I clarify my question: beyond the event horizon of a black hole, according to general relativity, the space-time flows faster than the speed of light. If it is the case, then, no information can be transmitted from here.

But then, if i drop an apple, say, in the black hole.

The black hole would then gain mass, and i could theorically mesure that gain with the event horizon radius variation and the attraction, meaning that the information of its mass and attraction change went from the center to get out of the event horizon.

In other words, that gravity information would have been faster than light?

How is that possible and where did i not understand something? (Just daydreamed about this stuff so maybe my question in itself is idiotic, sorry physicists)

  • Libra00@lemmy.ml
    link
    fedilink
    English
    arrow-up
    22
    ·
    7 hours ago

    Because light is affected by gravity but gravity isn’t. Gravity—the curvature of space-time—can’t stop changes in the curvature of spacetime from propagating outward. But also that information isn’t coming from inside the event horizon, it’s coming from spacetime around it.

  • CanadaPlus@lemmy.sdf.org
    link
    fedilink
    arrow-up
    11
    ·
    edit-2
    7 hours ago

    In this specific case, the gravity of the apple just never went away. It exerts one apple mass before it starts to fall, while it’s falling, and whenever it crosses the event horizon from your point of reference.

    Nothing is actually being “transmitted” per general relativity here. If someone were to jump in with some kind of gravitational wave generating device and send you a secret message from inside, that would be a straighter example. As I understand it that would not work; the waves follow null geodesics (light-type trajectories) and would be trapped with everything else. Which is weird, because spacetime is trapping itself, but deep physics is under no obligation to act normal.

    I clarify my question: beyond the event horizon of a black hole, according to general relativity, the space-time flows faster than the speed of light. If it is the case, then, no information can be transmitted from here.

    It’s a bit of a nitpick, but I’m not sure I’d use “flow” here. That makes it sound like it’s moving, while the Schwarzchild solution is actually static with respect to a properly chosen time coordinate (and without checking, probably the spinning and charged solutions as well). The spacetime is curved in such a way all timelike (c or slower) trajectories go inwards.

    • 𒉀TheGuyTM3𒉁@lemmy.mlOP
      link
      fedilink
      arrow-up
      4
      ·
      6 hours ago

      It’s a bit of a nitpick, but I’m not sure I’d use “flow” here. That makes it sound like it’s moving, while the Schwarzchild solution is actually static with respect to a properly chosen time coordinate (and without checking, probably the spinning and charged solutions as well). The spacetime is curved in such a way all timelike (c or slower) trajectories go inwards.

      Oh that makes sense. I though it was space time itself which was moving, bringing with it the objects on it. (probably had seen some illustration representing it like that)

      But yes the gravitational waves take is interesting, it burn my mind trying to imagine how to “trap” spacetime in itself.

  • Zoift [he/him]@hexbear.net
    link
    fedilink
    English
    arrow-up
    11
    arrow-down
    1
    ·
    8 hours ago

    Cause black holes don’t gravitate, but the event horizon does. Black holes dont really have volume in a way thats meaningful to us, but they do have a surface area, and thats what you can interact with.

    You’re correct anything past an event horizon cannot interact with us, for all intents and purposes it doesnt exist. So all the interactions you associate with a black hole are interactions with the event horizon itself.

  • AbouBenAdhem@lemmy.world
    link
    fedilink
    English
    arrow-up
    4
    ·
    8 hours ago

    You only know the total mass, charge, and angular momentum of the black hole—you don’t know how those properties are distributed inside the event horizon. You see the apple approach the horizon and the horizon expands to encompass the apple-black hole system, but that information isn’t coming from the singularity at the center—it’s coming from the horizon.

    • BombOmOm@lemmy.world
      link
      fedilink
      English
      arrow-up
      2
      ·
      8 hours ago

      Exactly, that information isn’t coming from inside the black hole. In fact it is the lack of information that tells us such things. We know the ratio between the lack of information (the event horizon) and the mass of everything inside.

  • TerminalEncounter [she/her]@hexbear.net
    link
    fedilink
    English
    arrow-up
    3
    ·
    8 hours ago

    The change in mass, electric charge, angular momentum are the only things that are detectable after the apple crosses the black hole - no hair theorem. As far as we know, no quantum information is recoverable. We don’t actually, like, see the apple ever cross the event horizon it’s a whole weird thing. The event horizon conceals all events from the interior of the black hole from the rest of the universe - we never see anything about the center of the black hole or any part inside it, ever. It’s all cut off.

    The additional mass that changes how much additional force there is due to gravity is communicated at the speed of light, no faster.

    There are interesting theories about black hole holography, universe holography brane vs bulk stuff, whatever.

  • floo@retrolemmy.com
    link
    fedilink
    English
    arrow-up
    2
    ·
    edit-2
    8 hours ago

    According to our current understanding of physics and technology, you can’t.

    Maybe that will change in in the future, but for now, sorry.

  • JohnDClay@sh.itjust.works
    link
    fedilink
    arrow-up
    2
    ·
    8 hours ago

    I have no idea. But maybe the gravitational location would appear to asymptotically approach the event horizon similar to how light from an object would appear to just approach the horizon and then stay there.