Self-gravitating systems and MOND

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Discussion Overview

The discussion revolves around self-gravitating systems, particularly their negative heat capacity and its implications for understanding gravitational dynamics. Participants explore the relationship between thermodynamic descriptions of self-gravitating systems and the Modified Newtonian Dynamics (MOND) framework, questioning how these concepts may interrelate at different scales, including galactic levels.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants inquire whether the concept of self-gravitation applies solely to bound stellar systems or if it extends to galactic scales.
  • There is a suggestion that the thermodynamic perspective on self-gravitating systems may relate to MOND, particularly regarding flat galactic rotation curves.
  • One participant expresses interest in the connection between MOND and thermodynamics as discussed in the context of entropic gravity, referencing Verlinde’s work.
  • Another participant seeks literature on MOND formulated in terms of negative heat capacity, questioning the extent to which this approach aligns with established formulations.
  • Concerns are raised about discussing unpublished sources and personal theories, with participants clarifying the forum's guidelines regarding acceptable topics.
  • A participant proposes a mathematical approach involving negative heat capacity and Tolman's relation for stationary spacetime, although this is met with confusion regarding its relevance.
  • It is noted that in self-gravitating systems, negative heat capacity is a recognized phenomenon, prompting discussions about the introduction of a gravitational temperature field.

Areas of Agreement / Disagreement

Participants express various viewpoints on the relationship between self-gravitating systems and MOND, with no consensus reached on the applicability of negative heat capacity in this context. The discussion remains unresolved regarding the connections and implications of these concepts.

Contextual Notes

Participants highlight limitations in the existing literature on the topic, particularly regarding the lack of peer-reviewed studies that explicitly connect negative heat capacity with MOND or entropic gravity. There are also unresolved questions about the appropriateness of discussing personal theories and unpublished sources within the forum.

JCTthatsME
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I have been studying self-gravitating systems and their unusual property of negative heat capacity. This makes me wonder how far such a thermodynamic description can be extended.

Does the concept of self-gravitation apply only to bound stellar systems, or could it also be applicable at the galactic scale?

In particular, is there any relation (or contrast) between this thermodynamic perspective and the MOND approach to flat galactic rotation curves?

Could it be said that the 'reach' of a self-gravitating system naturally ends where MOND-type effects begin?
 
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JCTthatsME said:
In particular, is there any relation (or contrast) between this thermodynamic perspective and the MOND approach to flat galactic rotation curves?
Are you familiar with the connection between MOND and thermodynamics that is inherent in Entropic (or Emergent) Gravity? (See https://en.wikipedia.org/wiki/Entropic_gravity.)
 
Yes, I am familiar with Verlinde’s work on entropic gravity, which actually motivated my interest in this topic. However, I have not seen a direct discussion of negative heat capacity (C < 0) in connection with MOND there. That is exactly the link I am trying to understand better.
 
I have been working for some time on a formulation of MOND based on negative heat capacity (C < 0).
However, I am not aware of studies where C < 0 has been explicitly discussed in this context. Are there references that formulate MOND or entropic gravity directly in terms of negative heat capacity, and to what extent is this approach comparable to established formulations? I am specifically looking for literature or exchange opportunities in order to align my ideas with known work.
 
JCTthatsME said:
Are there references that formulate MOND or entropic gravity directly in terms of negative heat capacity, and to what extent is this approach comparable to established formulations? I am specifically looking for literature or exchange opportunities in order to align my ideas with known work.
As far as I can tell, to date there are no credible papers published on this specific topic. However, if you google "negative heat capacity mond gravity" you can easily find an unpublished e-print that claims to consider this. But such a source is unsuitable for discussion here on Physics Forums.
 
I understand that Physics Forums does not allow discussion of personal theories or unpublished sources. My question is: am I allowed to raise a topic if I base it exclusively on peer-reviewed publications, while summarizing the connections in my own words?

For example, if I want to discuss negative heat capacity in self-gravitating systems and its possible relation to gravitational dynamics, but only cite established papers from the literature (without referencing unpublished e-prints), would such a discussion be acceptable?
 
JCTthatsME said:
For example, if I want to discuss negative heat capacity in self-gravitating systems and its possible relation to gravitational dynamics, but only cite established papers from the literature (without referencing unpublished e-prints), would such a discussion be acceptable?
The mentors can correct me, but my understanding is: yes, this is exactly what PF is intended to do. So I say have at it!
 
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I would like to discuss an approach based on negative heat capacity and Tolman's relation for stationary spacetime.

Since I am not sure how to correctly insert mathematical formulas here in the forum, I will make the approach available as a PDF file.

Result: For stationary spacetimes with a timelike Killing field, the gravitational redshift and the field strength can be described by a single gravitothermal potential θ:=lnTgrav (Tolman temperature)

[Moderator's note: attachment deleted]
 
Last edited by a moderator:
JCTthatsME said:
I would like to discuss an approach based on negative heat capacity and Tolman's relation for stationary spacetime.
I am confused as to the relevance of your attachment. The words "heat capacity" appear nowhere.
 
  • #10
In self-gravitating systems it is well known that the heat capacity can become negative [cite Lynden-Bell/Antonov]. This motivates introducing a gravitational temperature field, since standard thermodynamics does not apply directly. I therefore define a gravitothermal potential .
 
Last edited:
  • #11
Thread is closed temporarily for Moderation.
 
  • #12
JCTthatsME said:
I understand that Physics Forums does not allow discussion of personal theories or unpublished sources.
That's correct. And yet your post #8 does exactly that, as you confirm in your post #10. Therefore, this thread will remain closed.
 
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