[HN Gopher] Physicists confirm two cases of "elusive" black hole...
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       Physicists confirm two cases of "elusive" black hole/neutron star
       mergers
        
       Author : wglb
       Score  : 75 points
       Date   : 2021-06-29 14:16 UTC (8 hours ago)
        
 (HTM) web link (arstechnica.com)
 (TXT) w3m dump (arstechnica.com)
        
       | ars wrote:
       | Something I've wondered for a long time: Since time around a
       | black hole is frozen, how can we detect a merger? Or when they
       | say merger do they really mean close approach?
        
         | drewrv wrote:
         | I don't fully understand it, but I believe the way to think
         | about it is that: we never "see" something fall into a black
         | hole. But the photons from the "last moment we see" get so
         | redshifted they're essentially invisible. Therefore from a
         | reasonable distance it "looks" like the object disappeared and
         | the event horizon grew in size.
         | 
         | Here's a video, he talks about the redshift around the 8 minute
         | mark. https://youtu.be/vNaEBbFbvcY
        
       | cletus wrote:
       | It's crazy how violent these events are. I remember reading about
       | one of the first where an estimated 5 Solar masses were converted
       | into energy _in about a second_ , which is why it distorted space
       | a billion light years away. I have some questions.
       | 
       | 1. What if you were 1 light year from such an event? What would
       | you experience? What about 100 light years?
       | 
       | 2. What does warping spacetime really mean? I know this happens
       | around a black hole. But what would the macro effects of this be?
       | 
       | 3. So the universe is expanding. Does that mean more "space" is
       | being made? If so, how? Out of what?
        
         | bmitc wrote:
         | I don't have answers for you, but you might be interested in
         | the book _Black Holes and Time Warps: Einstein 's Outrageous
         | Legacy_ by Kip Thorne.
         | 
         | https://www.amazon.com/Black-Holes-Time-Warps-Commonwealth/d...
        
         | immmmmm wrote:
         | i'm a former physicist but yeah, a few stellar masses worth of
         | energy is beyond (my) imagination
         | 
         | 1. always wondered the same. i'd suspect that for most
         | astronomical BH you would first need to worry of X/gamma rays.
         | you could possibly hear a loud chirp since it is audio
         | frequency.
         | 
         | 2. the warping of space time here on earth is actually mostly a
         | warping of time, which is even weirder. i means that the time
         | at your feet is flowing slower that where you're head is. about
         | one second on your entire life. that's actually WHY you feel
         | earth gravity.
         | 
         | 3. yes, more space is created out of nothing! because there's a
         | vacuum energy density that inflate the local patch of universe.
         | 
         | funnily why all of the above is hard to understand for our
         | human brains, it all makes sense in the mathematics..
         | 
         | i highly recommend the YT channel PBS Space Time for more
         | explanations
        
           | macspoofing wrote:
           | >yes, more space is created out of nothing! because there's a
           | vacuum energy density that inflate the local patch of
           | universe.
           | 
           | I don't think you can say that with that kind of certainty.
           | We don't have a theory of quantum gravity, we don't know what
           | dark matter is, and we don't know what 'dark energy' is, so
           | we don't actually know what is driving the expansion of the
           | universe, so saying that 'space is created out of nothing' is
           | too strong. Even something like the theory of cosmological
           | inflation, which has some explanatory power, hasn't been
           | experimentally verified, but rather tuned to match the
           | observations.
           | 
           | It's something I've noticed in a lot of communicators of
           | science (whether they have a background in science or not).
           | They tend use terms that overstate our actual knowledge in
           | some specific area of science.
        
             | Iwan-Zotow wrote:
             | > I don't think you can say that with that kind of
             | certainty.
             | 
             | well, any classic (in SM sense) QFT will produce positive
             | vacuum energy density which translates into negative
             | pressure. P = -E
        
           | lapetitejort wrote:
           | > funnily why all of the above is hard to understand for our
           | human brains, it all makes sense in the mathematics..
           | 
           | Of the four fundamental forces, the higher order aspects of
           | gravity effect humans the least. Satellite operators may need
           | to correct their clocks every once in a while, but other than
           | that, we just can't reach the speeds or distance from earth
           | to notice time dilation, nor can we collide masses large
           | enough to detect gravitational waves.
           | 
           | I was shocked in college when my General Relativity professor
           | told me that very few scientists are studying GR, most likely
           | because it's surprisingly more intuitive than quantum
           | physics, and it's harder to experiment. I really wanted
           | gravity to just be... cooler, I guess.
        
