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Science

MiniGRAIL Online 24

An anonymous reader writes "MiniGRAIL - the first spherical resonant mass gravitational wave detector in the world - is now taking data!!! The MiniGRAIL (Gravitational Radiation Antenna In Leiden) detector is located at the Kamerlingh Onnes Laboratory of the Leiden University (The Netherlands). The MiniGRAIL detector is a cryogenic 68 cm diameter spherical gravitational wave antenna made of CuAl(6%) alloy with a mass of 1400 Kg, a resonance frequency of 2.9 kHz and a bandwidth around 230 Hz, possibly higher. The quantum-limited strain sensitivity dL/L would be ~4x10-21. The antenna will operate at a temperature of 20 mK. An other similar detector is being built in São Paulo, which will strongly increase the chances of detection by looking at coincidences. The sources we are aiming at are for instance, non-axisymmetric instabilities in rotating single and binary neutron stars, small black-hole or neutron-star mergers etc."
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MiniGRAIL Online

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  • by ghostlibrary ( 450718 ) on Friday November 19, 2004 @11:54AM (#10865205) Homepage Journal
    Okay folks, since MiniGRAIL is now taking data in the Netherlands and its partner is doing that in São Paulo, a cautionary.

    Please, those of you located equidistant from the two, don't jump, stomp your feet, or drop heavy books. They rely on asymmetry to weed out false signals, and you folks straddling the middle could throw it off.

    Remember, we must all do our bit for science.
  • by Anonymous Coward on Friday November 19, 2004 @11:56AM (#10865234)
    Dammit.. they don't have this translation option yet.
  • What? (Score:2, Insightful)

    by Muda69 ( 718162 )
    Did anybody at all understand exactly what in the world this GRAIL thing is supposed to do? In layman's terms please....

    And oh, the name is kinda lame. They could have at least brainstormed a bit and come up with another acronym like holyGRAIL or something.

    • Re:What? (Score:5, Informative)

      by Compuser ( 14899 ) on Friday November 19, 2004 @12:08PM (#10865378)
      They are looking for gravitational waves. The kind
      that are predicted to exist by various versions of
      relativity.
      This is why they are looking for things like black
      hole mergers - because those are supposed to give
      off major gravity ripples that could hopefully be
      seen by our puny labs on Earth.
      I am curious how their theoretical resolution
      measures up to the bigger projects like LIGO. I am
      also curious how much it costs to keep that much
      mass this cold continuously. You need a huge
      dilution fridge which would consume some unholy
      amount of liquid Helium 4. That's assuming you
      got no He 3 leaks. Costs please...
      • Re:What? (Score:2, Interesting)

        by Compuser ( 14899 )
        Hate to reply to myself but my first post was before
        I RTFA'ed.
        Looks like for some frequencies they will be in the
        same ballpark of sensitivity as GEO which is nice
        since I always doubted theoretical estimates from
        GEO and LIGO as being too optimistic. If they can
        get to these sensitivities then maybe the big boys
        can get there too.
        Oh, and given what I heard about Kadel (their dewar
        maker of choice) I reiterate my doubts about He 3
        leaks. Why not Oxford? And how much does their
        setup cost to run continuously?
    • the site offers no explanation that I could understand at least... Who knows. All I really understood is that a 63cm diameter device weighs about 1400 Kg... That's one dense something-or-other.
    • Re:What? (Score:3, Informative)

      by stevelinton ( 4044 )
      Gravity waves show up as (very) slight distortions of everything. So, for instance things might get a bit longer North-South and a bit shorter East-West for a bit, and then the other way for a bit, and so on.

      The changes are VERY tiny, something like 1 part in 10^20, so detecting them is not easy.

      Existing detectors measure tiny changes in the length of bars of metal. Results are borderline at best.

      Straight-forward detectors like LIGO and the much larger space-based proposal whose name I have forgotten for
  • Whoa. (Score:3, Insightful)

    by BigZaphod ( 12942 ) on Friday November 19, 2004 @11:58AM (#10865253) Homepage
    This has to be one of the most densely packed slashdot stories ever. I understand the words--just not so much the meaning of them in that order. :-)

    Someone bring me the Holy Hand Grenade of Antioch! "Bless this, O Lord, that with it thou mayst blow thine slashdot posting to tiny bits, in thy mercy."
    • The MiniGRAIL detector is a cryogenic 68 cm diameter spherical gravitational wave antenna made of CuAl(6%) alloy with a mass of 1400 Kg, a resonance frequency of 2.9 kHz and a bandwidth around 230 Hz, possibly higher. The quantum-limited strain sensitivity dL/L would be ~4x10-21. The antenna will operate at a temperature of 20 mK.

