
Black Holes and Hidden Dimensions 200
Slackware Geek writes "It is being reported in the Nature Science Update that a new observitory being built in Argentina to study cosmic rays could detect extra hidden dimensions if they exist. 'Cosmic rays could find holes in Standard Model of particle physics ...If the Universe contains invisible, extra dimensions, then cosmic rays that hit the atmosphere will produce tiny black holes. These black holes should be numerous enough for the observatory to detect.'"
Miniature Black Hole (Score:4, Interesting)
Re:Miniature Black Hole (Score:4, Informative)
Yes they would be detected by the shower of particles produced by the (very rapid) Hawking radiation decay of the black holes. Its in the article except they didn't mention Hawking radiation by name.
Re:Miniature Black Hole (Score:5, Informative)
>evaporating hole, or is it detecting other effects?
Yes, this is essentially what happens. The decay is actually somewhat more complicated; there is an initial "balding" phase in which the black hole loses its hair, along with a "spin-down" phase... after this, there's a very quick evaporation with high sphericity. Go to http://arxiv.org and search for "black hole production"; some recent papers by Giddings have details. It was believed for a while that the cross-section is geometric, which would lead to a good chance of detecting these in the next generation of colliders if large extra dimension (LED) models are correct. A paper by Voloshin indicates, on the other hand, that the cross-section is really exponentially suppressed by the black hole action. I'm not sure this has quite been settled completely.
The basic idea behind all this, by the way, is that there may be extra dimensions which are large compared to the Planck scale (up to a millimeter in size - that's about as far as gravity has been probed!). Gravity would be a field in "the bulk", that is it propagates in all the dimensions, but the standard model fields are localized on some sort of 4-dimensional "brane." There are actually a couple of different models with large extra dimensions - one is the ADD model (Arkani-Hamed, Dimopolous, Dvali) and another is the Randall-Sundrum or "warped extra dimension" model. Searching on arxiv.org for any of these names should get you links to the papers.
The basic reason for looking into all of this is the hierarchy problem, namely that the gravitational force is far weaker than the other forces. The electroweak scale is on the order of one TeV (= trillion electron volts, where one electron volt is about 1.6*10^-19 Joules). Gravity, on the other hand, is associated with a much higher energy scale. To explain this, the ADD model proposed that maybe the fundamental Planck scale is actually on the order of a TeV, like the electroweak scale. In other words, they solve the hierarchy problem by saying there is no hierarchy. Gravity propagates in more dimensions, so that its effect in our four-dimensional part of the universe looks much weaker. The other fields are localized in such a way that this ratio doesn't take any effect for them, so we see them at the "true" Planck scale on the order of a TeV.
It just so happens that the TeV scale is what we're looking at with current colliders, which is why there's so much interest in this lately. But cosmic rays give an alternate approach. Keep in mind that these ideas are very speculative, but still worth looking into.
Re:Miniature Black Hole (Score:2)
I find that amazing! Now if the theories allowed for those extra dimensions to periodically grow to sizes large enough to swallow single socks and small toy cars, I'd call it a very significant development.
Seriously, I'm amazed that gravity hasn't been experimented with on smaller scales. Would that be something that requires zero-g and objects in a vacuum, or do you get other problems, like electrostatic/electromagnetic forces or even gravity of surrounding objects on those scales that make gravity difficult to measure directly at that resolution?
Re:Miniature Black Hole (Score:2)
>experimented with on smaller scales. Would that be
>something that requires zero-g and objects in a
>vacuum, or do you get other problems, like
>electrostatic/electromagnetic forces or even
>gravity of surrounding objects on those scales that
>make gravity difficult to measure directly at that
>resolution?
Apparently the current limit is now somewhat less than a millimeter, but still on the order of a millimeter. Yes, it is very difficult to test. A group at the University of Washington has developed small-scale gravity tests; see http://www.npl.washington.edu/eotwash/shortr.html for an explanation.
Basically, you have the right idea; it's hard to screen out all of the other effects at a scale that small, which is why studies at the millimeter scale are extremely difficult.
Must resist... (Score:4, Funny)
Moderators, punish me now.
Re:Must resist... (Score:3, Insightful)
Argentina didn't come up with this science project - the world did. It's an international collaboration of dozens of countries and about 300 scientists worldwide. Argentina was chosen as the southern site of the array due to the location - the array consists of a flourescence detector, which requires stable weather and clear air. The northern site is still under discussion, though it seems most likely to be in Utah (along with the dozen or so other cosmic ray observatories in Utah).
