Black Holes, Quantum Gravity and the Curvature of spacetime

In summary: to measure how matter affects the geometry of spacetime---you can't do this directly, but you can use the mathematical tools of quantum theory to calculate the consequences of measuring the geometrynow, if you measure the geometry and find that it has changed---for example, if you measure the distance between two points and find that it has decreased---this is an experimental result that can be explained by the theory of general relativitybut if you measure the geometry and find that it has remained unchanged---for example, if you measure the distance between two points and find that it has remained at the same value---this is an experimental result that cannot be explained by the theory of general relativity===================so, in summary, quantum
  • #1
juan_rod
9
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What is Quantum Gravity and the Curvature of Spacetime and how is it all relevant to one another?
 
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  • #2
Welcome to the forum.
As your just getting started here allow me to offer a few tips.
If your not working on a classroom or homework problem (Top of the main page), go to the appropriate forum for the subject.
Looks like you've found your way kind of close to the area you want, but still forums work best when you know enough about the area to be able to ask a pointed question.
For questions like "What is this subject and what does it mean for some other subject" are better handled by starting with a book so you can have enough knowlage to ask a question.
And once you know enough to ask; remember you can often find where your question has already been asked use the SEARCH Function - find a few relevant threads and go though them, then you can also get a feel how to use the forum from the example of how other questions have been handled. Find and read the sticky threads (on top) and actually read and understand the forum rules.

How to pick a book to read - search for a question. Try looking for "quantum book" or "relativity book" I'm sure you'll see some recommendations and maybe some website explanations to read as well.
 
  • #3
Actually how quantum gravity relates to curvature of space-time seems like an interesting question. Is it really impossible to give some overview on the general approach on how to introduce backgound independence into quantum theory?
 
  • #4
Because my main interest was in understanding what is known about black holes, i began reading on the properties of black holes. in the article that i was reading Quantum Gravity is mentioned. now i am reading on Quantum Gravity and how it what occurs when Quantum Gravity Meets the Quantum Theory, my problem now is this equation and what it means in relation to Quantum Gravity and to the properties of a black hole.
"In general relativity, mass and energy are treated in a purely classical manner, where ‘classical’ means that physical quantities such as the strengths and directions of various fields and the positions and velocities of particles have definite values. These quantities are represented by tensor fields, sets of (real) numbers associated with each spacetime point. For example, the stress, energy, and momentum Tab(x,t) of the electromagnetic field at some point (x,t), are functions of the three components Ei, Ej, Ek, Bi, Bj, Bk of the electric and magnetic fields E and B at that point. These quantities in turn determine, via Einstein's equations, an aspect of the ‘curvature’ of spacetime, a set of numbers Gab(x,t) which is in turn a function of the spacetime metric. The metric gab(x,t) is a set of numbers associated with each point which gives the distance to neighboring points. At the end of the day, a model of the world according to general relativity consists of a spacetime manifold with a metric, the curvature of which is constrained by the stress-energy-momentum of the matter distribution. All physical quantities — the value of the x-component of the electric field at some point, the scalar curvature of spacetime at some point — have definite values, given by real (as opposed to complex or imaginary) numbers. Thus general relativity is a classical theory in the sense given above."
 
  • #5
juan_rod said:
What is Quantum Gravity and the Curvature of Spacetime and how is it all relevant to one another?
Oh, I did not see your most recent post. This is a reply to your original post.
Juan, the first thing to understand is the classical idea of the curvature of space, from back in 1915 before quantum theory entered the picture

it was Einstein's insight that what we experience as gravity is really geometry, and the Einstein equation of 1915 shows how the distribution of matter determines the shape of space around it-----this is the main equation of Gen Rel

a famous physicist later put that equation into words: "Matter tells spacetime how to curve. Spacetime tells matter how to move."

=================

starting in 1919 the geometrical theory of gravity (Gen Rel) was tested---repeatedly and with increasing precision. It really does predicts what will happen more accurately than non-geometric theories----theories in which space is a rigid rectilinear framework and gravity is explained by force vectors

===============
so after 80 years of testing Gen Rel, we pretty much accept that space is a dynamic, changing, active thing-----its shape changes as matter moves around in it.

fortunately it doesn't change very much except for very dense massive things, so we don't notice------it is still approximately the foresquare rigid spacetime that Newton imagined, so for practical purposes we still think of it like that.
===============

quantum theory comes in when you try to give this dynamic geometry, interacting with matter, a QUANTUM description-----that means using stuff like wave-functions, and having uncertainty built in.

it doesn't mean that space has to be divided up into little bits:rofl:

(sometimes people think space must be made of quanta)

it means that things that you observe and measure about the geometry of space----like SURFACE AREA, and ANGLE, and VOLUME, and even the dimensionality itself-----are no longer fixed definite things but are instead quantum observables (which can incorporate uncertainty)

For example, in a quantum model of a region of spacetime, the curvature is allowed to have some uncertainty---and depend on the quantum state of the system.

that's all I can provide as an introduction. the main thing is to understand the pre-quantum 1915 business first-----when that is assimilated it is easier to think about shifting to a quantum version of it.
 
