Mass Gain in Supernovae & Black Holes: Explaining Unaccounted Mass

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Discussion Overview

The discussion revolves around the concept of mass gain in supernovae and black holes, particularly in relation to Einstein's theory of relativity and the implications for dark matter. Participants explore the relationship between relativistic effects and the observed discrepancies in mass within galaxies, as well as alternative theories like Modified Newtonian Dynamics (MOND).

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that Einstein's theory suggests mass increases as objects approach light speed, potentially explaining the extra mass observed in supernovae and black holes.
  • Others argue that the evidence for dark matter arises from discrepancies in the gravitational binding of galaxies, which cannot be explained by relativistic mass changes, suggesting a significant amount of mass is unaccounted for.
  • A participant mentions that certain galaxies exhibit rotational curves consistent with Newtonian dynamics, challenging the necessity of dark matter and complicating the MOND perspective.
  • Another participant asserts that the initial premise regarding mass increase due to velocity is incorrect, stating that energy increases instead, referencing a specific energy-momentum relation.
  • There is a discussion about the predictions of MOND versus Cold Dark Matter (CDM) theories, with some participants noting that MOND can predict Newtonian dynamics in certain galaxies while also addressing discrepancies in galactic clusters.
  • Questions are raised regarding the concept of "extra mass," with some participants seeking clarification on what is meant by this term in the context of supernovae events.

Areas of Agreement / Disagreement

Participants express differing views on the implications of relativity for mass in supernovae and black holes, with no consensus on whether relativistic effects can account for the observed mass discrepancies. The discussion includes competing theories, particularly regarding dark matter and MOND, indicating ongoing debate.

Contextual Notes

Participants highlight limitations in the current understanding of mass in astrophysical contexts, including the dependence on definitions of mass and energy, as well as unresolved discrepancies in observational data.

drew500
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einstein's theory states the mass of an object increases as it nears light speed. Much mass therefore must be gained in supernovae events, super massive black holes, ect. Why could not this be offered a possible explanation for the extra mass?
 
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drew500 said:
einstein's theory states the mass of an object increases as it nears light speed. Much mass therefore must be gained in supernovae events, super massive black holes, ect. Why could not this be offered a possible explanation for the extra mass?

Dark matter is a conclusion that flows primarily from the fact that in ordinary, sublight galaxies, thousands of examples of which exists, matter on the fringes of the galaxies is bound much more tightly to the core of the galaxy than the distribution of luminous matter in the galaxy and a simple GMm/r^2 theory of gravity would imply.

Gravitational lensing data from light bent in the vicinity of galaxies likewise shows more bending of light than the luminous matter in the galaxies and Newtonian gravity would imply.

In galaxies of low surface brightness, this discrepency is very high, in different kinds of galaxies, different discrepencies are visible.

The weighted average discrepency from this data is huge, with the data implying that 80%-90% of mass in this low v envrionment is missing, and the disceprencies tend to be greater in lower v environments, rather than higher v environments. It therefore follows the any impact on mass from relativity is ruled out as a cause. The problem is either that there is substantial missing mass or that the non-relativistic case of Newtonian gravity is wrong.

I personally am a strong proponent of the later approach (called MOND for Modified Newtonian Dynamics). The scientific community as a whole favors the dark matter resolution of this data, but respect that there is a difference of opinion on the issue which is respectable.
 
There are also galaxies whose rotational curves fit nicely to Newtonian dynamics... i.e., no dark matter necessary. While this creates headaches for galaxy morphologists, it creates even more headaches for MOND.

When you look at large scale effects, like galactic clusters, any local relativistic contributions are necessarily included. Remember too, the energy debt incurred to increase relativistic mass balances the books - an equivalency principle thing.
 
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Besides, the initial premise is incorrect. Mass don't increase as a consequence of velocity (According to the point of view of the greatest part of the physics community). What increases is its energy, according to the formula
E=-pava
where va is the 4-velocity
 
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Welcome to Physics Forums drew500!

You may like to browse through the posts in the Special & General Relativity section of PF, it contains a lot of material discussing your post and amplifying considerably on meteor's (which hopefully sets you straight on what GR does, in fact, say).
 
Chronos said:
There are also galaxies whose rotational curves fit nicely to Newtonian dynamics... i.e., no dark matter necessary. While this creates headaches for galaxy morphologists, it creates even more headaches for MOND.

I'd differ with you on the evidence there. There are large classes of galaxies where MOND predicts strictly Newtonian dynamics. The principal gap in the evidence is in galactic clusters, where MOND and Newtonian dynamics make the same prediction, where there is a OOM discrepency in the direction one would hope (too little, rather than too much matter). MOND would propose bayronic dark matter in that context, CDM (Cold Dark MatteR) theories would predict modest amounts of CDM. But, CDM does a rather poor job, on its own, of predicting a priori how much CDM there will be in a particular system.
 
hello drew500. I'm not sure what you mean.

Much mass therefore must be gained in supernovae events

You mean due to the high speed at which the outer parts of the star move away from the supernova?
If so, no. All the energy in this energy now in the form of velocity was in the star to begin with.

you say it's an explanation for the 'extra mass'

What extra mass?
 

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