The Auger collaboration is then completely distinct from Argentina's government, so we don't really worry about the governmental problems except for the problems they cause our friends down there and the Argentine portion of the collaboration.
Re:Must resist... (Score:2)
Ahhh. Hopefully, it'll be a pretzel-proof dimension.
Re:Must resist... (Score:2)
No, that's American presidents. They'd be better off looking for a dimension full of spanish speaking Alan Greenspan clones willing to run.
(Note to anybody who takes that wrong - America had Herbert Hoover for their financially inept leader, and in comparison Clinton *and* Bush look good, either choking on a pretzel or choking an intern with his...)
--
Evan
Re:Must resist... (Score:2)
Better than J. Edgar Hoover. At least Herbert wore men's clothes, AFAIK.
`Width' of a single atom (Score:2, Interesting)
There's more information about the Pierre Auger Project here [auger.org].
Re:`Width' of a single atom (Score:1)
Re:`Width' of a single atom (Score:1)
Re:`Width' of a single atom (Score:1)
Re:`Width' of a single atom (Score:1, Flamebait)
Do you have a problem with the concept of 'width of a single atom' or what are you saying? Or perhaps radius would be a better word?
Width or radius, neither would matter. "During" the big bang (0 - 5 seconds for example), there were no atoms. The universe was far too hot for any to form.
Re:`Width' of a single atom (Score:2)
"Extra" (Score:1, Interesting)
Any other dimensions that are there are already existing, and are not "extra" or in addition to whats in the universe.
Re:"Extra" (Score:1)
Black holes... (Score:1)
Re:Black holes... (Score:1)
Never expected to read that story (Score:1)
circular/spherical space-time (Score:5, Insightful)
Think of it... In a world where light traveled in a fixed radius of one meter, you would see the back of your head if nothing is in the way. And, it would seem, that your head is 6.28 meters away from you. Problem is, you wouldn't be able to see beyond that one-meter radius circle. Now, what if that radius was shrunk to the atomic level... you wouldn't be able to see beyond the circle(sphere?) that the fixed radius spans. Obviously, your eye is way too large to detect that kind of precision.
Thoughts anyone?
Re:circular/spherical space-time (Score:1)
Re:circular/spherical space-time (Score:3, Informative)
Think of what the author said in terms of particle physics. He/She looked into a world where photons moved in a circular fashion. If the radius was big, it'd be just like our current universe. If it was small, we wouldn't be able to see much beyond our point of view.
What I'm trying to say is that photons move in the three orthonormal dimensions, and change coordinates with respect to the fourth dimension. Duh. Everyone knows that. But what if there were some other particles (Higgs boson, perhaps?) that function similarly, only on these "curled-up" dimensions? The reference to the website was made simply to introduce the reader to a circular/spherical coordinate system. My comments following the link asked the reader to reduce the radius of said coordinate system.
Re:circular/spherical space-time (Score:3, Funny)
Correct me if I'm wrong... we can't see beyond our point of view now. That's why it's a point of view.
Re:circular/spherical space-time (Score:1)
Re:circular/spherical space-time (Score:1)
On the universal time scale, what is 'sudden'
Last I heard, and I haven't payed attention in about 2 years, evidence was suggesting that Hubble's constant was getting larger over time
Re:circular/spherical space-time (Score:2)
The only other possibility I could imagine is the size of the universe divided by the speed of light, which is something like the age of the universe. That of course, would have been sudden when the universe was celebrating it's Planck's time birthday, but pretty darn sluggish today.
Re:circular/spherical space-time (Score:1)
I appologize for being a smart ass, I should have just said no.
Interesting theory, but practice? (Score:1)
Maybe I'm missing something...
Re:Interesting theory, but practice? (Score:1)
Re:Interesting theory, but practice? (Score:2)
Now, a slightly more interesting question is why the extra dimensions would lower the threshold of singularity formation. Do they make space more compressible by giving it more room to flex in or what?
Could help in validating string theory? (Score:1, Insightful)
Of course there are! (Score:2, Funny)
Re:Of course there are! (Score:1)
It has something to do with static electricity. It is interesting to note that while man has found a way to artificially create this phenomenon with a major appliance, dogs are able to do it on their own. Dave Barry wrote a great article [geocities.com] about this a few years ago. To quote:
Re:Of course there are! (Score:1)
Experimental proof for string theory (Score:5, Informative)
This would be a nice feather in the cap of string theory, which to this point does not have any experimental observations to back it up.
