Gravitational waves should permanently distort space-time
quantamagazine.org
quantamagazine.org
When I think of waves, I think of systems governed by the wave equation [0].
But IIUC that requires a restoring force. I'm not sure what that would mean in the case of gravity.
E.g., if the moon suddenly lurched towards the Earth, we'd perceive an increase in gravity between the two. But that would be a semi-permanent change in the strength of that attraction between the two objects; not what I'd think of as a wave-like fluctuation.
In general Einstein's field equations govern the dynamics of $g$, and if you take the first order behaviour in $\epsilon$ around $g_0$ as flat space, then you recover the wave equation for $h$ as in the article you linked, with propagation speed $c$ the speed of light. (There are some additional subtleties about choice of gauge, but this is not physical).
I'm not sure what you mean with your moon example.
Suppose the gravitational attraction between the earth and moon is 2e20 Newtons.
Now imagine something forces that attraction to strengthen from 2e20N to 3e20N. E.g. the Earth and moon get closer to each other, or the moon gets more massive somehow.
When we talk about "detecting gravity waves", I understand that to mean that on Earth we've managed to detect that increase from 2e20N to 3e20N.
My point was: perhaps that looks like the rising edge of a wave phenomenon, but it's not actually cyclic like I expect from a traditional "wave". So I couldn't understand why it's called a gravity wave.
Unfortunately, I don't know enough to explain the difference.
https://en.wikipedia.org/wiki/Gravity_wave
They have absolutely nothing to do with gravitational waves.
Nonetheless, in the gravitational wave community (i.e. LIGO) we don't usually ever talk about true "gravity waves" so we use the terms interchangably.
The exception is that "gravity waves" in the Earth and the atmosphere can couple to LIGO through ordinary Newtonian gravity, which is something we have to think about and exclude.
> I understand that to mean that on Earth we've managed to detect that increase from 2e20N to 3e20N.
This not what how gravitational waves behave. This assumption is not correct and will confuse you.
In differential geometry, the device called a "metric" let's you define things like angles and distances on some space. This is generally denoted as g with the Greek letters mu and nu as subcripts. Just to give you a feel of what's going on, I'll leave out the subscripts, but what OP's saying is that
g = k + h
which says that g, the space-time metric, decomposes into some known, usually easy to work with metric k, plus some perturbations on top, h. In the math you put restrictions on h to make precise the "small perturbations" part.Anyway, what Gravity Waves boil down to are situations (read distributions of matter) that cause h to obey the wave equation. In other words, gravitational waves are spacetimes that have a component that waves "on top" of a given reference "background" spacetime. Of course, you could cherry pick your background such that anything looks like waves on top, but typically we choose the background to be Minkowskian (i.e. flat).
FWIW, the above perturbative approach is called Linearized Gravity and is kind of a (nice) hack to restrict study of the really hairy non-linear Einstein Equation to cases that are manageable.
Importantly, gravitational waves are not waves of Newtonian gravity. Gravitational waves do not "push and pull" along the direction of propagation. They stretch and compress space along axes perpendicular to the direction of propagation.
> E.g., if the moon suddenly lurched towards the Earth, we'd perceive an increase in gravity between the two. But that would be a semi-permanent change in the strength of that attraction between the two objects; not what I'd think of as a wave-like fluctuation.
Indeed, gravitational waves do not work this way.
Unfortunately it is hard to explain gravitational waves without significant math.
In fairness, even Einstein himself waffled over whether gravitational waves would be a real effect predicted by the theory. Then it took nearly a century to detect them experimentally, and there were plenty of doubters along the way.
The results one gets from intuition are generally incorrect in important ways. Here's a derivation of a wave equation from Einstein's field equations:
https://en.wikipedia.org/wiki/Linearized_gravity
A more helpful introduction for a layperson might be the paper titled "Gravitational Waves on the back of an envelope":
https://aapt.scitation.org/doi/10.1119/1.13627
But, infuriatingly, that paper does not seem to be open-access. Here's someone's scanned copy:
https://www.ru.ac.za/media/rhodesuniversity/content/mathemat...
