The Sun seen through the Earth in “neutrino light” (2007)
strangepaths.com
strangepaths.com
There is no hard boundary to the core of the sun. The "core" is by definition where nuclear fusion reactions occur. However, those reactions don't just stop at a certain radius...but instead just occur at a lower and lower rate. So even if you could determine with 100% precision where a neutrino came from within the sun, you would still measure some exponential-like decay as a function of radius.
But to add even more complexity there's ~10 different nuclear processes within the sun that produce neutrinos. Those processes all have different radial profiles. So even if you measure with 100% accuracy the radial profile of neutrinos associated with one or two nuclear processes...you still haven't really measure the core of the sun...you've just measured it for a few specific reactions. And for the neutrinos produced by many of the reactions this method cannot work, those neutrinos are too low in energy to provide direction information. And beyond that there are a handful of nuclear reactions that occur within the sun that don't produce neutrinos. So there doesn't really exist any way to measure the radial profile of those nuclear processes.
And this all assume you can perfectly tell where the neutrino came from within the sun, which is also impossible. There will always be some relatively poor "resolution associated with your ability to place a neutrinos origin. Here is the "hard" physics limit to your angular resolution for a relatively high solar energy neutrino...it only gets worse as the energy goes down https://i.imgur.com/h3n8c4V.png. But getting to even that resolution is impossible b/c an interaction will only produce so many photons from Cherenkov radiation (think 100s of photons). Then it becomes a statistics problem...what's the best angular resolution you could possibly achieve given an average number of photons that's around (say) 500. It ends up the answer is "pretty good" but far from perfect. And all of that is assuming the electron scattered from the solar neutrino will travel in only one direction...that's extremely untrue, the electron will always bounce off of other electrons & atoms after scattering. This multiple-scattering leads to even worse angular resolution.
Here's a paper on the subject if you'd like further detail https://arxiv.org/pdf/1606.02558.pdf
Every time the Internet regurgitates this link it is misinterpreted by essentially everyone that comments on it.
https://journals.le.ac.uk/ojs1/index.php/pst/article/view/85...
Not practical, hmm?
Is this possible? I'm considering a loose definition of the word "possible" here, but could such an arrangement exist without collapsing to a black hole under gravity or being torn apart by centrifugal force?
that's a neat idea. the orbital mechanics involved are pretty mind-boggling, but I guess a civilization that could create a system of neutron stars could probably deal with the math ;).
So maybe we could use them as neutrino detectors and/or sails :)
Hm, can we detect big black holes that way - looking at their neutrino shadow?
https://www.power-technology.com/features/neutrino-energy-ha...
One of my far-future-tech fantasies is that we someday learn to make photovoltaics that are powered by cosmic rays and/or neutrinos.
If I'm reading that paper above correctly, which despite its silly premise appears to have been seriously written (by undergrads, but the numbers pass the smell test), neutrinos have ~1/70th the power flux of solar anyhow, assuming you could catch all of them, which you can't.
From a little poking around it sounds like cosmic rays have a more useful power flux.
To be "charitable", maybe someone multiplied the solar neutrino flux/sqcm by their "maximum" energy (wikipedia numbers: 17e10 x 8e6 ~= 0.2w) and thought "that could power things!!!"
But more likely this is some sort of deliberate scam.
Without a miraculous scientific breakthrough the math doesn't add up. We don't know of any way to capture neutrons in a way that would provide meaningful power. For those reasons, I'll suggest this is more likely a scam than a sincere or realistic effort.
Neutrinos, they are very small.
They have no charge and have no mass
And do not interact at all.
The earth is just a silly ball
To them, through which they simply pass,
Like dustmaids down a drafty hall
Or photons through a sheet of glass.
They snub the most exquisite gas,
Ignore the most substantial wall,
Cold-shoulder steel and sounding brass,
Insult the stallion in his stall,
And, scorning barriers of class,
Infiltrate you and me! Like tall
And painless guillotines, they fall
Down through our heads into the grass.
At night, they enter at Nepal
And pierce the lover and his lass
From underneath the bed - you call
It wonderful; I call it crass.
When neutrinos can be captured and emitted with good ability, and they can go through the earth, then how feasible it is to build a data link with them from between let's say Japan and US?
It's not possible today of course, because it would have been done already.
If corporates are literally blowing holes to mountains to get faster and more direct data links between trading places. Then it sounds like just a question of time when the technology matures enough (if it's possible already).
https://blogs.scientificamerican.com/observations/message-en....
In short, they were able to achieve about 0.1 bps with hardware that costs hundreds of millions of dollars.
Unreliable communication that gives you an advantage over mere chance 1% of the time can already be advantageous, you'll be right 51% of the time.
The detector here weighs 50,000,000kg, and still like 99.9..% of neutrinos pass though it without being detected - imagine that kind of signal loss in a data link.
This detector does not notice tiny amount of neutrinos produced at particle accelerators. It would have to placed right next to a 4GW nuclear powerplant to detect neurinos at any kind of reasonable rate.
