31

If space is the measured distance between 2 objects, then saying the space expanded is nonsensical unless we have a measuring stick outside of the space fabric to measure the expansion. 2 objects moving away from themselves isn't the same as space expanding.

What measuring stick is outside space? Doppler redshift shows the relative speed of a star in relationship to us - but would have no effect on a space expansion.

Edit: There seems to have been some confusion (very possibly on my part) on the nature of my question. I'm not talking about an explosion-type situation where matter in the universe is moving apart (with nuclear forces holding stars/planets and gravitation forces holding solar systems, and star clusters together). This is intuitive. I'm talking about statements made by physicists that "space itself" is expanding. An excerpt from a scientific American article: "the spacetime containing matter cannot remain stationary and must either expand or contract" https://www.scientificamerican.com/article/where-is-the-universe-exp/

Edit after related question presentation: So according to the answers on that related question, we should be able to measure exactly that extra energy spent holding matter together against the accelerating space-time expansion. Would radioactive decay would be speeding up too? Would it get easier and easier to split an atom? So thats how we'd measure spacetime expansion?

Mike S
  • 942
  • 1
    Related: https://physics.stackexchange.com/q/47259/2451 , https://physics.stackexchange.com/q/721/2451 , https://physics.stackexchange.com/q/300495/2451 and links therein. – Qmechanic Feb 08 '20 at 09:44
  • Comments are not for extended discussion; this conversation has been moved to chat. – rob Feb 10 '20 at 16:38
  • 1
    This is a really good question, Mike S. And yet, there's an even more brutally fundamental, utterly unanswered aspect of the theory: How can emptiness, AKA space, stretch? – White Prime Feb 10 '20 at 16:39
  • Also closely related (duplicate?) https://physics.stackexchange.com/q/223610/42637 – მამუკა ჯიბლაძე Feb 10 '20 at 17:55
  • 1
  • As you'll see by a look at the accepted answer to https://physics.stackexchange.com/questions/83531/does-time-expand-with-space-or-contract, the Sci Am bit you quoted is a little misleading: Time is not considered to expand in any immediate perception of any observer, and relativistic coordinate systems are figured with that assumption in mind, although I believe GR is consistent with the possibility that an infinite no. of observers may exist. – Edouard Mar 15 '20 at 15:28

6 Answers6

38

If spacetime itself is expanding, how could we ever tell?

It is a common question, if everything is expanding what gives the scale? The answer: by measurements of the movement of cosmic masses.

The simplest answer is seen in the analogy of the raisin bread, the raisin being matter, the dough being space expanding.

enter image description here

Why are the raisins not expanding as the loaf of bread expands, but the space between them grows? Because the raisins are held by chemical bonds, electric and magnetic forces much stronger than the expansion, and remain whole because they do not participate in the chemistry of the dough.

This is a simple analogy. A raisin (if conscious) deduces that the bread loaf is expanding because all other raisins are moving away from each other. It is not an explosion, because there is no center.that can be fitted with three dimensional kinematics.

What gives a measuring stick for the raisins to measure expansion is the geometric stability of the raisins themselves :they are made of solid matter held together by electromagnetic and strong forces and keep the size, because the effective force involved in the expansion of the loaf is by orders of magnitude smaller than strong and electromagnetic forces composing the raisin. The raisins keep their size so can deduce the expansion of the loaf because they have different chemical properties than the dough. The measuring stick is their size.

Doppler redshift shows the relative speed of a star in relationship to us - but would have no effect on a space expansion.

Doppler redshift from all directions about us, see the left image above, showed that every thing is receding from everything else. As this happens in explosions, the Big Bang cosmological model came into effect. That the atoms and molecules of matter do not expand with the expansion of the "bang" is due to the strong, electromagnetic forces holding matter together against this explosion allowing for measuring sticks in the size of stars; even the gravitational forces holding the galaxies together. The effective expansion force is very much weaker and thus the measuring sticks show a "big Bang".

It is interesting to read Hubbles biography. His observations coincided with the time General Relativity became dominant in the field of cosmology:

Starting with Albert Einstein’s 1917 paper “Kosmologische Betrachtungen zur Allgemeinen Relativitätstheorien” (“Cosmological Considerations on the General Theory of Relativity”), a number of physicists, mathematicians, and astronomers had applied general relativity to the large-scale properties of the universe. The redshift-distance relation established by Hubble and Humason was quickly meshed by various theoreticians with the general relativity-based theory of an expanding universe. The result was that by the mid-1930s the redshift-distance relationship was generally interpreted as a velocity-distance relationship such that the spectral shifts of the galaxies were a consequence of their motions. But Hubble throughout his career resisted the definite identification of the redshifts as velocity shifts.