  • #6
MeJennifer said:
Actually how quantum gravity relates to curvature of space-time seems like an interesting question. Is it really impossible to give some overview on the general approach on how to introduce backgound independence into quantum theory?
If and when someone can do it I suppose they might, but being able to give a correct way to start would mean you knew were you were going.
Smolin in his book and Perimeter Institute papers seem to show they have tried several approaches and are still looking very hard.
Personally I do not think they will succeed in combining the background independence of GR with QM or the Standard Model.
 
  • #7
marcus said:
Oh, I did not see your most recent post. This is a reply to your original post.
Juan, the first thing to understand is the classical idea of the curvature of space, from back in 1915 before quantum theory entered the picture

it was Einstein's insight that what we experience as gravity is really geometry, and the Einstein equation of 1915 shows how the distribution of matter determines the shape of space around it-----this is the main equation of Gen Rel

a famous physicist later put that equation into words: "Matter tells spacetime how to curve. Spacetime tells matter how to move."

=================

starting in 1919 the geometrical theory of gravity (Gen Rel) was tested---repeatedly and with increasing precision. It really does predicts what will happen more accurately than non-geometric theories----theories in which space is a rigid rectilinear framework and gravity is explained by force vectors

===============
so after 80 years of testing Gen Rel, we pretty much accept that space is a dynamic, changing, active thing-----its shape changes as matter moves around in it.

fortunately it doesn't change very much except for very dense massive things, so we don't notice------it is still approximately the foresquare rigid spacetime that Newton imagined, so for practical purposes we still think of it like that.
===============

quantum theory comes in when you try to give this dynamic geometry, interacting with matter, a QUANTUM description-----that means using stuff like wave-functions, and having uncertainty built in.

it doesn't mean that space has to be divided up into little bits:rofl:

(sometimes people think space must be made of quanta)

it means that things that you observe and measure about the geometry of space----like SURFACE AREA, and ANGLE, and VOLUME, and even the dimensionality itself-----are no longer fixed definite things but are instead quantum observables (which can incorporate uncertainty)

For example, in a quantum model of a region of spacetime, the curvature is allowed to have some uncertainty---and depend on the quantum state of the system.

that's all I can provide as an introduction. the main thing is to understand the pre-quantum 1915 business first-----when that is assimilated it is easier to think about shifting to a quantum version of it.

Thank you, this clears up a lot. But how is it all relevant to a black hole and it's properties?
 
  • #8
juan_rod said:
Thank you, this clears up a lot. But how is it all relevant to a black hole and it's properties?

Several people are around here who could reply well to that. I will give someone else a chance.
 
  • #9
juan_rod:” What is Quantum Gravity and the Curvature of Spacetime and how is it all relevant to one another?”

marcus:” a famous physicist later put that equation into words: "Matter tells spacetime how to curve. Spacetime tells matter how to move."

“it means that things that you observe and measure about the geometry of space----like SURFACE AREA, and ANGLE, and VOLUME, and even the dimensionality itself-----are no longer fixed definite things but are instead quantum observables (which can incorporate uncertainty)

For example, in a quantum model of a region of spacetime, the curvature is allowed to have some uncertainty---and depend on the quantum state of the system.

that's all I can provide as an introduction. the main thing is to understand the pre-quantum 1915 business first-----when that is assimilated it is easier to think about shifting to a quantum version of it.”

It seems that nature like follow to something very exceptional. In addition to
Marcus suggestion and in accordance with him look also the elliptical geometry in S7 E.Cartan “sphere” which admits an absolute parallelism.

juan_rod:” But how is it all relevant to a black hole and it's properties?”

I have no idea.
 
  • #10
Hence my problem... thanks a lot everyone.
 
  • #11
Anonym said:
juan_rod:” But how is it all relevant to a black hole and it's properties?”

I have no idea.