      IANAPhysicist, but I'll take a crack at it.

      -cryogenic = extremely cold
      -68cm CuAl sphere = ~2 1/4 foot metal sphere made of a copper/aluminum alloy that is 6% "parent" metal (th
      • -cryogenic : right.

        -68cm CuAl sphere : I think that would be 6% Al, 94% Cu.

        -Mass of 1400kg : right

        -Resonant frequency 2.9kHz : right. Moreover, a passing gravitational wave of this frequency will excite oscillations in the spere, so it amplifies gravity waves at that frequency and converts them to oscillations that can be measured by more conventional sensors.

        -Bandwidth of 230 Hz : Any resonant system has a particular frequency at which it likes to oscillate. A small input can cause large-amplitude os

  • The MiniGRAIL detector is a cryogenic 68 cm diameter spherical gravitational wave antenna made of CuAl(6%) alloy with a mass of 1400 Kg, a resonance frequency of 2.9 kHz and a bandwidth around 230 Hz, possibly higher. The quantum-limited strain sensitivity dL/L would be ~4x10-21. The antenna will operate at a temperature of 20 mK.

    Wha...? :) (picture monkey scratching head)
  • by christopherfinke ( 608750 ) <chris@efinke.com> on Friday November 19, 2004 @12:03PM (#10865314) Homepage Journal
    We've already got one; it is a-very nice!
  • So, the gravitational waves has to have a frequency pretty close to 2.9kHz to be detected, then? Why that specific frequency? The site seems to offer no clues. Is it just random? It seems awfully high to me...
  • I understood just enough to realize that I wouldn't have to pass the Knights who say "Ni!" on this one.

    That naughty naughty Zoot, leaving the grail shaped beacon on again!
  • by david.given ( 6740 ) <dg@cowlark.com> on Friday November 19, 2004 @12:14PM (#10865439) Homepage Journal
    Since this thing is fundamentally a gravity wave antenna, what's the range of frequencies it can usefully detect? Is it just limited to 2.9kHz waves (plus or minus 115Hz)? What about harmonics? Could it be tuned for other frequencies or would that require a redesign?

    The reason I ask is that not only does this thing have immense cool value, similar detectors might be very handy for SETI. We know practically nothing about the gravity wave spectrum; it's perfectly possible that the reason we can't find any alien communications with radio telescopes is because everybody's communicating with gravity waves.

    So I'm eager to find out what this thing is capable of seeing.

    Incidentally, I'm getting slightly disturbed how similar modern gravity wave detectors are getting to those described in David Brin's Earth. If anyone invents a strange new form of physics for manipulating singularities called cavitronics, I for one wish to emigrate to Mars.

  • Anonymous writes:

    The MiniGRAIL detector is a cryogenic 68 cm diameter spherical gravitational wave antenna made of CuAl(6%) alloy with a mass of 1400 Kg, a resonance frequency of 2.9 kHz and a bandwidth around 230 Hz, possibly higher. The quantum-limited strain sensitivity dL/L would be ~4x10-21. The antenna will operate at a temperature of 20 mK. An other similar detector is being built in São Paulo, which will strongly increase the chances of detection by looking at coincidences. The sources we are a

  • Now I know how all my non-computer friends feel when I start rambling on about computer lingo. You might as well have said "bla bla, bla bla bla 30khz, bla sphere, bla bla bla". anyone else think it looks like the interogation droid from Star Wars?!
  • they can detect gravitational waves with a sphere in a lab?? What are those multi-million dollar projects like the 4km LIGO for then.
    • Because they're cool. Honestly, who doesn't want a 2 1/2 foot diameter copper ball to play with?

      Actually, one of my classmates took a tour of the LIGO facility as part of an ASME conference and "it's cool" was basically the answer she got. It sounded, however, like this one only has a limited frequency range it can detect. Maybe LIGO detects a different range or at least a broader one. It also operates differently (laser beam in a vacuum instead of big ball in a freezer), so I suppose there's probably a

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