[HN Gopher] Gravitational-wave detector LIGO is back
       ___________________________________________________________________
        
       Gravitational-wave detector LIGO is back
        
       Author : gmays
       Score  : 110 points
       Date   : 2023-05-26 16:15 UTC (6 hours ago)
        
 (HTM) web link (www.nature.com)
 (TXT) w3m dump (www.nature.com)
        
       | fjfaase wrote:
       | For observatory status see [0]. It also gives the estimated
       | detector range in megaparsecs (Mpc). Initial LIGO's "range" (the
       | radius out to which LIGO could detect at least a binary neutron
       | star (BNS) merger) was 15 Mpc. With the latest improvements is
       | more in the 140 Mpc range. Meaning that it can see more than 9
       | times as far and that the area of space is increased by a factor
       | of more than 800. This will greatly increase the number of
       | gravitational waves being detected.
       | 
       | [0] https://online.ligo.org/
        
         | acqq wrote:
         | Do you know if even longer ranges logged there, like 600, are
         | practically useful or are they too short (in time) for that?
         | 
         | https://online.ligo.org/grafana/public-dashboards/1a0efabe65...
        
         | dr_dshiv wrote:
         | > Meaning that it can see more than 9 times as far
         | 
         | Hear 9 times as far?
        
       | galizar wrote:
       | Nice. There's even a citizen scientist initiative for LIGO [0]. I
       | wonder what's the status on LISA though.
       | 
       | [0] https://www.zooniverse.org/projects/zooniverse/gravity-spy
        
         | kataklasm wrote:
         | One of my professors worked on LISA Pathfinder, the demo
         | satellite used to proof-of-concept LISA technology until the
         | financial shortcomings in the early 2010s were overcome and he
         | recently said that everyone in the project is hard at work
         | getting ready for the program review, after which either a
         | contract is made or the program is reformulated. But no one
         | will put in the gigantic work needed to prepare such a review
         | if it is not almost certain the program will pass the review
         | and become a contract, so things are looking quite good for
         | LISA and its early 2030s launch!
        
           | cubefox wrote:
           | I remember reading about LISA as a kid, around 25 years ago.
           | Currently it is planned to launch in 2037. I somewhat doubt
           | it will ever become a reality.
        
           | wefarrell wrote:
           | I think it would be really neat to have a space based
           | telescope in close proximity to LISA so that when
           | gravitational waves are detected the telescope can point in
           | the direction of the source and capture the light from it.
        
       | captainkrtek wrote:
       | Big LIGO nerd here. If interested, you can get public alerts of
       | LIGO detected activity (on mobile and online):
       | 
       | https://www.ligo.caltech.edu/page/GWPhoneAlerts
       | 
       | https://gracedb.ligo.org/superevents/public/O3/
        
         | Simon_O_Rourke wrote:
         | Good, this is a necessary thing to get back up and running
         | again. Thanks for the update alerts, will subscribe and see
         | what's stirring in the galactic 'hood.
         | 
         | Question though - do gravitational waves diminish significantly
         | as a function of distance or intervening mass?
        
       | causality0 wrote:
       | The LIGO song is required background music for this article:
       | https://youtu.be/degD69wnZcY
        
         | groestl wrote:
         | Thank you for this (channel), I was one of the lucky 10k today!
        
         | wwarner wrote:
         | haha catchy love it
        
       | whoisthis4chan wrote:
       | > Typical gravitational-wave events change the length of the arms
       | by only a fraction of the width of a proton. Sensing such minute
       | changes requires painstaking isolation from noise coming from the
       | environment and from the lasers themselves.
       | 
       | i find it utterly fascinating that we're able to detect such a
       | minuscule deviation
        
         | pfdietz wrote:
         | Lasers beams are bounced back and forth many times, so the
         | deviation builds up. The beams have to be very powerful (100s
         | of kW) to reduce photon counting noise sufficiently.
        
           | wwarner wrote:
           | Kip Thorne explains it pretty clearly in this 2002 lecture
           | 
           | https://youtu.be/mGdbI24FvXQ
        
         | dekhn wrote:
         | interferometry is indeed amazing. When the ultra-important
         | Michelson-Morley experiment was run some ~100 years ago, they
         | were doing interferometry but in those days there wasn't really
         | good vibration isolation technology. They had to float their
         | whole experiment on a pool of mercury (!) in the sub-sub
         | basement of an idle building, and even then, deliveries nearby
         | (by horse) would cause problems.
         | 
         | Nowadays, physics students do the MM experiment in a lab on a
         | benchtop in a day.
        
           | acqq wrote:
           | I'd like to read how these problems are solved "in a lab on a
           | benchtop" today!
        