One of the predictions (or you could say requirements) of string theory, is that the universe contains a total of 11 space-time dimensions, 7 of which are "curled-up" and are extremely tiny. Every time you move, you pass through the entire universe in each of these 7 dimensions, although your position in the 3 "enlarged" dimensions hardly changes. The interesting thing is that a guy predicted these extra dimensions way back in the 1910's, and was ignored for about 50 years. Experimental evidence on the side of string theory (or as they're calling it now, M-theory) would go a long way towards convincing the experimental physicists that all these theoretical physicists aren't off their rockers.
Re:Experimental proof for string theory (Score:2)
Actually, String theory has moved to M-theory, and involves "super strings" and membranes. I've read many books on the subject... most of them have taken a long time to read, i.e. read a few pages, think about it for a few days, go back...
Anyhow, some links:
My take is that, as has been said before, the world consists of 11 dimensions. There are actually many super-string/m-theories, but they are not contradictory, kinda like different views of the same thing.
A main problem with these theories is that there are many (infinite?) solutions the math sets that descibe them.
A 'string' in the theory is like a circular guitar string that is taunt... it has certain modes of vibration, each mode representing a certain type of particle.
Also, there are different types of strings... strings that are self connecting, open string, string that loop around more than once...
Ok, that probably didn't clear anything up...
Re:Experimental proof for string theory (Score:2, Interesting)
Then again, with the SSC canceled, maybe not . . .
Re:Experimental proof for string theory (Score:1, Insightful)
Re:Experimental proof for string theory (Score:3, Interesting)
Direct evidence for string theory at any point in the near future is highly doubtful. We just can't get good evidence of such high energy scales. We could see associated effects, like extra dimensions or supersymmetry, but those don't necessarily imply string theory.
What is the Evaporation Process Then? (Score:1)
Re:What is the Evaporation Process Then? (Score:1)
Re:What is the Evaporation Process Then? (Score:1)
event horizon you get particle-antiparticle
creation. If memory serves the antiparticle is absorbed by the black hole ( reducing it's mass)
and the particle is emitted.
http://wwwusr.obspm.fr/admin/seminaire/chalonge
Re:What is the Evaporation Process Then? (Score:2)
An alternative interpretation (and the more popular one), is that virtual particles of positive and negative mass enegries are created near the event horizon, and the negative mass energy particles fall into the black hole, while the positive mass particles escape. Ordinarily such virtual particles are created all the time and quickly annhilate each other back out of existence, but in the rare case that one crosses the event horizon they can't come back together and thus one becomes a real particle. Since we assume that negative mass energies can never be truly realized, only positive particles will ever escape.
In both cases the blackhole loses mass and appears to emit particles. In fact, there is nothing about Hawking radiation that makes either interpretation more valid than the other.
New Observatory (Score:4, Funny)
Cosmetic rays will indeed prove that the univers is shallow and one dimensional.
A bit more on the multiple universe theory... (Score:4, Informative)
Re:A bit more on the multiple universe theory... (Score:3, Informative)
The idea of extra dimensions, on the other hand, simply implies that there are more spatial dimensions in the universe than it appears. Of course, there seem to be 3, plus one time dimension, but it's possible there are others that are visible on in small-scale (high-energy) effects. This has nothing to do with other universes.
Re:A bit more on the multiple universe theory... (Score:2)
Ordinary non-relativistic quantum mechanics, on the other hand, maintains the idea of a separate time dimension while treating spatial coordinates as operators. It's only in relativistic QM, and quantum field theory (QFT), that quantum effects and special relativity are reconciled. But this does not take general relativity into account, so QFT actually maintains the idea of global (but not absolute!) space + time coordinates, in a certain sense. We can't determine the position of a particle exactly, however (and there are problems with constructing "time-of-arrival" operators... but I'm getting in over my head with that comment.)
Also, there are elementary particles in quantum physics. We might never be completely sure that at some huge energy scale, the particles we think are elementary are not composite, but there are certainly particles which, from the standpoint of current theory, seem to be elementary.
Re:A bit more on the multiple universe theory... (Score:1)
Sadly, it is not up on Discover.com's website yet so I can not provide a link. It is in the latest (February 2002) issue and I highly reccomend it--it definitely re-piqued *my* interest in astrophysics...
