Showing posts with label Gravitational Radiation. Show all posts
Showing posts with label Gravitational Radiation. Show all posts

Wednesday, February 17, 2016

Feeling black holes collide from close-up

As soon as I heard about that LIGO thing, first thing I thought of, what would it have felt like if you'd been there, maybe an AU away from those coalescing black holes?

Eventually the Internet got around to telling me.
"As I read the historic news, there’s one question that kept gnawing at me: how close would you need to have been to the merging black holes before you could, you know, feel the distortion of space?  I made a guess, [...] you’d need to be very close.

"Even if you were only as far from the black-hole cataclysm as the earth is from the sun, I get that you’d be stretched and squished by a mere ~50 nanometers (this interview with Jennifer Ouellette and Amber Stuver says 165 nanometers, but as a theoretical computer scientist, I try not to sweat factors of 3).

Even if you were 3000 miles from the black holes—New-York/LA distance—I get that the gravitational waves would only stretch and squish you by around a millimeter. Would you feel that? Not sure. At 300 miles, it would be maybe a centimeter—though presumably the linearized approximation is breaking down by that point.

[...]

"Now, the black holes themselves were orbiting about 200 miles from each other before they merged.  So, the distance at which you could safely feel their gravitational waves, isn’t too far from the distance at which they’d rip you to shreds and swallow you!

In summary, to stretch and squeeze spacetime by just a few hundred nanometers per meter, along the surface of a sphere whose radius equals our orbit around the sun, requires more watts of power than all the stars in the observable universe give off as starlight.

"People often say that the message of general relativity is that matter bends spacetime “as if it were a mattress.”  But they should add that the reason it took so long for humans to notice this, is that it’s a really friggin’ firm mattress, one that you need to bounce up and down on unbelievably hard before it quivers, and would probably never want to sleep on."
From Scott Aaronson's blog, a post appealingly titled "The universe has a high (but not infinite) Sleep Number", h/t SSC.

Victor Toth writes:
"A gravitational wave is like a passing tidal force. It squeezes you in one direction and stretches you in a perpendicular direction. If you are close enough to the source, you might feel this as a force. But the effect of gravitational waves is very weak. For your body to be stretched by one part in a thousand, you’d have to be about 15,000 kilometers from the coalescing black hole.

"At that distance, the gravitational acceleration would be more than 3.6 million g-s, which is rather unpleasant, to say the least. And even if you were in a freefalling orbit, there would be strong tidal forces, too, not enough to rip your body apart but certainly enough to make you feel very uncomfortable (about 0.25 g-forces over one meter.) So sensing a gravitational wave would be the least of your concerns.

"But then… you’d not really be sensing it anyway. You would be hearing it. Most of the gravitational wave power emitted by GW150914 was in the audio frequency range. A short chip rising in both pitch and amplitude. And the funny thing is… you would hear it, as the gravitational wave passed through your body, stretching every bit a little, including your eardrums."
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I'm reading "The Welfare Trait: How State Benefits Affect Personality" by Dr Adam Perkins of King's College, London. He talks about the employment-resistant personality and how such people feature disproportionately on welfare. There they tend to have lots of children, both for increased benefits and because they're rather feckless, (A-, C-, in the five-factor jargon).

Amazon Link

Dr Perkins is worried about dysgenic consequences - plainly the potential is there - but how big is the effect? I'm waiting to see whether Dr Perkins gets quantitative, but if he does, he'll be using the Breeder's Equation.

Time for a quick review from West Hunter - this is the Breeder's Equation:
"R = h2S.

"R is the response to selection, S is the selection differential, and h2 is the narrow-sense heritability. This is the workhorse equation for quantitative genetics. The selective differential S, is the difference between the population mean and the mean of the parental population (some subset of the total population).

"For example, imagine a set of parents with IQs of 120, drawn from a population with an average IQ of 100. Suppose that the narrow-sense heritability (in that population, in that environment) is 0.5 . The average IQ of their children will be 110. That’s what is usually called regression to the mean.

"Do the same thing with a population whose average IQ is 85. We again choose parents with IQs of 120, and the narrow-sense heritability is still 0.5. The average IQ of their children will be 102.5 – they regress to a lower mean.

