4 papers · 1 filter

astro-ph.IM2024★ 3 cited

Uranus Study Report: KISS

Mark Hofstadter, Ravit Helled, David J. Stevenson +27

Determining the internal structure of Uranus is a key objective for planetary science. Knowledge of Uranus's bulk composition and the distribution of elements is crucial to underst…

astro-ph.EP2024★ 16 cited

Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?

Saburo Howard, Ravit Helled, Simon Müller

Revealing the internal composition and structure of giant planets is fundamental for understanding planetary formation. However, the bulk composition can only be inferred through i…

astro-ph.EP2024★ 35 cited

Evolution of Jupiter and Saturn with helium rain

Saburo Howard, Simon Müller, Ravit Helled

Phase separation between hydrogen and helium at high pressures and temperatures leads to the rainout of helium in the deep interiors of Jupiter and Saturn. This process, also known…

astro-ph.EP2024★ 2 cited

Uranus' Complex Internal Structure

Benno A. Neuenschwander, Simon Müller, Ravit Helled

Uranus' bulk composition remains unknown. Although there are clear indications that Uranus' interior is not fully convective, and therefore has a non-adiabatic temperature profile,…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.