Re:A bit more on the multiple universe theory... (Score:1)
Interesting, sorry about the error... I read a lot of science articles but on a very broad range of topics so I get things confused now and then. Too bad you can't edit posts... shucks.
Also, I actually have the newest Discover sitting about four feet from where I'm sitting but I have not yet had the chance to read the cover article. (I like to save the most interesting looking for last.) However the article on the new type of holography is absolutely not to be missed either, nor is the article on savants. Got a bit off-topic there... like I said, I have a varied taste.
Random thought: no dimensions, no space (Score:3, Interesting)
Why not go for a dimensionless graph universe of immutable particles/nodes representing conserved quantities? In addition to mass particles, have energy particles, charge particles, etc. (these are bad examples, of course; given the mass-energy equivalence, a "particle" of kinetic energy would have to be a compound entity). Just set up the rules to define the various types of connections, which have variable quantities (or possibly, are made and broken; however it works out to be simpler) and for determining the probabilities with which they may change from one arrangement to another. To put it in programming terms, take the data out of the particles, and put it into the relationships between them.
It wouldn't be easy, it might be useless, but I know it would at least give me fewer headaches to start with a clean slate than to twist the classical ideas of space all out of shape.
You can certainly have a graph system that behaves identically to a spacial system (though a graph system of Newton's physics would certainly be uglier than his elegant concepts), and it would lead to fighting fewer spacial preconceptions that give people such a miserable time keeping up with modern physics.
Anyway, just a random thought.
Re:Random thought: no dimensions, no space (Score:2)
Re:Random thought: no dimensions, no space (Score:2)
Matter is just a very tight bundle of energy.
Matter is also just the property of having momentum and being subject to gravity. It's just a 'mode' of being...
Hmm... personally, I think it is really interesting to consider how our modes of observation effect our possible theories. What if we were being that 'saw' in terms of microwaves? How would our theories be different? I suppose it would all ultimately lead to the same place.
Re:Random thought: no dimensions, no space (Score:3, Informative)
Re:Random thought: no dimensions, no space (Score:2)
Quantum mechanics is one way to fudge the matter by saying that we know how the particle is distributed over space, assuming space really had geometric (point-like) positions. String Theory takes this farther by building a structure for the universe where no objects are ever point-like. We believe that this can work because non-point-like objects can be described by the volume of space they take up, but it's probably not the best way.
Many of us in physics would love a system to represent the world that physics actually takes place in, but we just don't know how to do that so we continue to work in increasingly awkward point based geometries and try to figure out what physics looks like when we impose our artificial framework on top of it.
Re:Random thought: no dimensions, no space (Score:5, Interesting)
No, not exactly, though this is a common misconception.
Heisenberg's Uncertainty Principle has nothing to do with the act of observation. The actual uncertainty is fundamental to the quantum model. It's not that you can't measure both the position and the momentum at the same time, it's more that the particle's wave aspect cannot be constrained by both 'measurements' at the same time. Think of the particle like a water balloon on the position/momentum graph: if you compress it in one direction (measuring position) it spills out in the other (uncertain momentum).
The fun part is that you can actually use the uncertainty principle to make more accurate measurements. An experiment that was done years ago in Australia proved this. The idea is that a photon travelling here from a distant star has a very narrowly defined transverse momentum: it's heading almost directly towards us, so the uncertainty in its side-to-side momentum is directly related to how much space it takes up in the sky. (Since that defines the range of angles the photon could arrive from.) Since the transverse momentum is highly constrained, the transverse position must be highly spread out. So in theory the photon could be seen as a paper-thin pancake several miles across.
Now, from the standard double-slit experiments, you get an interference pattern as long as there is a possibility of the photon 'hitting' both slits at the same time. In this experiment, the slits were replaced with radio telescopes on train cars, on a long straight section of track. (Hence why this was done in the Australian outback.) So long as the telescopes are closer together than the uncertainty in the photon's position, you get an interference pattern. Once they're further apart than that, you revert to two seperate streams of photons.
So, you slowly move the telescopes apart, watching the star, until the interference pattern disappears. Presto, you have the 'size' of the photon, which gives the uncertainty of its transverse position. Back-calculating throug Heisenberg's inequality gives you a limit on its transverse momentum. And that gives you a good idea of the 'size' of the star in the sky, in fractions of an arc second.
This has been done, and gave answers that agreed with other observations of the stars. So the Uncertaintly Principle has, in this case, improved the accuracy of measurements.
