2005/07/08 by Fedor V. Prigara, Prigara, Fedor V.
Earth and Planetary Sciences · Physics and Astronomy · #Accretion (finance) #Accretion disc #Astrophysics #Astrophysics (astro-ph) #Dust and Plasma Wave Phenomena #FOS: Physical sciences #High-pressure geophysics and materials #Nuclear physics #Optical properties and cooling technologies in crystalline materials #Optics #Physics #Plasma #Radiation #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0507199
published in arXiv (Cornell University) (Cornell University) · 2 pages, in Astrophysical Sources of High Energy Particles and Radiation, Torun, Poland, 20-24 June 2005
arxiv created 2005/07/08 · openalex publication_date 2005/07/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
It is shown that the existence of radiation-induced solitary waves in hot plasmas of accretion disks depends on the radial temperature profile.