Radiatively efficient accretion onto BHs

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Discussion Overview

The discussion centers on the concept of mass-energy conversion in accretion disks around black holes, specifically addressing the question of where the mass goes when energy is emitted during accretion. The scope includes theoretical considerations and conceptual clarifications related to black hole physics and mass-energy equivalence.

Discussion Character

  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant states that if 1kg of matter falls into a black hole, 0.4kg is converted into energy, leading to a mass increase of only 0.6kg for the black hole.
  • Another participant requests a reference for the claim about mass-energy conversion efficiency.
  • It is suggested that the term "mass" can be confusing, as it has different meanings depending on the context of measurement (local vs. global).
  • One participant explains that the locally measured mass of an individual atom does not change regardless of its proximity to the black hole, while the mass of the black hole is a global quantity that reflects the system's total energy.
  • Another participant introduces the concept of mass deficit, stating that a bound system has less mass than an unbound system with the same constituents, attributing this to the system as a whole rather than specific components.
  • It is noted that the confusion arises from thinking at the atomic level, while the relevant considerations apply at the system level.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of mass in the context of black holes and accretion, with no consensus reached on the implications of mass-energy conversion or the nature of mass deficit.

Contextual Notes

The discussion highlights the complexity of mass-energy relationships in gravitational systems and the potential for confusion arising from different definitions and contexts of mass measurement.

zviz
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It is said that accretion disk around compact objects like black hole can convert up to 40% of the mass of an infalling material into energy.
This means, to my understanding, that if we throw 1kg of matter onto a BH through an accretion disk, during the accretion 0.4kg worth of energy in the form of radiation would be emitted, and the BH would increase its mass by only 0.6kg.

My question is: where did the rest of the mass go? My confusion arises from thinking about the problem in the atomic level. We throw X atoms of hydrogen (totaling 1kg) into the BH. The same X atoms reach the BH, and yet the BH increases its mass by the mass equivalent of only 0.6X atoms of hydrogen. Phrased differently, I wonder what would have happened if I would've stopped the X atoms just before they entered the event horizon, and measured their mass by some experiment, what would I have found? Would the mass be X or 0.6X?
 
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zviz said:
It is said
Where? Please give a reference.
 
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zviz said:
where did the rest of the mass go?
The term "mass" is confusing you here because it has two different meanings.

The locally measured mass of an individual hydrogen atom, let's say, does not change, whether you measure it far away from the hole, just above the horizon, or inside the hole.

The mass of the hole, OTOH, is a global quantity, not the same kind of thing as a locally measured mass. Objects falling into the hole that emit radiation become more tightly bound gravitationally to the hole; in other words, the gravitational binding energy of the hole + object, considered as a system, becomes more negative, which is another way of saying that the total energy of the hole + object system decreases (by the amount of energy contained in the radiation that is emitted and escapes to infinity).
 
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zviz said:
where did the rest of the mass go?
It went out with the radiation.

This is the famous mass deficit. A bound system has less mass than an unbound system with the same constituents. The mass deficit is not attributable to any specific sub-part of the system. It is a deficit of the system as a whole.

zviz said:
My confusion arises from thinking about the problem in the atomic level.
At the atomic level there is nothing to think about here. This feature only exists at the system level.

Measurements made on bound systems cannot identify a specific component where the binding energy came from. It came from the system as a whole, not some specific part of the bound system.

Note, this is not specific to black holes. It applies equally to any bound system. Planets bound to stars, electrons bound to nuclei, protons bound to a nucleus.
 
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