Wait, Juan and Anonym, I will try to reply. I thought some other people would like to reply, but they didn't.

You ask what BH has to do with classic 1915 Gen Rel and also with QG.

I think maybe you know the answer or part of the answer.

everything that has been observed about BH so far is simply consistent with classic Gen Rel and has nothing to do with QG

I think you will agree. If not, please say how I am mistaken. Astronomers have no observation of BH hawking radiation or BH evaporating. So there is no empirical data about relation of QG to BH!

By contrast there is a large amount of empirical data about stuff observed falling into BH and the minimal stable orbit radius----and the redshift of X ray from iron very close to hole----and so on. Wonderful empirical data. Stars have been observed orbiting the central BH in our galaxy and so on. All that is wonderful but perfectly classical.

So your question about what is relevance of QG to BH has a peculiar status. Unless we get some new observation, the question concerns something about which there is no empirical data, but is a rather more speculative question, purely about theory.
 
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  • #12
juan_rod said:
Hence my problem... thanks a lot everyone.
Well you seem more advanced than I thought your OP indicated.
I’d recommend considering what you already know about the fundamentals behind the two ideas: “Quantum Gravity” “Curvature of Spacetime” and how they are relevant to each other, before you worry about how they may be relevant to a Black Hole.

“Quantum Gravity” - Fundamentally based a quantum approach, utilizing QM (its derivatives or equivalents) and uses the Standard Model including the idea of particle exchange of gravitons (yet to be discovered) to account for gravity.

“Curvature of Spacetime” – Fundamentally linked to GR and accounting gravity by curves or warping in a 4D Dimensions (some claim 5) with our view of 3 dimensions and time along with gravity being the result. Note the lack of need or use of particle exchange.

Most see these two ideas, as completely incompatible. I agree with the view (but not all do) that they cannot be combined. As in, at least one must be shown as wrong (but they both work so well) some day! Hence my opinion that Smolin will not succeed in combining the background independence of GR with QM or the Standard Model.

Got to hand to those with the persistence to keep trying to combine them, IMO they are working on the core of your question.
 
  • #13
Parampreet Singh in Ashtekar's group at Penn State has proposed a new phenomenon to look for in Gammaray Bursts (GRB) that would have a QG signature. I heard this in a recorded Penn State seminar talk

:smile:

you see, I have to stretch very hard to reach some contact with empirical observation. He says that some instances of gravitational collapse would release a GRB with a distinctive lightcurve. I don't remember, the lightcurve would have some peculiar feature that astronomers could be told to look for.

In QG, gravitational collapse is different because gravity actually turns repulsive at near-Planck density. Some extreme cases might look different.

My apologies----I do not know if this work of Singh has even been published.
==================

I will try to think of some more cases. If one has no observational check then there is no certitude of talking about something real---it could all be just weaving words about the artifacts of theory.
 
  • #14
From my basic understanding of QG and QM, i know that quantum leaps from within electrons in the matter surrounding and in front of a BH make it seem as if time curves and or slows down. i also understand that space-time curvature helps both find and identify a BH.

if any of my assertions are wrong please share some insight.
 
  • #15
Marcus:” Wait, Juan and Anonym”
“everything that has been observed about BH so far is simply consistent with classic Gen Rel”

Sorry, when I was a student, I attended the seminar given by Y.Zeldovich at Moskow Stecklov Institute. The issue was not a particular problem or particular solution of some problem. Y.Zeldovich presented analysis whether the Einstein GR contains essential singularity. If I understood him correctly, the answer was no.
However, I agree to wait
 
  • #16
Of course, what happens to RT at this singularity?
 
  • #17
juan_rod said:
What is Quantum Gravity and the Curvature of Spacetime and how is it all relevant to one another?
With regards to this question I am interested to see what the members here think of integrating quantum theory with the priniciple of general covariance. Is it at all possible or would it indicate a fundamental flaw in at least one of the theories?
 
  • #18
DocN:” what happens to RT at this singularity?”

I beg your pardon for my ignorance, what RT stands for?
 
  • #19
Anonym said:
DocN:” what happens to RT at this singularity?”

I beg your pardon for my ignorance, what RT stands for?

I think he means "renormalization theory" or something like that

[EDIT: correction, I see from DocN next post that he may have meant "relativity theory"]

Anonym, I was interested by what you said here:
...when I was a student, I attended the seminar given by Y.Zeldovich at Moskow Stecklov Institute. The issue was not a particular problem or particular solution of some problem. Y.Zeldovich presented analysis whether the Einstein GR contains essential singularity. If I understood him correctly, the answer was no.
However, I agree to wait

I agree that classical Einstein GR with a positive cosmological constant Lambda can have a bounce that begins the expansion phase. It does not absolutely need to have a cosmological singularity there. But I am not sure that I understand what you are reporting from Zeldovich.

