Mass conservation in black holes

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Discussion Overview

The discussion centers on the conservation of mass in the context of black holes, particularly focusing on gravitational collapse and the implications for energy conservation as matter approaches the event horizon. It explores theoretical frameworks and interpretations related to mass and energy in black hole physics.

Discussion Character

  • Debate/contested
  • Conceptual clarification
  • Technical explanation

Main Points Raised

  • Some participants suggest that the mass of gravitationally collapsed matter may not be a meaningful question once a black hole forms, as the singularity implies no matter exists inside the black hole.
  • Others argue that in a classical scenario with no matter ejected, the mass parameter outside a non-rotating black hole remains the same before and after collapse, adhering to the Schwarzschild solution.
  • It is proposed that for spinning black holes, there is a trade-off between mass and angular momentum, but the relationship may not be straightforward and could involve complexities in the spacetime geometry.
  • One participant posits that in an idealized collapse with no emissions, the total mass of the system (emitted plus remaining in the black hole) can be conserved, although this is not reflective of real scenarios.
  • Questions arise regarding energy conservation as matter approaches the event horizon, with some participants challenging the notion that mass becomes infinite in this context.
  • There is a contention about whether the frequency of a photon increases infinitely as it nears the event horizon, with some participants disputing this claim and questioning its implications for energy and mass.

Areas of Agreement / Disagreement

Participants express differing views on the conservation of mass and energy in black holes, with no consensus reached on the implications of gravitational collapse or the behavior of matter near the event horizon.

Contextual Notes

Discussions involve assumptions about idealized scenarios versus real-world conditions, and the definitions of mass and energy may vary among participants. The complexities of rotating versus non-rotating black holes also contribute to the uncertainty in the discussion.

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Is the mass of gravitationally collapsed matter conserved in a black hole?
 
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Depends what you mean.

Classically, gravitational collapse leads to a singularity. There isn't any matter inside the hole once the collapse completes, so whether its mass is conserved or not isn't a necessarily a meaningful question.

If the initial state was spherically symmetric and non-rotating then the gravitational field outside the hole is Schwarzschild with the same mass parameter before and after the collapse (assuming no matter was ejected before crossing the horizon). That might be what you mean.

If the black hole is spinning then you can trade between mass and angular momentum, within limits. That may not match what you mean. Also, as far as I'm aware, nobody has proved that the spacetime around a rotating mass that isn't a black hole is Kerr (and I rather suspect it isn't exactly). So it's at least possible that the mass parameter in the spacetime around the black hole is not the same as the one around the original star, even allowing for mass loss.
 
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Ranku said:
Is the mass of gravitationally collapsed matter conserved in a black hole?
In an idealized collapse where nothing is emitted (no matter or radiation or gravitational waves), the mass of the spacetime, i.e., the geometric property (for example, the mass you would get by putting a test object in orbit and measuring its orbital parameters) is conserved.

Of course no real collapse occurs with nothing being emitted. But there are still ways to define the mass that's emitted such that the total mass (what's emitted plus what remains in the black hole) is conserved. ("Mass" is not the usual expression for the quantities involved, "energy" is, since rest mass is not the only contribution to it.)
 
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Ibix said:
If the black hole is spinning then you can trade between mass and angular momentum, within limits.
Even in this case, I believe there is a way to capture the exchange so that the mass and the angular momentum of the overall spacetime are conserved.
 
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Does energy conservation hold when matter approaches the event horizon of a black hole and its mass becomes infinite?
 
liuzilu said:
Does energy conservation hold when matter approaches the event horizon of a black hole and its mass becomes infinite?
The mass of matter doesn't become infinite as it approaches the event horizon. Where did you get the idea that it does?
 
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Ibix said:
The mass of matter doesn't become infinite as it approaches the event horizon. Where did you get the idea that it does?
For example, as a photon approaches the event horizon, its frequency becomes infinitely high. Doesn't that mean its energy (mass) becomes infinite as well?
 
liuzilu said:
For example, as a photon approaches the event horizon, its frequency becomes infinitely high. Doesn't that mean its energy (mass) becomes infinite as well?
Huh? Where did you get THAT idea?
 
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liuzilu said:
For example, as a photon approaches the event horizon, its frequency becomes infinitely high.
No it doesn't - where did you get that idea?
 
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