Try sci-hub.
Is it possible to compress space?
Space is a mathematical abstraction. You can do anything with, because it's just math. If you want to bend, curve, distort, rip space, or add more dimensions — go for it.
Physical medium should be compressible, like any other medium. Higgs «field» (let's call it Higgium — Higgs+Vacuum) is presented everywhere, because Higgs boson gives mass to every particle in the Visible Universe and beyond, so it should conduct gravitational waves. As demonstrated by LIGO/VIRGO, gravitational waves causes distortions in light travel. These distortions can be explained as changes of conductivity in Higgium, which can be caused by changes in density, so yes, it can be waves of compression.
The Higgs is a scalar field; gravitational waves are spin-2.
Spin-0 particles are round particles, like o (like ball), or something that cannot rotate at all. Spin-2 particles are symmetrical particles, like 8 (like H2 molecule).
For spin-0, it can be changes in density only. For spin-2, it can be changes in orientation, in rotation speed, in rotation orientation, Dzhanibekov effect, wobbling, and some other if it has more complex shape, e.g. two spirals connected.
The geodesic distance between inertial test masses increases and decreases.
Colloquially we say that space has stretched and compressed.
Geodesic distance can be measured by the time it takes light to travel between the points.
Inertial test masses can be simulated by hanging them from fine wires (LIGO) or by setting them up in an orbital constellation (LISA).
This may be, likely is, a stupid question, but how do you measure this if space itself is stretched or compressed? Won't any yardstick lying in that space also be stretched or compressed? Or is it a matter of this distortion of space changing geodesics through it so light following a straight line will end up in a different place? It seems that LIGO uses interferometry to measure a change in distance between two points, though, and I don't understand how that can be measured if space is stretched, only if space is added. Perhaps that is the answer right there: when space is stretched dimensionless particles traveling through that space are not stretched, because they are dimensionless. Or perhaps better, objects in space stretch, but their momentum vectors don't stretch.
"If light waves are stretched by gravitational waves, how can we use light as a ruler to detect gravitational waves?" https://universe.sonoma.edu/moodle/pluginfile.php/89/mod_res...
The way I explain it: The light already inside the arm cavity is stretched. But newly entering light is not. We are basically using the light as clock to measure the length of the arm. When the arm is in the "stretched" state, light will take longer to make a roundtrip in the arm. It will accumulate slightly more phase, which is measured interferometrically.
It is important that the storage time of the light in the arm is short compared to the period of the gravitational wave.
This is an interesting idea, but I think it's not right.
To be honest, even as an experimentalist who worked on LIGO, I'm not sure how to treat the effect of the g.w. on photons in the arm. Instead I think of the entire arm cavity vacuum as a giant phase modulator.
I would say that we measure space in two different directions concurrently.
> and then looking for changes in the interference pattern between light moving along each of the dimensions
This is true, but I like to push back against the use of the phrase "interference pattern." We're not looking at a "pattern", which to me brings to mind a complicated interference pattern resolved spatially. We do not resolve the "interference pattern" spatially. We measure the amplitude (er, power) of the light coming out of the interferometer with a photodiode (a single pixel, if you will.)
> In practice, gravitational waves will come from all sorts of weird angles, but they will distort each of the two dimensions differently
This is true. The detector's sensitivity to waves coming from different directions is the "antenna pattern."
> t they will distort each of the two dimensions differently and allow us to figure what direction they were propagating by the interference pattern that's observed.
With a single detector, we cannot determine the direction in which a g.w. is propagating. With a single detector and a transient (short-lived) source, we cannot tell the difference between a loud source in a direction where the detector is not very sensitive versus a quieter source in a direction where we have good sensitivity.
With a network of detectors and/or signals that persist for a long time (compared to the rotation of the earth, etc) we can resolve the source direction.