I was glad to hear that you were attending seminars at the Steklov. This is to be congratulated as a kind of good fortune. Very famous institute. I hope your present location is also stimulating and has plenty of ideas.
 
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  • #20
doestn't relativity theory "collapse" at the singularity just like all physics laws?
Doc
 
  • #21
DocN said:
doestn't relativity theory "collapse" at the singularity just like all physics laws?
Doc

What is it that you mean exactly by "collapse", and how do all the laws of physics "collapse" at the singularity?
 
  • #22
DocN said:
doestn't relativity theory "collapse" at the singularity just like all physics laws?
Doc

a singularity is defined in the context of some particular theory---as a place where that particular theory breaks down (i.e. produces meaningless results)----so a singularity, or breakdown, in the theory helps define the limits of applicability of the theory.

A breakdown in Gen Rel would not, AFAIK, imply a breakdown in actual physical reality (however one defines that :-) ) or a necessary breakdown in other physical laws.

One way to say this is "singularities do not exist in nature, as far as we know, they are glitches in theories".

I think you may very well agree with what I just said. If you don't please offer us some physical evidence of the existence of the big bang singularity, besides just the fact that one theory, Gen Rel, breaks down there.

Assuming you DO agree with what I just said, let me try to answer the question you asked, that was quoted here.

"Doesn't Gen Rel break down at the cosmological singularity?"

Yes, by definition. The cosmological singularity is defined using Gen Rel, as a place where Gen Rel breaks down. So yes.

"...just like all other physical laws."

How do we know other physical laws break down at the beginning of expansion? Other theories constructed to replace Gen Rel do NOT predict infinite pressure, curvature, density, temperature. I don't know of any empirical evidence yet to say who is right. I would assume that much of physical law would have to be CORRECTED to be applicable at very high (Planck) temperature and density. Perhaps one would need radically new law or perhaps extensive quantum corrections. I simply don't know. But I have no scientific reason to suppose that ALL physical law simply "collapses" and ceases to apply.
 
  • #23
Marcus:” I think he means "renormalization theory" or something like that

[EDIT: correction, I see from DocN next post that he may have meant "relativity theory"]”

“I agree that classical Einstein GR with a positive cosmological constant Lambda”

“everything that has been observed about BH so far is simply consistent with classic Gen Rel and has nothing to do with QG”

Let define what we are discussing. I suggest:
1.classic Einstein GR means without cosmological term;
2.GR means “relativity theory”;
3.nothing to do with QG means "renormalization theory" is not relevant.

I am outsider here. I jumped into discussion since juan_rod originally posted his thread in Quantum Physics. I was sure that you laughing in me (and I deserve it).I was ready to quit. However, perhaps, I misinterpret you.
Now I guess that DocN referred to Ch.12-14 of the later edition (6) of L.D. Landau, E.M. Lifshtz “Field Theory” which I never read until today. It turns out that E.M.Lifshtz desided to improve L.D.Landau. However, Y. Zeldovich et al are discussed there in details. I refer to seminar since I hadn’t reference in hand ( by the way, this is the only seminar at Steklov I was attending. Occasionly I jumped to Moskow and was invited to listen “as a kind of good fortune”).

I interpret the negative answer of Y.Zeldovich as a statement that BH may be “gauged” away from GR in contrast with your statement.

Why I am here I will explain in the next post.

DocN:” doestn't relativity theory "collapse" at the singularity just like all physics laws?”

And what are substitutions? Hollywood movies?

I guess that it is the collapse of wave packet speaking (transition from Quantum world to Classical world: E. Schrödinger Cat). BH out, WH remain similarly as W.Ritz in the classical electrodynamics.
 
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  • #24
Anonym; And what are substitutions? Hollywood movies? I guess that it is the collapse of wave packet speaking (transition from Quantum world to Classical world: E. Schrödinger Cat). BH out said:
My original question consisted of a general and or limited understanding of Quantum physics and the curvature of space-time. now you have introduced electrodynamics, how is this relevant to the properties of a BH?
 
  • #25
juan_rod:” My original question consisted of a general and or limited understanding of Quantum physics and the curvature of space-time. now you have introduced electrodynamics, how is this relevant to the properties of a BH?”

