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Darren New <dne### [at] san rr com> wrote:
> Ha! You're teaching me as you go! :-)
Scratch that. It could be LOT worse. I could be this guy (worth at listen at
about 31:00):
http://www.thisamericanlife.org/Radio_Episode.aspx?episode=293
Also interesting/entertaining:
http://insti.physics.sunysb.edu/~siegel/quack.html
http://math.ucr.edu/home/baez/crackpot.html
- Ricky
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clipka escreveu:
> nemesis <nam### [at] gmail com> wrote:
>> Darren New escreveu:
>>> nemesis wrote:
>>>> kind of after image that seems to ever approach the event horizon
>>>> without ever touching it, but in reality the crossing of the EH
>>>> already took place and nothing of what happens in the inside is seen...
>>> Hmmmm.... I'll have to think on it.
>> I think it has something to do with the last photons coming out of the
>> object entering the EH are severely slowed down by the massive gravity
>> and only reach you after much more time than normal has passed.
>
> Yeah - interestingly, the distance between a point near the EH and a point far
> away is shorter when moving towards the EH than when moving away from it on the
> very same route...
So that's why light takes a lot more time to reach us and thus the after
image just before the crossing is visible. OTOH, time and space are two
sides of the same coin, isn't it?
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nemesis wrote:
> "We start with effects actually seen in the lab, which I think gives it
> more credibility than black holes"
>
> evidence.
The effects of what appear to be black holes are seen in astronomy. Just not
in the lab as such.
> If we assume blackholes exist, without much evidence so far,
A fair amount of evidence, actually.
> Perhaps the blackhole is then just a curve along
> this surface and the poor fellow ends up in another region of
> space-time.
Basically, yes. Some types of black hole structures are thought to work that
way. Like, a rotating black hole can be traversed like that without hitting
the singularity, supposedly.
It's all math, tho, with no actual physics evidence beyond what the math
implies. If reality isn't isomorphic to the math after all, it won't work.
--
Darren New, San Diego CA, USA (PST)
"Ouch ouch ouch!"
"What's wrong? Noodles too hot?"
"No, I have Chopstick Tunnel Syndrome."
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Darren New <dne### [at] san rr com> wrote:
> nemesis wrote:
> > "We start with effects actually seen in the lab, which I think gives it
> > more credibility than black holes"
> >
> > evidence.
>
> The effects of what appear to be black holes are seen in astronomy. Just not
> in the lab as such.
>
> > If we assume blackholes exist, without much evidence so far,
>
> A fair amount of evidence, actually.
Yes, but according to the article you linked, QM physicists are giving another
explanation for the same effects without the paradoxes blackholes carry, the
same ones we were avidly discussing about previously: the "lost information"
and the "after-image" effect of something crossing the EH as seen from an
external observer. Of course, they are trying to explain it by relying on a
supposed dark matter star that has never been detected before either. :P
Surely the Dark side is very sneaky!
OTOH, will we ever witness such object, blackhole or dark matter star? Such
humongous gravitational force surely has many objects orbiting it,
"overcrowded" as clipka mentioned, and most of it being gas and stars, so what
is the chance of seeing what isn't supposed to be seen except against a clear
starry background?
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Darren New <dne### [at] san rr com> wrote:
> A fair amount of evidence, actually.
Absolutely fascinating:
http://www.eso.org/public/outreach/press-rel/pr-2008/phot-46-08.html
- Ricky
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triple_r wrote:
> http://www.eso.org/public/outreach/press-rel/pr-2008/phot-46-08.html
Kewl. I was thinking of this one.
http://en.wikipedia.org/wiki/Cygnus_X-1
--
Darren New, San Diego CA, USA (PST)
"Ouch ouch ouch!"
"What's wrong? Noodles too hot?"
"No, I have Chopstick Tunnel Syndrome."
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Darren New <dne### [at] san rr com> wrote:
> triple_r wrote:
> > http://www.eso.org/public/outreach/press-rel/pr-2008/phot-46-08.html
>
> Kewl. I was thinking of this one.
> http://en.wikipedia.org/wiki/Cygnus_X-1
Convincing evidence, but I'm a sucker for the visually spectacular ones:
http://en.wikipedia.org/wiki/Elliptical_Galaxy_M87
- Ricky
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"triple_r" <nomail@nomail> wrote:
> Darren New <dne### [at] san rr com> wrote:
> > A fair amount of evidence, actually.
>
>
> Absolutely fascinating:
>
> http://www.eso.org/public/outreach/press-rel/pr-2008/phot-46-08.html
Yes. Look the last video, it's a journey to the center of the galaxy through a
multilayered collection of ever zooming galaxy shots. It ends with both the
collected frames aquired over 16 years and accelerated by a few million times
and a CG detailing what's going on.
Truth be told, I don't think the video gives the exact scale of the thing. I
mean, I thought the central blackhole, or whatever it is those stars are
orbitting around, would be much bigger. Yes, I know it's hyperdense, but even
still...
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> Depends on definition if speed, but as it is usually specified based on
> the
> observer's timeframe: Yes. Gravitation near a black hole is so strong
> that -
> from an observer's POV - through time delation and the warping of space it
> causes "that poor old sod over there" to slow to a halt.
I always thought that it could be possible to go forward in time by some
arbitrary amount just by making a close orbit around a black hole. The
closer you go, the more time you can jump forward. So just type in the year
3050 to your ship, it fires you off towards the nearest black hole, and a
few months later you return back towards Earth in the year 3050 +/- a few
months ;-)
Or doesn't it work like that?
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clipka <nomail@nomail> wrote:
> Well, from an outsider's perspective - given that everything falling into the
> black hole comes to a standstill at the EH...
Slowing down asymptotically is not the same thing as being stopped.
Also, as I have been saying, since it will emit constantly less and less
photons, which are more and more red-shifted, at some point it will be
practically impossible to observe the object. It will just fade to black.
--
- Warp
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