"You can think of it this way. In the first case, the parents have 20 extra IQ points. On average, 50% of those points are due to additive genetic factors, while the other 50% is is the product of good environmental luck. By the way, when we say ‘environmental” we mean “something other than additive genetics”. It doesn’t look as if the usual suspects – the way in which you raise your kids – contributes much to this ‘environmental’ variance, at least for adult IQ. In fact we know what it’s not, but not much about what it is, although it must include factors like test error and being hit on the head.

"The kids get the good additive genes, but have average ‘environmental’ luck – so their average IQ is 110. The luck (10 pts worth) goes away

"The 120-IQ parents drawn from the IQ-85 population have 35 extra IQ points, half of which are from good additive genes and half from good environmental luck. But in the next generation, the luck goes away… so they drop 17.5 points.

"The next point is that the luck only goes away once. If you took those kids from the first group, with average IQs of 110, and dropped them on an uninhabited but friendly island, they would presumably get around to mating eventually – and the next generation would also have an IQ of 110. With tougher selection, say by kidnapping a year’s worth of National Merit Finalists, you could create a new ethny with far higher average intelligence than any existing. Eugenics is not only possible, it’s trivial."
Dysgenics too: as personality has similar heritability to intelligence (0.5), still mulling over the application of this to the profligate underclass ...

You might also want to take a look at this.

Thursday, February 11, 2016

The LIGO announcement

BBC News rapidly broke away from the 3.30 pm news conference back to the studio, where their own woefully ill-informed correspondent recycled the headlines. The press conference, aimed at lay people, was crammed full with awesome videos and clear explanation. So if you really want to know why this is such a big deal, here's the video - you may have to advance it a little to the start.



LIGO instruments measure gravitational waves at a time resolution of milliseconds. We were both intrigued that planned devices will be able to measure gravitational radiation with a cycle time of a billion years (!) - at 57 minutes 13 seconds.

Wednesday, February 10, 2016

Quotes

Quote from Andrew Ng, Chief Scientist at Chinese search giant, Baidu:
"Worrying about AI evil superintelligence today is like worrying about overpopulation on the planet Mars."
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An anonymous comment at Scott Alexander's Slate Star Codex:
“Slate Star Codex is 140 IQ discussion about 105 IQ issues.”
(Ouch! That post has more amusing and cringe-inducing stuff).

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Watch out for the LIGO announcement tomorrow that the coalescence of two orbiting black holes has been observed through their gravitational wave signature:

"The masses of the black holes will be 36 and 29 solar masses at the beginning; and 62 for the resulting black hole. The reconstructed orbital speed will be almost exactly the speed of light. As a bonus, they will also observe the "ringdown to Kerr"
More here.

Wednesday, October 28, 2015

The Final Parsec Problem

Another interesting link from Jess Riedel's blog. He refers to an article with this title: "Supermassive black holes found spiraling in at seven percent light speed".
"Data from NASA’s Galaxy Evolution Explorer (GALEX) and the Hubble Space Telescope has confirmed the presence of a pair of supermassive black holes orbiting each other so closely that they're moving at relativistic speeds—a significant fraction of the speed of light.

Supermassive black holes are expected to come in pairs pretty often. That’s because every galaxy has its own supermassive black hole, and galaxies often merge, bringing the two together. These mergers are very slow processes that distort both galaxies until their stars settle into new orbits (a process known as "violent relaxation"). While this is happening, extremely heavy objects, such as supermassive black holes, will tend to move in toward the center of the new galaxy. The new galaxy would end up with two supermassive black holes, one from each original galaxy, orbiting each other at its core."
The supermassive black holes (millions of solar masses) tend to orbit each other at a distance of a few parsecs (1 parsec = 3.26 light years). Orbits are pretty stable things - the Earth has been orbiting the sun for quite a while - so to get really close (for example, so close that both black holes would fit inside the dimensions of the solar system) they have to lose energy somehow. But how do you slow down supermassive black holes? This is the Final Parsec Problem.

The binary black holes in the article have:
 "an inferred distance between them somewhere between .007 and .017 parsecs, which is not much bigger than the diameter of the Solar System. That’s astoundingly close for two objects of this size .... To maintain their orbit, the black holes have to be whipping around at relativistic speeds."
The black holes in question will coalesce in perhaps one million years in a massive burst of gravitational radiation. Strictly speaking this has already happened as the system is 3.5 billion light years away - in fact it occurred at the origins of life on Earth!

Here's a Caltech/Cornell computer simulation:



And for further reading, here's the Wikipedia article on binary black holes.