             | funac wrote:
             | you can build very good hydrostatic vibration isolators in
             | a home machine shop nowadays; commerical optical tables are
             | /very/ steady
        
               | [deleted]
        
             | dekhn wrote:
             | the original experiment is pictured here: https://en.wikipe
             | dia.org/wiki/Michelson%E2%80%93Morley_exper...
             | 
             | what makes it possible to do in a desktop lab course
             | combination of a large number of different innovations. The
             | first is that we know how to make extremely
             | stiff/rigid/strong/flat/thermally stable tables
             | (https://www.thorlabs.com/navigation.cfm?guide_id=41) which
             | can optionally be placed on active vibration-cancelling
             | struts (https://www.thorlabs.com/newgrouppage9.cfm?objectgr
             | oup_id=10...). The second is using cage systems for
             | mounting things with everything lined up parallel and
             | centered
             | (https://www.thorlabs.com/navigation.cfm?guide_id=2255).
             | The third is precise kinematic mounts which make real-time
             | angle tuning a lot easier/more reliable (https://www.thorla
             | bs.com/thorproduct.cfm?partnumber=KM100#ad...). The fourth
             | is now we have powerful lasers and LEDs that make
             | generating lots of light all pointing in the right
             | direection easier (https://www.thorlabs.com/thorproduct.cfm
             | ?partnumber=CPS532-C...). The fifth is that high quality
             | standardized optical parts (mirrors, lenses, etc) are
             | easily available from a wide range of vendors (https://www.
             | thorlabs.com/newgrouppage9.cfm?objectgroup_id=10...).
             | 
             | There are a number of other innovations in material
             | science. but I'd recommend taking a look at Thorlab's
             | Michelson-Morley educational kit. For $3K you get basically
             | everything you need to carry out the experiment:
             | https://www.thorlabs.com/thorproduct.cfm?partnumber=EDU-
             | MINT... plus a nice manual https://www.thorlabs.com/drawing
             | s/5d9e11209b7d4536-820A3379-... that walks you through
             | physical setup and theory behind the experiment (which
             | among other things helped lead to special relativity).
             | 
             | if you want more like this, see https://www.thorlabs.com/ne
             | wgrouppage9.cfm?objectgroup_id=11... which is a hardware
             | kit that accompanies an actual optical lab class. The
             | course is online: https://www.thorlabs.com/drawings/5d9e112
             | 09b7d4536-820A3379-... and gives a fairly straightforward
             | introduction to optics. With this, you can easily build a
             | microscope from components or any number of other nifty
             | optical systems.
             | 
             | Non-optics people (IE, programmers, etc) with enough time
             | and money can learn how to do real-world optical
             | experiments in their garage (this applies to astronomy
             | too). For example after a significant time/money
             | investment, have started building my own microscopes which
             | use real-time object detection to track tardigrades to do
             | behavior analysis (lest anybody feel imposter syndrome,
             | trust me it took a ton of time and money and even then I'm
             | not quite at the level of a good grad student).
             | 
             | It's not my favorite but you can also read
             | https://www.amazon.com/Perfectionists-Precision-Engineers-
             | Cr...
             | 
             | If you want to truly go down the rabbit hole,
             | https://pearl-
             | hifi.com/06_Lit_Archive/15_Mfrs_Publications/M...
        
               | acqq wrote:
               | Wonderful answer, thanks!
               | 
               | Do you know if the "Michelson-Morley educational kit" is
               | really enough to achieve the accuracy of the original
               | experiment or is it just to make "any" functioning
               | interferometer?
        
               | dekhn wrote:
               | I'm pretty sure it exceeds the accuracy of the original
               | experiment. I think not being based on a trough of
               | mercury is pretty important as well. But the manual shows
               | several types of interferometers that can be built in lab
               | courses.
        
               | acqq wrote:
               | Still, I see it is actually called "Michelson
               | Interferometer Educational Kit", not "Michelson-Morley"
               | and the user guide I'm reading (your link gives "The
               | resource you are looking for has been removed", so I've
               | clicked on the "User Guide" on the page instead) also
               | takes care to never directly mention Morley or to suggest
               | that the same experiment can be reproduced with that kit.
        
       | epberry wrote:
       | I absolutely love LIGO. YC actually did a great interview with
       | one of the lead physicists on the project where he described some
       | of the technical hardware and software challenges -
       | https://www.youtube.com/watch?v=1D2j8nTjOZ4
        
         | jackmott42 wrote:
         | That's the guy who when someone told him they got their first
         | detection was incredulous "I don't have time for this" or
         | something to that affect, because he assumed it was a false
         | positive to have gotten something so quickly, but it was real!
        
           | throwawaymaths wrote:
           | How do we know it was real and not overinterpreting noise
           | again?
        
             | kmote00 wrote:
             | It's my understanding that it was correlated by data from
             | the twin facility on the other side of the country.
        
             | Gare wrote:
             | https://en.wikipedia.org/wiki/GW170817
        
               | bsder wrote:
               | That event is _amazing_.
               | 
               | I had no idea how much cross correlation they produced
               | (see the "Scientific Importance" sections). I love the
               | fact that measurements got like _10 orders of magnitude
               | or more_ better--that 's just absolutely absurd.
        
