Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Videos

Alternative model of the Antonov problem.

L Velazquez1, F Guzmán

  • 1Departamento de Física, Universidad de Pinar del Río, Martí 270, Esq. 27 de Noviembre, Pinar del Río, Cuba. luisberis@geo.upr.edu.cu

Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics
|February 3, 2004
PubMed
Summary

Astrophysical systems, unlike those in rigid containers, naturally evaporate. This study proposes an energetic prescription to confine particles, creating a unified model of astrophysical thermodynamics with emergent system size.

Related Concept Videos

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Black Hole Spectroscopy and Tests of General Relativity with GW250114.

Physical review letters·2026
Same author

GW250114: Testing Hawking's Area Law and the Kerr Nature of Black Holes.

Physical review letters·2025
Same author

Quasi-stationary distributions for the collective motions of a binary astrophysical system: A Langevin dynamics approach.

Chaos (Woodbury, N.Y.)·2025
Same author

Complex systems and inter/transdisciplinary research: A review.

Chaos (Woodbury, N.Y.)·2024
Same author

Langevin equation for the collective motions of a binary astrophysical system.

Chaos (Woodbury, N.Y.)·2023
Same author

Quantitative methods to determine the student workload: II. Statistical models for the microcurricular performance indicators.

Chaos (Woodbury, N.Y.)·2022

Area of Science:

  • Astrophysics
  • Thermodynamics
  • Statistical Mechanics

Background:

  • Astrophysical systems are inherently open and prone to particle evaporation due to gravity's limitations.
  • Traditional models often use artificial confinement (rigid containers) to simulate equilibrium, which is unrealistic.
  • The Antonov isothermal model describes gravitational collapse but requires confinement.

Purpose of the Study:

  • To propose an energetic prescription for particle confinement in astrophysical systems.
  • To develop an alternative Antonov isothermal model that unifies isothermal and polytropic profiles.
  • To investigate a model where system size naturally emerges from particle evaporation.

Main Methods:

  • Developing a novel energetic prescription for particle confinement.

Related Experiment Videos

  • Formulating an alternative Antonov isothermal model.
  • Analyzing the thermodynamic properties, including gravitational collapse and negative specific heat.
  • Main Results:

    • The proposed energetic prescription successfully confines particles, preventing unrealistic evaporation.
    • The new model unifies isothermal and polytropic profiles within a single framework.
    • System size naturally arises as a consequence of particle evaporation, resolving a key challenge.

    Conclusions:

    • The proposed energetic prescription offers a more realistic approach to modeling astrophysical thermodynamic equilibrium.
    • This unified model provides a more comprehensive understanding of stellar systems and gravitational collapse.
    • The emergent system size is a significant advancement, reflecting natural astrophysical processes.