And demonstrated that the HUP is a lot more fundamental than what you said. Particles simply do NOT have "simultaneous exact position and momentum."
-- Bryan Feir
Argentina -- a bad idea. (Score:3, Interesting)
Not really (Score:3, Informative)
The observatory is actually in a place along the Chilean border called Malargue (you'll never find it on a map - ever) which (according to all my friends there) is a little bit worried about the goings on in BA, but life, for the most part, seems normal.
Seriously, the government overhaul is the least of the Observatory's problems - the biggest problems we have are getting things in and out of the country. International customs is horrible. Ever try to explain to someone what a photomultiplier is? Or how something that looks like a very big light bulb is worth $1000?
Re:Not really (Score:1)
Re:Not really (Score:2)
Ezeiza's inspection really has never been anything at all to me - they don't even LOOK at anything non-Argentines bring in, because they don't care - all they're checking for is an excess of the import duty-free limit (which, I've been told, can easily be avoided, like all taxes in Argentina - which is one of their problems). No one has ever even spoken to me in that line - it's just hand over import form, smile, nod, and walk.
The Recoleta didn't really impress me. I was also extremely disturbed by the number of cats in that graveyard. That's just plain weird. The area was nice, but seemed a little too touristy. Just my opinion though. I love Malargue, though (where the project actually is - in the Mendoza province). It's like a jump back 50 years in time, and the people are all incredibly friendly. The only problem I have is that the geography is so incredibly boring, as Argentina, save for the Andes, is simply ridiculously flat.
Possible source of cosmic rays (Score:2)
Re:Possible source of cosmic rays (Score:4, Interesting)
Empty-space acceleration would have to be massive to counteract the utterly huge deceleration caused by energy loss in galactic/extragalactic magnetic fields, interaction with the interstellar medium, and, most importantly for extreme high energy cosmic rays (UHECRs), the GZK effect - photopion production by interaction with the cosmic microwave background radiation. It's simply not possible to accelerate particles like this in empty space - we would've seen it already in particle accelerators.
Seriously, physicists right now have no idea how these particles are accelerated. Supernovae? Not nearly enough energy, by any stretch of the imagination - fundamental arguments like conservation of energy kill you far below the 10^20 eV limit. Gamma-ray bursts? Maybe, but the distribution of cosmic-rays doesn't agree with GRBs as a possible source. Extragalactic? Not unless you throw away basic physics and ignore the GZK effect - there's no way they could propagate that far.
Basically, the one question that there have been tons upon tons of papers in the recent literature for is "where is this gigantic particle accelerator nearby us?"
Re:Possible source of cosmic rays (Score:2)
I dont know where it is, but its probably run by some mice.
And furthermore.... (Score:4, Funny)
yes!! (Score:1)
Must resist... (Score:1)
(Humor. Not troll.)
Why should this happen? (Score:1)
Re:Why should this happen? (Score:1, Informative)
Re:Why should this happen? (Score:3, Informative)
Let me try to outline what's going on: I'm getting this from "Black hole production in TeV-scale gravity, and the future of high energy physics" by Steven Giddings (hep-ph/0110127 on arxiv.org). It's a nice article to start with, if you want to dig into the literature on this.
(By the way, this is using the "warped" extra dimension model but the general ones are similar.)
The Planck mass in D dimensions is M_p^(D-2) = (2 pi)^(D-4) / (4pi G_D) with G_D the gravitation constant. It turns out (M_4 / M_p)^2 = (M_p)^(D-4)V_{w}, with V_{w} the "warped volume" of the extra dimensions. (I'm not being very rigorous here; in fact this is how the volume is defined, and the ratio is given by a certain integral in terms of the warped metric.) This is essentially a sort of "Gauss law" argument, over the extra dimensions.
Now, let's consider a black hole with radius r_h much less than the geometrical scale R_c of the extra dimensions. It turns out that for a black hole of mass M, spin J, in the J = 0 limit, we have r_h = 2 [C M / M_p^(D-2) ]^[1 / (D-3)] where C is some constant in terms of D that I don't want to bother writing. The Hawking temperature looks like T_h = (D-3)/(4pi r_h). This description is valid roughly for M_p > 1.1 TeV -
Black hole cross-section was assumed to be geometrical (pi (r_h)^2), but as I mentioned in another post this is questioned (look up papers by Voloshin - but Giddings questions those), and there may be an exponential suppression. Anyhow, the important point is that, once you take all this into account, you get that the cross section sigma grows when D is larger, i.e. you don't have to put energy into as small a region if there are more dimensions.