         | tzs wrote:
         | I'm not sure if answers to those specific questions are there,
         | but in general PBS Space Time deals with that kind of thing
         | (and a lot more). Here's their YouTube channel [1] and here is
         | their page at PBS.org [2]. It's also available via the PBS app
         | on many streaming devices and smart TVs.
         | 
         | Most of their videos are in the 8-13 minute length, and they do
         | a pretty good job at the start of each linking back to earlier
         | episodes that cover prior material that the current video
         | builds on, so if you see a video whose title/topic seems
         | interesting it is fine to start their first.
         | 
         | [1] https://www.youtube.com/channel/UC7_gcs09iThXybpVgjHZ_7g
         | 
         | [2] https://www.pbs.org/show/pbs-space-time/
        
         | drran wrote:
         | 1.
         | 
         | 5 solar masses is 1x10^34 g. 1 g of mass is roughly 0.9x10^14 J
         | (mc^2).
         | 
         | So, roughly 1x10^48 J.
         | 
         | 1 ly is roughly 1x10^16 m. Surface area of a sphere with r=1
         | ly, is 4pr^2 = 4p x 10^32 m^2 or roughly 1x10^33, so each m^2
         | of surface will receive 1x10^48/1x10^33 = 10^15 Watt, or about
         | 10^12 x brighter than our Sun on Earth in sunny day, but for 1
         | second only.
         | 
         | 2. Spacetime is 4d array: [x,y,z;t]. Warping of spacetime means
         | that a scientist applies a mathematical formula to the array
         | directly, like shader in OpenGL. It has no physical meaning. It
         | just a quick way to simulate unknown physical process, to make
         | a prediction.
         | 
         | 3. No, it doesn't. Our local group of galaxies is expanding,
         | but this is a coincidence. Actually, we are falling into a
         | black hole. Nearest big black hole is in the center of our
         | galaxy, then Great Attractor, then Shapley Attractor.
        
           | nine_k wrote:
           | 1. I suppose 10^12 brighter than the Sun for 1 second is like
           | standing right next to a large nuclear blast, or a series of
           | them to extend the irradiation phase to 1 second. It would
           | take less than 1 second for an observer to evaporate, but the
           | time is important to see if e.g. the surface of the planet
           | would turn to cinder and glass.
           | 
           | 2. I suppose it's still possible to illustrate. We can
           | imagine that the spacetime gets "bulged" a bit, so light rays
           | become slightly bent when passing it. It's likely impossible
           | to notice with a naked eye from inside without being torn by
           | tidal forces. But it's quite visible from some distance:
           | pictures of gravitational lensing on astronomical scale are
           | easy to find.
        
           | hypertele-Xii wrote:
           | > about 100x brighter than our Sun on Earth in sunny day, but
           | for 1 second only.
           | 
           | Sounds hot. Flash burn everything not made of stone. Land
           | life wouldn't survive?
        
             | drran wrote:
             | I made a mistake in the calculation (10^34 x 10^14 is
             | 10^48, not 10^38), so it's 10^12 brighter. Nobody will
             | survive on the lit surface of a planet.
        
               | x3n0ph3n3 wrote:
               | And it would likely ignite the atmosphere, which would
               | travel at the speed of sound to the "dark" side of the
               | planet, yes?
        
               | phasetransition wrote:
               | So 1e6 light year radius to match the solar irradiance
               | from purely inverse square losses? Wow.
        
         | diegoperini wrote:
         | 2. One macro effect would be (assuming the observer is at a
         | safe distance) unexpected tidal waves in the oceans seeming to
         | appear from nowhere right after the merger.
        
         | ben_w wrote:
         | Frustratingly, when I tried to ask on Physics Stack Exchange if
         | you could hear a gravitational wave and if so how powerful it
         | would have to be, I managed to _simultaneously_ have the
         | question closed as a duplicate with a link to someone saying
         | "yes" without saying how powerful, and find the top answer on
         | my question was "no".
         | 
         | https://physics.stackexchange.com/questions/560833/could-a-h...
        
           | Thorondor wrote:
           | Hi Ben, as the person who initially flagged your question as
           | a duplicate, I'm sorry. I can see why this was frustrating.
           | I'll try to provide a more detailed answer here.
           | 
           | According to a 1948 paper by Bekesy [0], a human ear can
           | detect sounds through several mechanisms. In a gravitational
           | wave, since the whole head would vibrate, sound would reach
           | the ear by bone conduction through the skull. Fortunately,
           | this also happens to be the most sensitive mechanism. The
           | smallest vibration amplitude detectable by bone conduction is
           | about 4 x 10^-9 cm at around 3 kHz. If a typical skull is
           | about 17.5 cm from front to back, that gives a minimum
           | detectable wave amplitude h (the fractional expansion and
           | contraction of spacetime) of about 2 x 10^-10.
           | 
           | The frequency of the gravitational waves produced in a
           | collision between a neutron star and a small black hole turns
           | out to be pretty close to an optimal match for the human ear.
           | To estimate the amplitude, the first black hole collision
           | detected at LIGO produced a strain of about 10^-21 at a
           | distance of 410 Mpc. (The events in the article were smaller,
           | but within the same order of magnitude.) Thus, since the
           | amplitude scales as 1/r, the gravitational waves from the
           | collision in the article would have been theoretically
           | audible at a distance of about 400 AU or 40 billion miles.
           | 
           | Alas, attempting to test this calculation experimentally
           | would incur certain practical difficulties. Notably, you
           | would be vaporized by gamma radiation from the collision
           | several seconds before the gravitational waves became
           | audible.
           | 
           | [0]: https://asa.scitation.org/doi/10.1121/1.1906433
        