You received the identical answer to your original question from Marcus and me.But nobody know the ultimate truth. Let me formulate our answer in my own words:

The classical A. Einstein local field theory of gravitational interactions is not complete ( It can’t be wrong, it based on universally valid and firmly established experimental result that the inertial mass is identical to the gravitation mass. It has enormous predictive power, it was verified and confirmed by all available experiments. In addition, it is most beautiful theory ever formulated by human mind). However, our answer was: the Cartan’s torsion should be added (see Marcus in the “Einstein was wrong, and should be Cartanized!” session and F.W. Hehl et al, Rev. Mod. Phys., 48, 393 (1976) for example). They wrote:”Not least among this evidence is the demonstration that the U(4) theory arises as a local gauge theory for the Poincare group in space-time”. That I also know with certainty from completely different consideration (the structure of the tensor products in QM). Compare with A. Einstein (1915), today we have experimental evidence that in addition to the long range interactions transparent in the Classical world, two short range interactions are hidden classically and transparent in the Quantum world: weak and strong. All four are called the fundamental interactions. It is generally accepted that no other fundamental interactions exist. All fundamental interactions have the same origin: presence of phases in the QM description of system states. It allows to formulate a principal postulate of the physics: Principle of Local Gauge Invariance (E. Schrödinger, H. Weyl, Y. Aharonov, D. Bohm and ultimately C.N. Yang and R.L. Mills; for review see L. O’Raifeartaigh “ The Daving of Gauge Theory”, Prinston Univ. Press (1997). Using that postulate the phenomenological U(2) theory of electroweak interactions was formulated ( S. Weinberg et al). It has unquestionable experimental confirmation. In addition, the identical approach allows to formulate the preliminary version of the strong interactions (QCD). It also has substantial experimental support.

All that I consider as elements of the relativistic quantum field theory. The consistent formulation of that theory is still open problem. I do not believe that the formulation of QG may be obtained before, however, every attempt is legitimate. This is the way the physical knowledge is acquired.

For the described reasons I consider our debate about BH very interesting but at present status of the theory groundless. I have no required background in gravitation (I did not work in that area of scientific research, only read sporadically experimental and theoretical papers). In past I was deeply impressed by Y. Zeldovich presentation, he demonstrated time oscillations in classical world which I associate with the quantum behaviour. For all these reasons I did not accept Marcus statement “everything that has been observed about BH so far is simply consistent with classic Gen Rel”. But frankly, I have no idea. For sure, the complete classical as well as quantum gravitation theory must be in compliance with all physical knowledge obtained during last 450 years and not in contradiction with it.

If what I said still seems to you complicated, next time try to ask more simple questions.
 
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  • #26
Can one say that at the singularity, we would find such a transition from GR to quantum states? It appears that even the black hole itself is circular in shape--still a classical formation?
 
  • #27
For the described reasons I consider our debate about BH very interesting but at present status of the theory groundless. I have no required background in gravitation (I did not work in that area of scientific research said:
it seems maybe, that i am trying to put things together in my own terms using only limited knowledge. thank you all for your help. Because no one fully understands the properties and the behavioral activity of a BH it seems that one must wait and see what answers comes with time.
Juan_Rod
 
  • #28
DocN said:
Can one say that at the singularity, we would find such a transition from GR to quantum states? It appears that even the black hole itself is circular in shape--still a classical formation?

is it really an impossibility to say that classical and quantum physics are both one and the same; a thing of perspective rather than two different things? i am reminded of the geometrical classic Flatland and Spaceland books.
 
  • #29
when studying physics in the late '50s, some of us were pulling for Einstein and his unification theory but many were not amorous about the whole thing--quantum concepts ruled. Now, does it seem that string theory (which is quantum based) is the only old ,Einsteinian way?
 
  • #30
juan_rod:”My original question consisted of a general and or limited understanding of Quantum physics and the curvature of space-time. now you have introduced electrodynamics, how is this relevant to the properties of a BH?”

” it seems maybe, that i am trying to put things together in my own terms using only limited knowledge. thank you all for your help. Because no one fully understands the properties and the behavioral activity of a BH it seems that one must wait and see what answers comes with time.”

Do not wait. Do something that excite your curiosity and fit your knowledge.

Now I take a risk that DocN and Marcus again will laugh in me. I will be my own “interpreter”. However, it may be used as example what self-interference means (My brain as well as yours is natural realization of the quantum computer).