Bug (Score:5, Funny)
The problem is that
"The result of casting elementary particles outside the inheritence hierarchy is undefined."
The Manual 4.1, chapter 7 cited in Universe(3)
More info on the Observatory (Score:5, Interesting)
Forgive me for going completely crazy replying to everyone, but this is just too cool.
OK, so long as people promise not to Slashdot the server (heh, that was dumb) for anyone who wants more information, go to the main Auger website [auger.org], or for even cooler information, go to the Auger site in Argentina [auger.org.ar].
Auger is actually a very interesting project, and it's not like anything you'd ever think of - it's a 1600 km^2 array of water Cerenkov detectors (10 cubic meters of water) spaced 1.5 km apart - the picture in the article is of the flourescence detector, which is more like what you think of for a standard detector, but due to the limitations of the flourescence method of detecting cosmic rays, its duty time is only 10%, as opposed to the 100% of the surface array.
The project is proceeding along... pretty well. We've basically finished the Engineering Array, a small-scale testbed to find all of the design flaws in the initial project (and boy, did we find them) and we've detected some cosmic rays which we believe to be ~10^19 eV. We've also demonstrated the hybrid design as well (events where the flourescence detector triggers as well as the surface detector).
The black hole stuff isn't the important goal of the project - the goal is to elucidate the spectrum of cosmic rays above 10^20 eV, because we have no idea where those particles come from - all of basic physics says they can't exist. This is one of the big questions in astrophysics in recent years, up there with gamma ray bursts and odd quantum states of matter.
It's way cool. And not just because I work on it...
Re:More info on the Observatory (Score:3, Informative)
That, and for those in the cosmic ray research area, this observatory is so critical. At the last ICRC in Hamburg, the rappoteur (sp?) in the "Cosmic Rays >10^19 eV - Upcoming Projects" area said that the one thing that the recent data underscored most significantly is how much Auger is needed. I couldn't agree more - the two largest current observatories, AGASA and HiRes, both have markedly contradictory data, with no clear way to resolve this difference! Previous observatories tend to somewhat agree with HiRes (Haverah Park), but that's iffy at best, as AGASA has some fundamental advantages over the HiRes design. Therefore, it seems extremely unlikely that the international collaboration will let the project suffer for any troubles that the Argentines have.
It is a little unnerving, though, because for me, personally, the most promising people that I work with down there are the Argentines (and one Frenchman to be left unnamed) - the prospect of losing them due to lack of funding is really worrying. However, it should be noted that the beauty of international collaborations and a small field of study is that you get people moving cross countries to work on a project. There's already one Argentine who just got his PhD and is headed to Colorado, so we definitely won't lose him.
It should be noted - strongly! - that the observatory still is in the construction phase. 1600 autonomous water Cerenkov detectors are difficult - and expensive - to build! We're still working out a lot of the kinks in the design, so right now a lot of the work is being done off-site, though there is PLENTY of work being done on-site as well.
Um... (Score:1)
Someone's been smoking a *little* too much Argentinian "coffe".
Visualize the hypercube... (Score:1)
Reason: Please use fewer 'junk' characters. Fucking lame-ass filter.
1.) Visualize a line. It has one dimension.
2.) Now add another dimension. Visualize a square. It has two dimensions.
3.) Now add yet another dimension. Visualize a cube. It has three dimensions.
4.) Now add another dimension. Visualize a hypercube. It has four spatial dimensions. Kinda fucks with your head doesn't it? Stuff like this is REAL bad to think about if you can't sleep, by the way.
Tim!
Re:Visualize the hypercube... (Score:2, Informative)
Quick background info on him. He has worked on texture mapping for quite some time now. Created such things as "Perlin Noise [kenperlin.com]." Here is a good example [nyu.edu]. He also got an oscar [nyu.edu]for this work.
I hope this all helps you visualize the hypercube now.
Re:Visualize the hypercube... (Score:2)
T
Re:Visualize the timecube... (Score:2)
+ Wierd for sure
Jaysyn
What if one uncurls? (Score:2, Interesting)
What the universe be like if we suddenly got some osrt of extra spacial dimension?
Or going the other way, would there ever be any risk of one of our current spatial dimensions curling up?
Yes! (Score:2, Funny)
I shall be The One!
Can't wait. (Score:2, Funny)
cosmic rays trillion accelerators (Score:3, Informative)
energetic than the largest human accelerators.
