By the way, apart from the fact that dark matter predictions have been contradicted by increasingly sensitive experiments over and over and over, there is another inconvenient piece of observational evidence: An analysis of stellar velocities at the edge of the Milky Way, published last year [1] shows that they are "Keplerian", i.e. following classical behavior without the influence of any purported dark matter. So e…
The possibilities for dark matter have shrunk
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Re: The possibilities for dark matter have shrunk
#12By the way, apart from the fact that dark matter predictions have been contradicted by increasingly sensitive experiments over and over and over, there is another inconvenient piece of observational evidence: An analysis of stellar velocities at the edge of the Milky Way, published last year [1] shows that they are "Keplerian", i.e. following classical behavior without the influence of any purported dark matter. So e…
We've also seen instances where visible "clumping" in a galactic disc correspond to differences in the rotation curves, which dark matter can't really explain. But this is still a topic of much debate. However, there's lots of good evidence for dark matter besides rotation curves of galaxies. For instance, models of galactic formation work a lot better with it than without it (without dark matter, as galaxies coalesc…
Re: The possibilities for dark matter have shrunk
#13By the way, apart from the fact that dark matter predictions have been contradicted by increasingly sensitive experiments over and over and over, there is another inconvenient piece of observational evidence: An analysis of stellar velocities at the edge of the Milky Way, published last year [1] shows that they are "Keplerian", i.e. following classical behavior without the influence of any purported dark matter. So e…
We've also seen instances where visible "clumping" in a galactic disc correspond to differences in the rotation curves, which dark matter can't really explain. But this is still a topic of much debate. However, there's lots of good evidence for dark matter besides rotation curves of galaxies. For instance, models of galactic formation work a lot better with it than without it (without dark matter, as galaxies coalesc…
I'm guessing gravito magnetism hasn't been included in those models yet.
Re: The possibilities for dark matter have shrunk
#14There is no dark matter in theories of superfluid quantum gravity. Dirac later went to Dirac sea. Gödel had already proposed dust solutions, which are fluidic. PBS Spacetime has a video out now on whether gravity is actually random. I don't know whether it addresses theories of superfluid quantum gravity. >>> "Gravity as a fluid dynamic phenomenon in a superfluid quantum space. Fluid quantum gravity and relativity."…
It doesn't, it talks about the possibility of randomness allowing gravity to be classical and not quantum. If my understanding is correct, the gist of it is that certain random fluctuations in gravity would prevent it from contradicting Heisenberg's uncertainty principle when interacting with quantum entities.
Re: The possibilities for dark matter have shrunk
#15So either they exist but are too rare for the experiment to see, or they are massive but not that massive*, or dark matter isn't WIMPs (or dark matter doesn't actually exist at all).
Re: The possibilities for dark matter have shrunk
#16Re: The possibilities for dark matter have shrunk
#17Earlier quoted context omitted.
We've also seen instances where visible "clumping" in a galactic disc correspond to differences in the rotation curves, which dark matter can't really explain. But this is still a topic of much debate. However, there's lots of good evidence for dark matter besides rotation curves of galaxies. For instance, models of galactic formation work a lot better with it than without it (without dark matter, as galaxies coalesc…
> For instance, models of galactic formation work a lot better with it than without it I'm guessing gravito magnetism hasn't been included in those models yet.
Re: The possibilities for dark matter have shrunk
#18Earlier quoted context omitted.
Hmm... you could probably still do a powered flyby though: https://en.wikipedia.org/wiki/Oberth_effect This is different from a normal gravity assist. Close to a black hole the gravitational field would be quite strong, making this potentially very powerful.
I love this human can-do attitude. Screw black hole radiation, distortion of space time fabric at its core, just lets use it as a mega slingshot!
Re: The possibilities for dark matter have shrunk
#19By the way, apart from the fact that dark matter predictions have been contradicted by increasingly sensitive experiments over and over and over, there is another inconvenient piece of observational evidence: An analysis of stellar velocities at the edge of the Milky Way, published last year [1] shows that they are "Keplerian", i.e. following classical behavior without the influence of any purported dark matter. So e…
We've also seen instances where visible "clumping" in a galactic disc correspond to differences in the rotation curves, which dark matter can't really explain. But this is still a topic of much debate. However, there's lots of good evidence for dark matter besides rotation curves of galaxies. For instance, models of galactic formation work a lot better with it than without it (without dark matter, as galaxies coalesc…
Re: The possibilities for dark matter have shrunk
#20Earlier quoted context omitted.
Hmm... you could probably still do a powered flyby though: https://en.wikipedia.org/wiki/Oberth_effect This is different from a normal gravity assist. Close to a black hole the gravitational field would be quite strong, making this potentially very powerful.
I love this human can-do attitude. Screw black hole radiation, distortion of space time fabric at its core, just lets use it as a mega slingshot!
https://www.youtube.com/watch?v=AGmTZeiCmJY
There wouldn't be much radiation unless the black hole were actively "eating" something, which a PBH in far solar orbit would not. That's part of what makes it hard to find and what makes PBHs candidates for dark matter: they're dark and don't do much unless something encounters them. There would be no net emission of Hawking radiation since the BH's Hawking temperature would be colder than the cosmic microwave background.
The hypothetical PBH that could be planet 9 would be about 2-3 Earth masses and about the size of a golf ball in terms of event horizon radius. You couldn't get that close to it without being "spaghettified" and added to its mass.
Probably the most valuable thing we could do with it is study it and use it as a lab to learn about quantum gravity. We could chuck small things into it with probes nearby to precisely measure the result, etc. All black holes we know about are far too distant to reach. Having one we could study would be huge.