The only man made source of neutrinos you could detect from another continent is a massive thermonuclear blast.
https://www.sciencedirect.com/science/article/pii/S240560141...
So, you're saying there's a chance?
Plus error correction... When you add error correction and consider the number of missed bits and the need to retransmit / keep transmitting, it's probably not possible to realize a latency win here.
So your communication turns into some random string of detections where you never know if the absence of a detection means there was no neutrino, or it was just missed.
Perhaps, but if you consider the probability of missing an individual neutrino your error correcting scheme will have to be either very long or very clever because your odds of collecting the right neutrino at the right time will go down very quickly as the packet gets longer.
On top of that, if you used some kind of pulse scheme (i.e. morse code with neutrinos) it has to be slow enough to be detectable, but fast enough to beat the latency of a cable (let's say 100ms - speed of light + processing and errors) and also fast enough not to use enough power as to be unprofitable.
Isn't that what I wrote:
> > it's probably not possible to realize a latency win here
?
> On top of that, if you used some kind of pulse scheme (i.e. morse code with neutrinos) it has to be slow
"slow pulse" == long pulse. It will be "fast" in that it will go faster than the speed of light in fiberoptics and the path will be shorter, but it will be slower because error correction will demand a great deal of redundancy which, among other things, means long pulses.
I think we're in agreement.
https://www.math.columbia.edu/~woit/wordpress/?p=4646
It's not impossible, but it's kind of absurd. Neutrinos are insanely hard to detect. You need immense detectors, and even you get only a ludicrously tiny fraction of the neutrinos passing through. You'd have to modulate it by turning on and off an immense nuclear power plant, so despite shaving off milliseconds of latency you still wouldn't be able to communicate fast.
There's no reason to expect any of that to become more practical any time soon. Neutrinos are too small, too fast, and too devoid of interaction to manipulate easily.
A particle accelerator would be much more responsive.
The immense detectors on the other side would stay, and you'll need entire minutes just to get a single neutrino anyway (and then, how many do you need to be sure? at least 2, I imagine.)
There was a new HN thread about such a beam just an hour ago: https://news.ycombinator.com/item?id=23528970
We'd modulate this high-energy beam. Data bandwidth would likely be quite low, but in terms of latency, it should be the fastest.
A beam directly going through Earth (e.g. from North America to Asia) is definitely going to be faster than optical fibre (or satellite) links that have wrap around the Earth.
I'm assuming neutrinos are sparse in nature, which is 50,000 metric ton pool of water was needed to detect the neutrinos emanating from the sun. But if we artificially create a highly concentrated beam of many many neutrinos, even a 99.99% loss / non-detection rate shouldn't be problem. (Again, bandwidth would be low, but we are aiming to minimize latency.)
Unfortunately, not even then. Nowadays you generally neglect the latency of the physical act of receiving a bit and being sure whether it is a one or a zero because it is such a small amount of time compared to the other characteristics of the journey, but in this case you can't do that. The amount of time it will take to be sure whether it's a 1 or a 0 being sent will be dwarfed by the amount of time it would take to send a conventional TCP packet containing significantly more than one bit.
Note that while we neglect it, it still exists. If you zoom down to a small enough scale, you don't get a pristine series of ones and zeros, but a noisy voltage or light signal, and there can be plenty of attoseconds where the current voltage/light could correspond to either a 0 or a 1 coming in next.
No, that's not the reason. The reason is that they barely interact with anything, including detection equipment.
> even a 99.99% loss / non-detection rate shouldn't be problem.
"Two water-filled detectors of this type (Kamiokande and IMB) recorded a neutrino burst from supernova SN 1987A. Scientists detected 19 neutrinos from an explosion of a star inside the Large Magellanic Cloud – only 19 out of the octo-decillion (10^57) neutrinos emitted by the supernova." (from https://en.wikipedia.org/wiki/Neutrino_detector)
We report on the performance of a low-rate communications link established using the NuMI beam line and the MINERvA detector at Fermilab.
The link achieved a decoded data rate of 0.1 bits/sec with a bit error rate of 1% over a distance of 1.035 km, including 240 m of earth.First, you have to modulate the source in such a way as to encode a message. I think we can rule out things that involve blocking the beam, so you'll have to adjust the generation power. You're gonna need a massively powerful nuclear reactor or particle accelerator or something to be at all possible to notice the message, so it will probably be pretty tough to modulate that much power at a frequency high enough to get any kind of decent data rate.
Then we need a detector. Since the article is about a massive and massively expensive detector being able to create sort of an image of the Sun after multiple years of observation, I'm not optimistic about that side. We can build a detector that can tell if a manmade beam is on or off, eventually. I'm not very optimistic about building a detector sensitive enough to detect subtle variations in the power of the beam. We're gonna have a real tough time getting a decent data rate.
Doesn't make much difference if 1 bit can be transmitted through the earth faster than an electric signal can make it around if the electronic one can send billions of bits in the time the neutrino detector takes to send two.