I assume that you started your steps in physics. You start very well. You try to understand roughly a general situation. Now you should find your very specific point. Try to make it as simple as possible. Then apply all what you know. If it is within study of gravitational interactions, remember that it should explain why our world is four dimensional with the Minkowski metric. You will not find the answer to that question in the “Hollywood movies”. The A. Einstein GR is the generalization of the Maxwell field theory. The field theories also are called Wave Mechanics (HJ formulation). You should know and understand electrodynamics, otherwise you have no chance. The general picture of the present status of classical electrodynamics as well as QED you may see in the enlightening discussion in size of photon particle session of Quantum Physics Forum.
As I mentioned already, your question about BH may be also connected with the problem of advanced and retarded solutions in electrodynamics. In addition, the physics is an empirical science. It have no ground without measurement theory. Here I have good news for you. The Measurement Problem in the non-relativistic limit is solved.
 
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  • #31
RandallB said:
“Quantum Gravity” - Fundamentally based a quantum approach, utilizing QM (its derivatives or equivalents) and uses the Standard Model including the idea of particle exchange of gravitons (yet to be discovered) to account for gravity.
I hope you don't mean that "Quantum Gravity" implies making use of gravitons. There are other approaches too, such as described in
R. Van Nieuwenhove, Quantum Gravity : a Hypothesis, Europhysics Letters, 17 (1), pp. 1-4 (1992)), or in Puthoff's polarizable vacuum concept. Such approaches are based on considering gravitation not as a fundamental force but as derived from modified quantum vacuum properties.
 
  • #32
DocN:” Can one say that at the singularity, we would find such a transition from GR to quantum states? It appears that even the black hole itself is circular in shape--still a classical formation?”

juan_rod:” is it really an impossibility to say that classical and quantum physics are both one and the same; a thing of perspective rather than two different things? i am reminded of the geometrical classic Flatland and Spaceland books.”

Let me give an example (and the additional argument that it is worth to know electrodynamics):
The peaceful coexistence of quantum and classical physics is well-known in the quasi-classical approximation. One obtains that according to W. Heisenberg UR number of particles is the self-adjoint operator with continuous spectrum (P.Carruthers, M. Nieto, Rev. Mod. Phys., 40,411
(1968)). Indeed, you should use non self-adjoint operators which are relevant in QM as was demonstrated by V.A. Fock many years ago.
 
  • #33
Why does the curvature of spacetime cause matter to experience gravity?
 
  • #34
Blackhaven said:
Why does the curvature of spacetime cause matter to experience gravity?

That was the central idea of the theory of general relativity that appeared in 1915. We have a whole forum at PF that is devoted to relativity (both special 1905 and general 1915). You might try asking your question in that forum.
 
  • #35
Blackhaven said:
Why does the curvature of spacetime cause matter to experience gravity?
Actually: curvature of worldlines would be better, since curved spacetime is a misnomer.
Since spacetime consist of events that combine a position and a time based on the state of an observer, the worldline of the observer is straight (by definition). The observer isn't a person, but the zero point of the frame of reference.
That's a free-falling observer. Seen from there other worldlines are curved, because of gravity.
The reason is - in my eyes- something different and the curvature is an outcome and not the cause.
(Personally I see gravity as an effect of interactions of 'parallel lightcones' that interact and deflect the other one, since there seems to be some kind of rotation with these cones.)
 

1. What is a black hole?

A black hole is a region in space where the gravitational pull is so strong that nothing, including light, can escape from it. This happens when a massive star dies and collapses under its own gravity.

2. How is quantum gravity related to black holes?

Quantum gravity is a theory that attempts to reconcile the principles of general relativity (which explains gravity on a large scale) with those of quantum mechanics (which explains the behavior of particles on a small scale). Black holes are important in the study of quantum gravity because they are regions of extreme gravity, where the effects of both theories are believed to be significant.

3. What is the curvature of spacetime?

The curvature of spacetime is a concept in general relativity that describes how mass and energy can bend the fabric of space and time. This curvature is what causes objects to move towards each other due to the force of gravity.

4. How do black holes affect the curvature of spacetime?

Black holes have an immense amount of mass and therefore create a significant curvature in spacetime. This curvature becomes infinitely strong at the center of the black hole, known as the singularity.

5. Can we observe the effects of quantum gravity and the curvature of spacetime?

Currently, we do not have the technology to directly observe the effects of quantum gravity and the curvature of spacetime. However, scientists use mathematical models and observations of black holes and other extreme objects in space to study these phenomena and make predictions about their behavior.

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