       | borissk wrote:
       | Since learning about gravitational waves I was always curious if
       | a type III civilization could potentially use them as a weapon.
        
         | abecedarius wrote:
         | Pretty hard to direct.
         | 
         | If you've set up a close-orbiting neutron star binary and
         | you're in a military frame of mind, one thing you could do is
         | accelerate missiles to a good fraction of lightspeed. (Same
         | principle as the gravity assists used by planetary probes like
         | Voyager.) The tides would limit the practical size of the
         | missile, though I haven't tried to compute this limit.
         | 
         | (I don't consider this comment to be aiding the interstellar
         | enemy, it's too obvious.)
        
         | saiya-jin wrote:
         | I dont think so, they go in all directions as a shockwave, pass
         | through everything including black holes (even though it would
         | warp it a bit), so its dark forest signalling basically to
         | whole universe.
         | 
         | Since we came to exist so early in the overall age of universe,
         | there is absolutely no chance we are the only sentient civ
         | across hundreds of billions x hundreds of billions/trillions x
         | nr of planets realm.
         | 
         | Super focused super dense ray of very hard gamma rays/cosmic
         | rays should do any trick required for anything made out of
         | matter. Or just swipe left with a black hole or two.
        
           | MaxikCZ wrote:
           | Correct me if I am wrong, but since not even spacetime can
           | escape blackholes, even gravitational wave would get
           | swallowed, wouldn't it? Of course, since we can't "point"
           | gravitational waves in a certain direction, because of the
           | rest of the wave traveling around the hole would basically
           | propagate it even directly behind blackhole (from perspective
           | of source), but that's because the wave goes around, not
           | trough.
           | 
           | Or do grav waves really pass ~trough~ black holes?
        
             | borissk wrote:
             | Hmmm, gravity does escape black holes, so maybe
             | gravitational waves do too.
        
         | sparker72678 wrote:
         | Maybe? There would be far less energy-intensive ways to wipe
         | other civilizations out of the universe, though.
        
         | dekhn wrote:
         | step 1: arrange two black holes near your enemies step 2: wait
         | 2 billion years
        
         | kadoban wrote:
         | Seems orders of magnitude too difficult to be worth it. If you
         | can approach that level of energy, pointing a gamma ray burst
         | sounds more fun. Or just throw some rocks at fractions of c.
        
         | cde-v wrote:
         | Anything can be used as a weapon.
        
           | bsder wrote:
           | Any sufficiently advanced propulsion also qualifies as a
           | weapon.
        
           | HansHamster wrote:
           | First thing that comes to mind is a lethal dose of neutrino
           | radiation: https://what-if.xkcd.com/73/
           | 
           | Now the tricky part is probably to build a neutrino /
           | gravitational wave / whatever source that is intense enough
           | to be useful as a weapon without just evaporating everything
           | in a supernova scale explosion before...
        
             | mhh__ wrote:
             | See also neutrino HFT
        
             | causality0 wrote:
             | One of the most interesting yet sadly least rigorous What-
             | Ifs. He relies on simply scaling up a calculation in
             | absorbed dose at the distance of one parsec. Neutrinos do
             | not interact with nuclei the same way gamma rays do, and
             | the effects of a particular amount of neutrino radiation on
             | living tissue is unstudied and unknown. The paper he cites
             | explicitly points this out but he ignored it.
        
               | raverbashing wrote:
               | Of course it doesn't, I think that was given by the
               | relationship between neutrino count and sieverts
               | 
               | But make no mistake, there is such a thing as a fatal
               | amount of neutrinos. It's just that's a supernova mind
               | boggling amount, but it exists. They do interact due to
               | the weak force, which is more than neutrons do (and a
               | lethal dose of those is well known)
        
       | tommywiseausmom wrote:
       | detect this gravitational wave. oh!
        
       | _Microft wrote:
       | Beside the mentioned laboratories in the US, Italy and Japan,
       | there is another one in Germany albeit of much smaller size [0].
       | The length of its arms are only 600m (1/3mi) each but it serves
       | as testbed for technologies [1] that might later be used for
       | other observatories.
       | 
       | [0] https://www.geo600.org/ ,
       | https://en.wikipedia.org/wiki/GEO600
       | 
       | [1] https://en.wikipedia.org/wiki/GEO600#Advanced
        
       | quercusa wrote:
       | Michelson and Morley smile
       | 
       | https://en.wikipedia.org/wiki/Michelson%E2%80%93Morley_exper...
        
       | waynecochran wrote:
       | The image at the top of the page is not a real image is it? We
       | don't have real photos of black holes yet right? (except the one
       | at https://www.nasa.gov/mission_pages/chandra/news/black-
       | hole-i...)
        
         | [deleted]
        
         | sp332 wrote:
         | The image is credited to the SXS Project, which does black hole
         | simulation.
        
       ___________________________________________________________________
       (page generated 2023-05-26 23:00 UTC)