I would add that considering counterfactual situations like "if the sun were to move instantly to the right" is of limited utility. That cannot happen (violates conservation of momentum). (Granted, other thought experiments have been quite influential in this field...)
Gravitational waves are also different from changes to the amount of gravitational force. This can be seen from the fact that gravitational waves affect the distances between objects, whereas the sun which exerts far more gravitational force has no measurable effect (at least, to my knowledge rotating objects don't change length noticeably).
Electromagnetic waves are similar. The Lienard-Wiechert field formulas [1] have 2 terms. The first term describes the delayed field, and is proportional to 1/r^2, while the second describes waves and is proportional to 1/r.
[1] https://en.wikipedia.org/wiki/Li%C3%A9nard%E2%80%93Wiechert_...
So the idea isn't that space itself is storing information, just that a gravitational wave doesn't put everything back where it found it. Presumably if you cleared out all the stuff, there would be no memory left behind.
But I wonder, notwithstanding the article's assertion, are objects really completely restored back to their former position in spacetime? Spatial coordinates, sure, but timewise? I don't claim to know the answer, just posing this as a question, but imagine a really powerful gravitational wave going through a large object. Wouldn't it create some kind of timewise interference pattern in the object where at the peaks of oscillation, the constituent subatomic particles would feel a stronger gravitational force and age more slowly than the particles at the troughs of oscillation? So after the wave had passed, you'd be left with an object that has areas of divergent age?
I mean even with standard GR we experience aging on a gradient, in that our feet are somewhat younger than our heads thanks to the gravitational pull of the Earth. ( https://www.theatlantic.com/technology/archive/2010/09/study... )
I would not trust the text of the article. Pop science articles are often untrustworthy even on much simpler topics. Actual papers are much better sources.
> are objects really completely restored back to their former position in spacetime?
Of course not; that's impossible. Any talk about restoring objects to their original position can only mean position in space. (And since "position in space" depends on a particular choice of reference frame, one then needs to ask what reference frame.)
> the constituent subatomic particles would feel a stronger gravitational force and age more slowly than the particles at the troughs of oscillation?
The "rate of aging" does not depend on "gravitational force". In situations where such concepts as "gravitational force" and "gravitational potential" are even applicable (which will not include very strong gravitational waves in any case), the "rate of aging" depends on gravitational potential. (For example, in the vicinity of the Earth, one's altitude above the Earth affects "rate of aging".) However, one can still assess differential aging in more general situations, just not with the rule of thumb you gave.
> after the wave had passed, you'd be left with an object that has areas of divergent age?
This is possible, but, as noted above, it cannot be assessed with the rule of thumb you gave. You would have to know the details of the spacetime geometry of the gravitational wave (and you would have to be prepared for some pretty heavy duty numerical computations).
https://en.wikipedia.org/wiki/False_vacuum_decay
I guess it's not worth worrying about, because if it happened, it would happen at the speed of light and be impossible to see coming.
Bad news is 10 watts is not much, spread thru a large volume. Good news is its "easy" to measure the infra red radiation from Pioneer and Voyager space probes running less than a KW point source of energy.
I wonder if the gravity probe A and B missions would show those permanent deformations in their data.
Permanent deformation should be detected in large scale long term orbits, eventually?
Plus, it's not like galaxies are temporarily pulling on a memory foam, before releasing the pressure, so I m not sure why you think inflation (such a bad name, people think balloon) is so close to that model.
> “The memory is nothing but the change in the gravitational potential,” said Thorne, “but it’s a relativistic gravitational potential.” The energy of a passing gravitational wave creates a change in the gravitational potential; that change in potential distorts space-time, even after the wave has passed.
Gravitational waves are that energy.
Not to mention that there's no reason to assume conservation of energy still holds if the laws of physics simply change over time (which would be the case in the simplest possible theory were all interaction distances simply shrink over time).