The tradeoff is "luminosity". You may only see a
few of the highest energy cosmic rays in a year,
while you want zillions of hgih energy particles
in an accelerator.
Entropy and Temperature of these black holes. (Score:2, Informative)
Re:antimatter particles (Score:1)
Re:antimatter particles (Score:5, Informative)
Reply to parent: nothing. antimatter is not a very exotic thing, normal matter with reverse charge reverse spin. Once in the blackhole there is no telling whether what fell was matter or antimatter, they all behave the same (increase black hole's mass, that is, and nothing else.)
Re:antimatter particles (Score:1)
Re:antimatter particles (Score:2, Informative)
How hawking radiation actaully occurs is something I understand but do not grok. I can't really explain from ground up, since I'm not an expert. I'll give it a try but don't quote me on this.
The whole process is lending a bit of energy from nothing, such that it won't violate conservation of energy by being strictly in limits of uncertanity part of uncertainity principle. Sometimes this energy is borrowed in form of two photons with opposite momentum, some times a particle-antiparticle pair. You have to pay back soon what you have borrowed, but sometimes the blackhole gets greedy and swallows either one of your photons or you particles. When the death calles for destruction, black hole no option but to pay back what debt it has inherited. So far, so good. Now here is the part I don't really understand (I can explain preceeding part in techincal terms and in detail if you prefer, but not this part) but accept: black hole for some reason pays the debt for the pair, not only the one it has assimilated. If it does this, the other particle, photon, whatever is free to roam the universe.
Re:antimatter particles (Score:2)
>matter with reverse charge reverse spin. Once in
>the blackhole there is no telling whether what fell
>was matter or antimatter, they all behave the same
>(increase black hole's mass, that is, and nothing
>else.)
Sorry for being so pedantic, but they also affect its charge and angular momentum. So you're essentially right, except that if you know, for instance, that either an electron or positron fell into a black hole, and you could somehow monitor its charge, you could distinguish which.
Re:antimatter particles (Score:1)
These are two thing I (as a chemical engineer) "know" about black holes which conflicts with each other. I have always wondered this, which one is correct so thanks for giving me a chance to ask:
1 - If a charged particle drops into a black hole it has to change black hole's chargebecause of conservation.
2 - It also happens to be the case that no information can be obtained from (if you excuse the term) "inside of" event horizon, we can determine mass changes and angular momentum changes because it changes the shape and size of event horizon. If something happens to the black hole that doesn't change the properties of its detectable "border", event horizon, we aren't supposed to be able to detect that.
So how can charge be preserved if it doesn't affect event horizons properties? How can you tell total charge of a black hole?
Re:antimatter particles (Score:4, Interesting)
So, to explain: black holes have three properties. They're the universe's most massive particles in that respect.
Charge does affect the event horizon's properties, basically in the same way that angular momentum does - it alters it massively. You can get very weird black holes, including ring singularities instead of point singularities (black hole donuts!).
In reality, it's very difficult to charge up a black hole. Most of the matter falling in is neutral, and a buildup of one charge will result in a preferential draw of the other charge (opposites attract, y'know) and therefore, an overall neutral black hole. In falls an electron, and a proton is drawn preferentially over another electron. You also need a ton of charge to change the event horizon significantly - but in theory, it is possible to tell.
Re:antimatter particles (Score:2)
>it has to change black hole's chargebecause of
>conservation.
This is correct - charge, momentum, and angular momentum are all globally conserved, so far as we can tell.
Note that "mass" is not *really* conserved - this is especially obvious in certain decays of elementary particles (i.e., electron+positron -> photon+photon; you end up with 0 mass). What *is* conserved is the energy-momentum four-vector (E, p), and for any one particle E^2 - p^2 = m^2. Mass only is conserved in the nonrelativistic limit. But I digress...
>2 - It also happens to be the case that no
>information can be obtained from (if you excuse
>the term) "inside of" event horizon,
This is basically true: no information is obtained. It is said that "black holes have no hair." But they do have a few properties - charge, mass, and angular momentum are essentially it. (Temperature and entropy also, but these depend on mass.)
>determine mass changes and angular momentum
>changes because it changes the shape and size of
>event horizon.
