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But in this analogy, isn't the straight line possible to continue into … Paths that carry on indefinitely are called complete geodesics, and those that stop abruptly, incomplete geodesics.Geodesics can fail to be complete for a variety of reasons. Or, roll marbles at one end of a trampoline and see if you can determine, without looking, if a person at the other end is sitting on the trampoline or standing on one toe.What about binary systems where one member is a black hole formed from a collapsed star?

One cannot predict what might come "out" of a big-bang singularity in our past, or what happens to an observer that falls "in" to a black-hole singularity in the future, so they require a modification of physical law. This all leads me to think that when a neutron star converts to a black hole Neutron stars don't convert themselves into black holes. In late 1915, Albert Einstein published his first paper on the subject of General Relativity. The energy condition required for the black-hole singularity theorem is weak: it says that light rays are always focused together by gravity, never drawn apart, and this holds whenever the energy of matter is non-negative. I delete obvious spam, but other comments are generally approved.I mention this now just in case anyone’s wondering about the previous comment. And of course the reverse is true if the mass goes down.First, let’s talk about what’s happening right now, and then consider what happens if the Sun turned into a black hole.

Spacetime is stretched in this regard.

The event horizon is the "point of no return" around the black hole. )We’ll just have to agree to disagree at this point.All I’m saying is that the mass will be farther away from the earth due to stretching. Please report this behaviour to We're not around right now. The best answers are voted up and rise to the top As Earman himself notes, however, the theorem in question only predicts the existence of the second type of singularities - namely, those involving geodesic incompleteness and therefore b-incompleteness - without telling us more about their nature (p. There are many different kinds of singularities in science.In the context of a black hole, the center is said to be a gravitational singularity, because density and gravity are suggested to become infinite, according to the GR equations.GR says: when you have a lump of matter that's big enough, it starts to collapse into itself so hard, there's nothing to stop it. That’s why you can approach a black hole from ALL three degrees of freedom and get sucked in.


similarly small? star's mass compacted into the size of the plank length or something I read that matter encounters geodesic incompleteness in the singularity in an uncharged black hole. hole?, surely the core collapsed into something, just really small Singularity, as pointed out by Stan Liou (a note about If you pick two points on the sheet (like A and B in the figure which show part of unfolded cube), the geodesic is the shortest path connecting them, that is abscissa A-B. University of Richmond undergraduates are involved in all aspects of this research. In it, he described a picture of our universe as a 4-dimensional space with one time dimension, now referred to as a spacetime. But both space and time in the context of a black hole are very seriously warped.

I was in a “snarky” mood. In other words, a freely moving or falling particle always moves along a geodesic. Discuss the workings and policies of this site It seems like there is matter being added to the center, because they can grow in size and intensity, no?

Sign up Please beware of booking services soliciting your personal information for travel and accommodation bookings for AMSI conference or events. Geodesic incompleteness occurs when a space has "holes" in it, or if it is possible to "fall off the edge" of the space. Here is the null version: Learn more about Stack Overflow the company

One thing about the event horizon: once matter is inside it, that matter will fall to the center. So Ted’s right!No I never disputed that, Phillip.
)I think I know what you are saying, but it won’t affect the orbit of the Earth. The question is about classical gravity.

Other versions of the theorem involving the weak or strong energy condition also exist. Publish it somewhere, as it’ll be the most important result in general relativity in 70 years.

There are many versions. The center of mass of the black hole is farther away than the center of mass of the star.It’s due to the change of the geometry of spacetime.One of the properties of space time that is affected by energy-momentum is space length and curvature. I was watching a YouTube video on black-holes and there was a quip regarding black holes and their warping of space time, to the point where the narrator said something along the lines of This is more of a question for the Physics stack, but I'll give it a shot, since it's fairly basic.You need to understand something before we begin.

But the fact that I understood enough theoretical physics to correctly understand this point when I was five and you still don’t is disheartening.In case anyone’s wondering, I don’t have much of a comments policy, because I don’t get very many comments. And of course I’ll upload a video of this exact scenario someday.In the meantime, the field equations do support what I’m saying though.Do I understand correctly that you retract the ““spiral[ing] away in increasingly eccentric elliptic curves” language? could just fall from the surface of the sun to its center, you would travel a distance approximately equal to the radius of the sun.But if you could fall into a black hole, the distance would be many times as much. This is not because you can't move out fast enough, but because So, why the center of a black hole is called a "singularity"?

If geodesic paths through deep space fail to terminate in this way, it could indicate the universe is infinite in expanse, or that it is cyclic like the surface of the Earth, where travelling in one direction for long enough leaves you back where you started.Properties like having a black hole, or an edge over which an observer could fall are topological properties of the universe; That is, they describe what space “looks like” on a large scale.

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