> To create the neutrino beam, a beam of protons from the Super Proton Synchrotron at CERN was directed onto a graphite target. The collisions created particles called pions and kaons, which were fed into a system of two magnetic lenses that focused the particles into a parallel beam in the direction of Gran Sasso. The pions and kaons then decayed into muons and muon neutrinos in a 1-kilometre tunnel. At the end of the tunnel, a block of graphite and metal 18 metres thick absorbed protons as well as pions and kaons that did not decay. Muons were stopped by the rock beyond, but the muon neutrinos remained to streak through the rock on their journey to Italy.
The photo-detectors observe the Cherenkov light and through some well tuned algorithms the electrons direction is "reconstructed". Super-K has no doubt spent significant effort improving & evaluating their reconstruction algorithms.
Once you have the reconstructed electron direction there's almost no hope that you can reconstruct the incident neutrino direction...but that's generally okay, b/c you can usually just assume the neutrino traveled exactly parallel to the electron (i.e. directly away from the sun). But that's sometimes wrong which is (partly) why you see a lot of "fuzz" around the solar core in the image.
Is this image telling us anything new? Can this method be used for any type of observation? Or it simply serve as observation in the opposite direction: knowing where the neutrinos come from, you can infer in what cone the bounced electrons can move?
A fun thought: if one day, a secret organization starts running an undisclosed nuclear fusion reactor, will it show up on this "photo"?
All that being said, the specific shape of the "sun" in the image is influenced by many factors many of which are related to the detection mechanism and the detector itself...and don't tell you that much about the sun. Eventually (one hopes), detectors will improve to the point where the "shape" information of the image is reliable enough to extract interesting solar physics measurements from it.
P.S your fun thought on the detection of a fusion reactor is extremely on point. There exists a under-construction experiment in the UK called "Watchman" that hopes to detect a neutrino signature from a nuclear power plant being shut off and then being used to produce material for a nuclear weapon. The idea would be that you could observe activities of nuclear facilities in a "rouge nation". See here https://www.nytimes.com/2018/03/27/science/nuclear-bombs-ant... or here http://svoboda.ucdavis.edu/experiments/watchman/
The moral implications of such a device are fraught. To use it is to detonate the very weapons that one should not detonate.
For example, when Project Orion was being seriously considered the scientists had to find ways of making large quantities of fairly powerful nuclear weapons cheaply and quickly. Based on something Freeman Dyson said, I think they succeeded to some extent, but that secret now has died with the scientists who worked on it.
There has to be a lot of writing squirrelled away somewhere, because there are restrictions like "You agree to obtain a validated export license when exporting if this product is incorporated into the design, development, production, or other activities related to chemical weapons, biological weapons, nuclear weapons, or ballistic missiles." but no available literature on how these packages may actually be used in this context. (https://welsim.com/download)
One of the reasons Nuclear Testing is now very uncommon is because computers and software are now advanced enough to simulate them accurately. And yet, despite that, there is no "Nuclear Weapons design: A modern approach" available for public consumption. These are worked on by physicists so someone must be wasting time by writing books somewhere.
Also, in order to cause the Cherenkov radiation, the neutrino has interact at least with an electron, I wonder about the percentage of the number of neutrinos interacting with the water in this vs. the number of neutrinos that interacted with Earth on the way.
Not anything practical... I'd just be curious.
And I don't know any specific numbers but you can be sure a large amount more of neutrinos interacted with the air/rock between the Sun and Super-K than interacted in the detector volume. But that number (whatever it is) is still tiny compared to the total flux (which is ~5 million per square centimeter per second).
And that's of just the "high energy" type neutrinos that Super-K is sensitive to. The lower energy varieties are more like 10 billion per square centimeter per second.
("The Cherenkov Effect, completely normal phenomenon" if you've seen Chernobyl - if you haven't, it's very good)
I wonder how much more feasible it is to send information via neutrinos if 0.000000013 Mbps were considered reasonable speed.
The daytime data and night time data are decoupled quite easily. Whenever an event is recorded by the detector you just make sure a timestamp is associated with the event. Then you use that timestamp to determine the location of the sun at the time of the event. If the sun is below the horizon it's "night" and if it's above the horizon it's day.
Edit: I see that someone else asked a similar question, the answer being that you image electrons that have been knocked loose by neutrinos, which is much easier.
Well, that's relative ;) It still takes hundreds of highly-sensitive detectors and many tons of hyperpure water to detect neutrino reactions.
Effectively, a bad unit cracked, and because they were submerged in a fluid, it created a shock wave that caused other units to crack, which caused more units to crack. They had to replace some large percent of the sensors and it set them back something like a year.
I'm not a physics guy so it would bee be better if someone with domain knowledge could chime in.
[1] Here's a picture of one: https://amp.businessinsider.com/images/5b23cd9d1ae66220008b5...
Neutrino detectors can also "see" active nuclear reactors. One could imagine using a detector located outside of a suspect nation to validate their claims with regards to nuclear nonproliferation (ie that they're not running their reactors overtime to produce more plutonium than they report).
It could reveal the general shape of the universe or center of universe.
Is the image aligned to the "main" ecliptic plane of Solar system or rather to Sun's rotation plane (7.25° from those) ?