When do two masses stop being gravitationally bound? Is that when each mass's relative speed exceeds the escape velocity of the other mass?
No, that can't be right: they could still end up in orbit - obviously gravitationally bound.
It's called thinking out loud, this is still allowed, right, or should I assume criticism and hipster-like snark must be the defining marks of subject matter expertise?
The claim read like dragging a blackhole or massive object through space permanently alters it. I never said space was a rubber-band or a balloon, you did. Most people don't understand the Big Bang wasn't a point source per se either. Pick a name and run with it.
Can anyone dumb this down a little more for me? What holds on to the deformation? If spacetime can be deformed by a gravitational wave, then how can its original be entirely decided by the amount of and the arrangement of matter nearby. Meaning: if a wave passes by, unless it impacts the arrangement of matter in the locality, then what "holds" the deformation?
If you want to talk about physics of the process, then you need to pick up a physical medium first, not an array of measurements.
that's a neat video haven't seen that slicing idea before
THere's still one "flaw" with this video: explaining that the grid "moves" is a little confusing. It doesn't move per-se, it .. evolves? ... over time. That's weird. I keep wanting to think the curves are static, but from t0->tn the grid pinches up. Yes, that's why they call it spacetime, but I have to stop and reset myself because how can the grid keep pinching up indefinitely but it doesn't it is just a concept. That is a stumbling block. 35 years after my last physics class...lol.
https://nautil.us/issue/69/patterns/how-the-universe-remembe...
I expect it may be possible in the future to confirm this, very small, persistent shift in spacetime, but not in my lifetime.
Expansion of the universe due to gravity lost in waves.
headlines.But the distance scales and force magnitudes are so far out of my experience that even with the help of math I would be hard pressed to be convinced one way or another.
"According to general relativity, every gravitational wave should leave an indelible imprint on the structure of space-time...."
All kinds of possibilities can be found in equations. The derivation of possibilities is no guarantee that they correspond with physical realities.
An earthquake leaves an undelible imprint on some matter in space-time. Different thing. The presence of stars is said to 'warp' space-time. Never saw a suggestion that the warp is permanent. Do stars orbiting a galactic center 'permanently warp' the space-time they pass through?
"How, exactly, will a passing wave distort space-time? The possibilities are literally infinite, and, puzzlingly, these possibilities are also equivalent to one another...."
Literally infinite? Colorful language, no math, no hint of why the possibilities are non-zero.
"While detecting the memory effect caused by a single gravitational wave is infeasible with current technology...."
Maybe so much speculative fiction based on no empirical evidence is no fit way to conduct science.
Well, if they can make predictions that could in principle be measured, then LIGO or some future version may become good enough to measure them (or observe their absence). That's actually one of the ways that science is conducted.
My idea is a square piece of fabric (space). You cut a single strand of fabric somewhere, which is the origin of the wave event. This affects the whole fabric as the destruction ripples throughout, and also results is a permanent scar/distortion on the fabric as a whole.
This would be amazing if true because spacetime would be rough on very tiny scales because of all the waves that passed through it.
Speculating wildly, this might even have observable quantum-level effects.
The proposal is to arrange three spacecrafts in an equilateral triangle with sides measuring 2.5 million km (for comparison, each "arm" of LIGO is 4 km long).
[1] https://en.wikipedia.org/wiki/Laser_Interferometer_Space_Ant...
If the wave imparts energy on an object and makes it move, how is that energy still available for the next object the wave goes through?
Based on conservation of energy, I would assume that friction can weaken a gravitational wave by turning some of its energy into heat.
Though if we're talking about permanently changing the location of an object, that theoretically requires a negligible amount of energy... reminds me of the magic drive in https://qntm.org/frontier
It turns out that energy is not conserved globally in General Relativity.
https://math.ucr.edu/home/baez/physics/Relativity/GR/energy_...
The objects don't move. The space between them stretches and compresses.
