Mass Gain in Supernovae & Black Holes: Explaining Unaccounted Mass

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In summary, Einstein's theory states that an object's mass increases as it nears light speed, which could explain the extra mass gained in supernovae events and super massive black holes. However, observations of galaxies and gravitational lensing data suggest that there is a significant amount of missing mass, leading to the theory of dark matter or the modified theory of MOND. While there is debate among the scientific community, MOND seems to better fit certain observations, but creates challenges in other areas such as galactic clusters. Ultimately, the idea that mass increases due to velocity is incorrect and it is actually the object's energy that increases.
  • #1
drew500
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Einstien'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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  • #2
drew500 said:
Einstien'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.
 
  • #3
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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  • #4
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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  • #5
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).
 
  • #6
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.
 
  • #7
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?
 

FAQ: Mass Gain in Supernovae & Black Holes: Explaining Unaccounted Mass

What is the process of mass gain in supernovae and black holes?

Mass gain in supernovae occurs when a massive star reaches the end of its life and undergoes a powerful explosion, releasing large amounts of energy and matter into space. This explosion can also create a black hole, which is a region of space with an extremely strong gravitational pull that can trap matter and even light.

Why is there unaccounted mass in supernovae and black holes?

The unaccounted mass in supernovae and black holes is a result of the intense gravitational pull of these objects. This gravitational pull is so strong that it can pull in matter from the surrounding area, including gases and other debris, which adds to the overall mass of the object.

How do scientists explain the unaccounted mass in supernovae and black holes?

Scientists use various models and theories to explain the unaccounted mass in supernovae and black holes. One theory is that the intense gravitational pull can cause matter to collapse and form into a singularity, which is a point of infinite density and zero volume. Another theory suggests that the unaccounted mass may be dark matter, which is a type of matter that does not interact with light but still exerts a gravitational pull.

Can the unaccounted mass in supernovae and black holes be measured?

The unaccounted mass in supernovae and black holes can be indirectly measured through observations of their effects on surrounding matter and light. For example, scientists can study the gravitational lensing effect, where the intense gravity of a black hole bends and distorts light from distant objects, to estimate the mass of the black hole.

How does understanding mass gain in supernovae and black holes help us understand the universe?

Studying mass gain in supernovae and black holes can provide valuable insights into the life cycles of stars and the formation of galaxies. It also helps us understand the role of gravity in the universe and how it shapes the movement and interactions of celestial objects. Additionally, understanding how black holes form and grow can help us better understand the fundamental laws of physics and the nature of space and time.

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