             | ajross wrote:
             | > I'll try to provide a more detailed answer here.
             | 
             | Maybe you could provide a more detailed answer THERE
             | instead?
        
             | BitwiseFool wrote:
             | >"Notably, you would be vaporized by gamma radiation from
             | the collision several seconds before the gravitational
             | waves became audible"
             | 
             | How much lead shielding would you need to survive such a
             | thing? Would standing on the far side of an Earthlike
             | planet absorb the gamma rays?
        
               | Thorondor wrote:
               | You'd need a lot of shielding. A planet is about the
               | right order of magnitude, though it's still not clear
               | that a human could survive. You wouldn't die of acute
               | radiation poisoning; a few thousand km of rock would be
               | enough to absorb the gamma rays. At 400 AU, you wouldn't
               | immediately boil to death, either. Part of the collision-
               | facing surface of the planet would be converted into
               | plasma and ablated into space, which would insulate the
               | rest of the planet from the worst of the heat.
               | 
               | My guess is that you'd still die from shock waves
               | propagating through either the atmosphere or the planet
               | itself, but it's difficult to predict the exact effects.
        
               | treeman79 wrote:
               | In the right scenario the neutrinos would kill you. Aside
               | from everything else. Read somewhere you would need a
               | light year of lead to stop them
        
             | ben_w wrote:
             | Awesome, thanks for the detailed response!
        
             | Topgamer7 wrote:
             | Hacker News once again proving to be the king of social
             | networks.
        
               | jazzyjackson wrote:
               | Or at least the royal court where you can bump into the
               | squires and get your issue resolved without the plebeian
               | bureaucracy.
        
             | arthurcolle wrote:
             | This is amazing. What are the chances you'd find this?
        
             | java-man wrote:
             | why not post _this_ answer to physics.stackexchange.com?
        
               | Thorondor wrote:
               | The question is currently closed, so I can't post a new
               | answer. I voted to reopen it, and I've edited the title
               | to focus on the aspect of the question that is not
               | adequately answered by the duplicate.
        
               | R0b0t1 wrote:
               | Be careful when you do this. It is easy to want to change
               | a question you can't answer into one that you can, but
               | you really have no idea what the original poster was
               | asking. I had a question changed into something extremely
               | idiotic by dilettantes who thought they knew what they
               | were doing.
        
             | quakeguy wrote:
             | Great reply!
        
             | varjag wrote:
             | (400 AU is ~ 10x-15x the distance to Pluto)
        
         | NegativeLatency wrote:
         | Possibly your atoms, and probably your molecules would be
         | ripped apart by the gamma rays and other particles emitted
         | before a shockwave hit?
        
           | AnimalMuppet wrote:
           | _Before_? Gravitational waves travel at the speed of light
           | too...
           | 
           | (Or are you saying that the gamma rays are emitted earlier in
           | the merger process than the gravitational waves?)
        
             | goldenkey wrote:
             | A better way to think of the speed of light is as the
             | stiffness of spacetime. This allows for you to intuit what
             | warping effects do to the trajectory of light and gravity.
        
       | triangleman wrote:
       | Is there any chance these were somehow the same event, and the
       | universe sort of loops back on itself?
        
       | boringg wrote:
       | How long ago did these events actually happen though? Is it a 1:1
       | ratio therefore events happened 1.2B years in the past?
       | 
       | All these merging events that we are picking up now - are there
       | still on-going events or has the frequency dropped off as the
       | cosmos have moved apart and relative, to early years, "settled"
       | down?
        
         | marcosdumay wrote:
         | > How long ago did these events actually happen though?
         | 
         | If you are asking if gravitational waves move at the speed of
         | light, then yes, they do.
        
       | rrauenza wrote:
       | Having just finished Diaspora this summer based on a different HN
       | posting recommending it... this is really cool.
       | 
       | (I don't know that I could recommend Diaspora. It's dense and I
       | think requires a level of familiarity with quantum physics to
       | truly enjoy. It felt like a bit of a slog for me...)
        
       | phasetransition wrote:
       | FYI, primary source is Open Access:
       | https://iopscience.iop.org/article/10.3847/2041-8213/ac082e
        
         | m4r35n357 wrote:
         | Impressive author list!
        
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