Now, if the gravitational wave moves through a large massive object like a star or planet, the electromagnetic forces of the "stuff" in the object will cause it to resist this stretching or compressing. I think this does cause a very very very tiny "backreaction" to the gravitational wave, weakening it slightly.
"Gravitational waves are disturbances in the curvature of spacetime, generated by accelerated masses, that propagate as waves outward from their source at the speed of light." [0]
They are hitting everything what is on their way just like sea waves are.
So as water wave is hitting rock or any other object(mass/energy) on its way gravitational waves should hit also everything and anything on their way until they lose energy and collapse.
"Gravitational waves are constantly passing Earth; however, even the strongest have a minuscule effect and their sources are generally at a great distance. For example, the waves given off by the cataclysmic final merger of GW150914 reached Earth after travelling over a billion light-years, as a ripple in spacetime that changed the length of a 4 km LIGO* arm by a thousandth of the width of a proton, proportionally equivalent to changing the distance to the nearest star outside the Solar System by one hair's width[0]."
Gravitational waves are all around us but they have minimal impact whatsoever unless I suppose some large event(source) propagates strong gravitational waves near us.
*Laser Interferometer Gravitational-Wave Observatory
When we have a gravitational wave what measurable quantity changes?
[0]https://www.esa.int/Science_Exploration/Space_Science/Gravit...
I don't doubt that science and you all are right, I'm only asking questions in the hope that there is a simple explanation that would make a light-bulb go off in my head.
Can we measure the "pull" of a specific distant mass?
Or do we measure something else like the change in distance between two points?
// we can only see the variation
Can we also see the direction from which the wave is coming from ?
Gravitational waves are vibrations in spacetime. They interact very weakly with matter. They travel at more or less the speed of light without 'hitting' any rocks. The question is what are the 'rocks' - since gravitational waves don't really interact with matter significantly, and we don't really understand the makeup or source of spacetime.
That was my original question to you, and the answer isn't obvious, because we don't actually know.
They can have big impact: "The waves can also carry off linear momentum, a possibility that has some interesting implications for astrophysics. After two supermassive black holes coalesce, emission of linear momentum can produce a "kick" with amplitude as large as 4000 km/s. This is fast enough to eject the coalesced black hole completely from its host galaxy. Even if the kick is too small to eject the black hole completely, it can remove it temporarily from the nucleus of the galaxy, after which it will oscillate about the center, eventually coming to rest. A kicked black hole can also carry a star cluster with it, forming a hyper-compact stellar system. Or it may carry gas, allowing the recoiling black hole to appear temporarily as a "naked quasar"[1].
And idk what do you mean by "source of spacetime" you mean quantum origin[2]? https://knowablemagazine.org/article/physical-world/2019/qua...
[1] https://en.wikipedia.org/wiki/Gravitational_wave
[2] https://knowablemagazine.org/article/physical-world/2019/qua...
[1] https://www.arxiv.org/pdf/0706.0190v2
Water waves can crash into eachother. There's no reason that spacetime waves cannot either. You can get some hint of this if you look at the oscillations that comprise the Higgs field.
The negative curvature of gravitation should be cancelled out by the positive curvature of matter and energy.
Exactly it's called Frame-dragging[0]: "Frame-dragging is an effect on spacetime, predicted by Albert Einstein's general theory of relativity, that is due to non-static stationary distributions of mass–energy. A stationary field is one that is in a steady state, but the masses causing that field may be non-static -rotating, for instance."
What is spacetime made of? Nobody knows yet.
That can't be right - surely the gravitational field permeates the whole of space; and surely the wave and the force are the same thing?
Nope. This is a common misconception.
The difference between gravitational waves and gravity is a little bit like the difference between electromagnetic waves (emitted by an accelerating charge) and the electrostatic force (caused by a net charge at rest).
It's not possible to detect the effect of a charge far away, but easy to detect the propagating electromagnetic wave (light, ratio, etc).
The closest situation I can think of is ST TNG "Force of Nature", where warp travel was damaging subspace.