This is somewhat true; I'm not sure I would have expressed it in terms of "shape and size." I have to admit my knowledge of the black hole solutions in general relativity is fairly rudimentary, so I'm not sure in exactly what way that is true, but I think it is. There is a metric - called the "Kerr black hole" - that describes black hole solutions that spin; I think when they have charge there is another term. But the thing to note is that the metric of spacetime is actually different for different values of black hole spin, or charge. You'll also see a change in the electromagnetic potential (phi, A) outside the black hole for the charged case. So there are external effects.
>So how can charge be preserved if it doesn't
>affect event horizons properties? How can you
>tell total charge of a black hole?
The simple answer is: Maxwell's equations. Anything with charge, even a black hole, will change your electromagnetic potentials.
In other words, black holes tend to wear their charge, angular momentum, and mass "on the outside", in some sense.
Re:antimatter particles (Score:4, Informative)
Schwarzschild metric: mass only
Kerr metric: mass+angular momentum
Reissner-Nordstrom metric: mass+charge
Kerr-Newman(sp? on second): mass+charge+angular momentum - i.e., real black holes.
J messes with the angular dependence and structure of the horizon. Not sure what charge does - it doesn't enter into the metric in many places other than the numerator. You'll note that a != 0 causes the metric to be nonsingular at the origin...
Charged/spinning black holes are interesting, because the Schwarzschild throat/Einstein-Rosen bridge may be passable in some geometries. For a standard Schwarzschild geometry, it's not - try to pass through the center of a nonspinning noncharged black hole, and you'll die, as it's not stable.
Re:antimatter particles (Score:2)
Re:antimatter particles (Score:3, Informative)
Net charge is a property we could infer from the electric field, but the actual field emanates from the event horizon, not the unreachable singularity.
Re:Bad idea? (Score:3, Informative)
Nobody's talking about creating any more black holes than get created naturally. They are talking about detecting black holes that do get created naturally in our upper atmosphere.
If you actually need more explanation, go to the article.
OK,
- B
It happens all the time! (Score:4, Informative)
As the article said higher up, the smashing of cosmic rays into ozone has been known to create such an amount of energy at such a tiny level that an extremely unstable black hole can be created for an infinitesimal period of time. This object does not have close to enough energy to suck anything into it. Even if the black hole created was a bit larger than an atom, it couldn't do more than take in a few atoms before it expends the energy it has available and "fizzle[s] out".
The article also states that it is a decently rare experience that rays with enough pent-up energy arrive that a black hole can be created.
The attempt to generate these black holes ourselves is somewhat of a different matter, but not much. CERN originally got a lot of flak for attempting to do this, since a lot of uneducated people freaked out about the thought of a black hole being created. But, that has since died down because it was so long ago and, annoyingly, the average person is kinda forgetful :).
Now, onto the good stuff. The black holes that CERN is attempting to generate are the equivalent of those that the article talks about that the PAO is trying to detect. Why it won't hurt us is due to the nature of black holes and how they are created.
A black hole requires an immense amount of energy to be created on a grand scale. That's the reason that only the largest of giant stars will become black holes when nova. The more energy it has in it while in a black hole state, the greater stability is has (though it's likely excruciatingly chaotic, and that's another branch of really fun science :). The ones that will be created will only have a small amount of energy, so little in fact that they could not possibly stay in existence for long enough to do damage. More so, with every particle that is brought into the black hole it requires a specific amount of energy expended by the black hole to drag this particle in. This is, of course, the fun part because no one's quite sure what happens to this particle. Does it disappear from our dimension? Does it come back when the black hole dissipates? There's only one way to find out, and by using harmless black holes so small they cannot do any sort of damage (if it's really damage) to more than a few nearby atoms, we are extremely safe from the attempt.
Hope you find some solace in all that :)
- DaftShadow
Re:BFD (Score:1)
Re:BFD (Score:1)
Re:Will do research for food... (Score:2)
Please also realize that Argentina (media) = Buenos Aires, and Argentina (country) = a whole lot more. Malargue, the place where the observatory is located, is about as "politically unstable" as we are - not that that's saying a whole lot. Really don't trust the media as to what's going on in Argentina.
Also, who exactly would buy a PMT on the black market? They're useless commercially. The only thing of any value commercially in the entire project are the solar panels for power, and they'd be rather difficult to take (and not be noticed by the gauchos - a covert op into a ranch is not exactly easy).
Finally: SuperK is not downed at all. If you check their Web site, it's an absolute given that they're going to rebuild the observatory. $30M for one experiment that's proven and contributed massively to science is dirt friggin' cheap.
Re:Will do research for food... (Score:2)