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researcher

S. Davis

65 papers hereh-index 385.7k citations87 works total

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

author position
  • first author14
  • middle author30
  • last author21

Across the 65 of 65 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE32
  • astro-ph17
  • astro-ph.GA7
  • astro-ph.IM4
  • astro-ph.CO3
  • astro-ph.EP1
same name
  • S. Davis — 33 papers, h 15
  • S. Davis — 26 papers, h 17
  • S. Davis — 16 papers, h 21
  • S. Davis — 10 papers, h 4
  • S. Davis — 8 papers, h 5
  • S. Davis — 5 papers, h 5

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
20032023
most citedIntrinsic disc emission and the Soft X-ray Excess in AGN

622 citations · 7.3k across the 65 of their papers we have counts for

collaborators
Showing 2013 · astro-ph.HEShow all

4 papers · 2 filters

astro-ph.HE2013★ 114 cited

Line driven winds and the UV turnover in AGN accretion discs

Ari Laor, Shane W. Davis

AGN SEDs generally show a turnover at lambda 1000A, implying a maximal accretion disc (AD) temperature of T_max~50,000K. Massive O stars display a similar T_max, associated with a…

astro-ph.HE2013★ 121 cited

On the Thermal Stability of Radiation Dominated Accretion Disks

Yan-Fei Jiang, James Stone, Shane Davis

We study the long-term thermal stability of radiation dominated disks in which the vertical structure is determined self-consistently by the balance of heating due to dissipation o…

astro-ph.HE2013★ 77 cited

Dynamics of warped accretion discs

Scott Tremaine, Shane W. Davis

Accretion discs are present around both stellar-mass black holes in X-ray binaries and supermassive black holes in active galactic nuclei. A wide variety of circumstantial evidence…

astro-ph.HE2013★ 38 cited

Saturation of the MRI in Strongly Radiation Dominated Accretion Disks

Yan-Fei Jiang, James M. Stone, Shane W. Davis

The saturation level of the magneto-rotational instability (MRI) in a strongly radiation dominated accretion disk is studied using a new Godunov radiation MHD code in the unstratif…

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