Archive for the ‘Mountain climbin’’ Category

Mapping the radioactive heat beneath our feet

Thursday, January 17th, 2008

Heat

Geochemical bods tell us that the Earth is heated from within by the decay of various isotopes, mainly uranium, thorium and potassium. Knowing the distribution of these elements is crucial for understanding the Earth’s inner dynamics.

Geochemists have penty of ideas about how the Earth’s interior may work but no way of taking measurements to prove their ideas. For example, they think there are far more of these hot elements in the Earth’s crust than its mantle but without data, they can’t prove it.

But the geobods ain’t givin’ up and are a-hopin’ and a-prayin’ that the humble neutrino is gonna come to their rescue. The process of radioactive decay gives off neutrinos that would alert geobods to exactly what’s going on and where, if only they could measure ’em.

Truble is that neutrinos are hard to catch at the best of times. Physicists have recently spotted terrestrial neutrinos for the first time, although only by their energy spectrum, not by their direction which is what will be needed if geochems are to work out the distribution of radioactive stuff down there.

Now Stephen “Live and Let” Dye at the University of Hawaii and a pal have worked out exactly what will be needed to map the radioactive brew within the planet. They reckon a large ocean-based detector plus a smaller land based one should do the trick (both will have to be well away from nuclear power stations which produce unwanted neutrinos that would swamp the signal).

The technology to do this is available now but whether they can drum up the support (and the money) needed to make it happen is another question.

Ref: arxiv.org/abs/0801.2366: Estimating Terrestrial Uranium and Thorium by Antineutrino Flux Measurements

The cold dark matter scrap

Friday, January 4th, 2008

WIMP

There’s a race on to find the first direct evidence of cold dark matter. And it ain’t pretty. There’s probably a Nobel at stake for the winner which means the leading groups are at each other’s throats, like alleycats over chicken bones.

For any of ya’ll who wanna know who’s who in this backstreet brawl, Laura Baudis at the University of Zurich has compiled a card of the main fighters. All these guys are lookin’ for Weakly Interacting Massive Particles and she gives a good summary of all the contenders looking to be crowned king of  WIMPs.

The basic idea is that WIMPs sit around in space twiddling their thumbs until a great big lump of ordinary stuff like the Earth comes along and smashes into them. When this happens physicists should be able to see the impact in their labs as atoms get pranged.

Laura takes the rather optimistic view that “the major questions have shifted from ’how
to detect a WIMP’ to ’how can we identify its nature in case of a signal’”
.

She neatly avoids the biggest question which is whether WIMPs exist at all.

They’ve been imagineered to explain the observation that many galaxies are spinning so fast that the matter they contain ought to be thrown outwards.  Something has to be holding these galaxies together and so astrobods have hypothesised that particles called WIMPs provide the extra gravitational ooomph to hold galaxies together.

But plenty of theorists think other explanations are just as feasible, modified newtonian gravity, for example. And if they’re right, then the hundreds of millions of dollars being spent in this area might as well have been dumped at the bottom of a dirty great mine shaft. Which, as fate would have it, is where most of the WIMP detectors happen to have ended up anyway.

Ref: arxiv.org/abs/0711.3788: Direct Detection of Cold Dark Matter

The number of fundamental dimensional constants reduced to two

Tuesday, December 4th, 2007

Time and space but not mass

Yer only have to go back to Plank to find a pretty detailed argument that there are three fundamental dimensional constants from which all others can be derived. They are length, time and mass. Plank argues that as long as you got a tape measure, a clock and set of scales you can measure anything in the universe.

Seems reasonable but various philosophers have argued over the details sayin’ maybe there are no constants or perhaps two or God knows how many. But being philosphers, they ain’t interested in actually provin’ anything only arguin’ about it.

Now a group of Brazilian eggheads this week say they have proven the result objectively and that Plank is wrong. They reckon there are only two of fundamental dimensional constants and that these correspond to length and time. They argue that all ya need is a tape measure and a clock.

A key to their thinkin is that they assume that all that can be measured are intervals in space and time. This leads to the idea that gravitational mass is the same as inertial mass, which is a big leap but one they say they prove. Given that, mass is simply the acceleration produced on a test particle at a certain distance. Ya don’t need no scales to measure that.

Interesting approach. When it comes to fundamental dimensional constants, two is a big improvement on three.

Ref: arxiv.org/abs/0711.4276: The Number of Dimensional Fundamental Constants

Recipes for other Earths

Friday, October 26th, 2007

It ain’t gonna be long now before we find another Earth orbiting a nearby star and the question is: what are we gonna do when we find one?

(By some accounts we already found at least one but in reality these bodies are too big to be like Earth.)

Eric “Nose” Gaidos at the University of Hawaii and his buddies know. They gonna use it to study various theories about how small rocky planets form. Do they form close in to a star which seems difficult given the inhospitable conditions that exist near stars when they form, or do they form further away and spiral inwards?

Nobody knows which recipe is correct or whether other ideas may eventually trump these ones but they is hoping to find out soon.

Ref: arxiv.org/abs/0710.2366: New Worlds on the Horizon: Earth-Sized Planets Close to Other Stars

The science of the Edelweiss

Wednesday, October 24th, 2007

The Sound of Music always brings a tear to mah eye. And now it’ll have new meaning thanks to the sterling work of Jean Pol “Pot” Vigneron and his buddies at the Facultes Universitaires Notre-Dame de la Paix in Belgium.

Pol Pot has been a-caressin’ and a-cuddlin’ one of the movie’s stars: the Alpine flower Edelweiss, and has discovered that the white hairs covering its leaves are actually photonic structures tuned to ultraviolet wavelengths. So Edelwiess turns out to be one of only a handful of plants that can actually grow photonic structures.

In the Alpine meadows where Edelweiss grows, UV levels are much higher than at lower altitudes and would ordinarilly damage plant cells. But the hairs prevent UV light from reaching the leaves while allowing other colours to pass unhindered. Pol Pot says the hairs are hollow tubs with ridges running along their length that trap light at UV wavelengths.

One outstanding mystery is what happens to the UV light once it becomes trapped in the filament. Pol Pot and his team have been a-contemplatin and a-meditatin on this for a while now and speculate that the tubes may be filled with water which absorbs UV light.

The hairs may even turn out to be be useful. Most UV sun screens rely on nanometre-sized particles of titanium oxide which can be difficult to handle and may not be usable for certain applications such as food packaging. Now we have an alternative: the hairs from the Alpine flower Edelweiss

Ain’t thatta bee-yoo-tiful piece of science?

Altogether now…

Edelweiss, Edelweiss
Every morning you greet me
Small and white,
clean and bright
You look happy to meet me.
Blossom of snow
may you bloom and grow,
Bloom and grow forever.
Edelweiss, Edelweiss
Bless my homeland forever.

Sniff…

Ref: arxiv.org/abs/0710.2695 : Optical Structure and Function of the White Filamentary Hair covering the
Edelweiss Bracts