On the evolution of a primordial interstellar gas cloud

DOI10.1063/1.5144917zbMath1455.85001OpenAlexW3085111537MaRDI QIDQ5141056

Mayer Humi

Publication date: 17 December 2020

Published in: Journal of Mathematical Physics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1063/1.5144917

zbMATH Keywords

cosmologyprimordial gastime-dependent Euler-Poisson equations

Mathematics Subject Classification ID

PDEs in connection with fluid mechanics (35Q35) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Galactic and stellar dynamics (85A05) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Astrophysical cosmology (85A40)

Related Items (2)

Traveling waves in an evolving interstellar gas cloud ⋮ Nonlinear dynamics of structure formation in protoplanetary disks

Cites Work

• On uniformly rotating stars
• Non-uniformly rotating, self-gravitating, compressible masses with internal meridian circulation
• Exact self-gravitating disks and rings: A solitonic approach
• The gravitational potential due to uniform disks and rings
• Ellipsoidal figures of equilibrium—an historical account
• Unnamed Item
• Unnamed Item

This page was built for publication: On the evolution of a primordial interstellar gas cloud