The concept of four dimensional space time being directly connected with the masses and energy in the universe and all the variations of modelling the universe comes with General Relativity and its mathematics. The Big Bang model is a GR model and is the mainstream cosmological model at present. It models the redshifts as expansion of four dimensional space and is not falsified at present, as it is extended to fit any new observations.

The answer to:

I'm talking about statements made by physicists that "space itself" is expanding.

is that we have a General Relativity mathematical model that fits all the data and observations at present, including the redshifts, by the hypothesis that four dimensional space is expanding from an original four dimensional "region". The expansion is measurable because matter is held together much more strongly than the expansion rate.

bb

This shows a two dimensional cut of the four dimensions, time being the x axis and space the y. It is a fit to the observations, including the Hubble velocity. The other two dimensions not shown have the curvature of space too. It is the mathematical equations that give these plots, and they depend on general relativity.

We can tell, because the G.R. model fits all the data we have up to now.

See this extensive answer here.

anna v
  • 233,453
  • 9
    The raisin bread analogy works just as well for classical motion though. When a hand grenade goes off, every splinter would see every other splinter moving away, just like how we see every galaxy moving away. The question is, how can we tell that space itself is expanding in the galaxy case, but not in the grenade splinters case. – Ryan_L Feb 09 '20 at 02:34
  • 1
    I is the reason it is called the big bang and the four dimensional mathematics ( hand grenade is three dimensional) , i.e. gives the explanation in terms of space changing as a function of the mass/energy available.. The model is called general relativity, and is the main stream one. – anna v Feb 09 '20 at 05:32
  • 11
    I'm just saying the raisin bread or hand grenade analogies don't work. They don't explain the difference between things just all moving apart and the expansion of space. – Ryan_L Feb 09 '20 at 06:15
  • 1
    @Ryan_L analogies are not an explanation per se. They are in order to give an intuition how data can be gathered by the raisins ( that everybody is moving away from them) , and it is because the raisins themselves are not expanding due to the forces holding them together.. The mesuring stick is the sixe of the raisins themselves.. The mathematics of the expansion of space comes from mathematically fitting the cosmic data in four dimensions, with GR and it has successfully explained them. – anna v Feb 09 '20 at 07:52
  • 6
    The main issue with the analogies is that both the bread and the splinter “cloud” have a boundary. You are right: if the galaxies were all rushing away from a point into some empty region of space, it will look just like it does. But only if we were very far from the expansion front. We surmise our place in the universe is like every other place (Copernican principle) and thus the universe has no edge. – Andrea Feb 09 '20 at 11:07
  • 9
    I feel like This answer doesn't adequately address the question, particularly in the context of Ryan_L's addition. Matter retaining its size as distances between matter increases would be true whether the objects were physically moving away from each other or if the space itself was expanding, and this answer doesn't provide a way to be able to tell the difference between these two scenarios (which is the crux of the entire question). – Abion47 Feb 09 '20 at 16:51
  • 1
    And the heat from the oven causes the red shift. – CJ Dennis Feb 10 '20 at 02:03
  • 2
    @Ryan_L : " When a hand grenade goes off, every splinter would see every other splinter moving away". Nope. In case of the grenade, there is a central explosion driving the splinters (which were outside of the explosion), so from point of view of a splinter, some splinters are moving much faster away, while some others are moving in nearly the same direction. – vsz Feb 10 '20 at 09:10
  • 2
    @vsz If you observe fragments from an explosion that are further away from the centre, then obviously they have travelled faster in order to get there, hence there would be a relationship between velocity and distance. The idea that galaxies are just moving away from us doesn't work unless we are at (or near) the centre of the expansion. If the centre were anywhere else then the expansion we observe would not be isotropic (which it is). – ProfRob Feb 10 '20 at 09:48
  • @Ryan_L it is indicated by measurements of red-shift, that we can differ between components from actual movement (e.g galaxies moving towards the "great attractor" ) and apparent movement due to expansion of space - primarily due to seasonal changes in the measured red-shift, the resulting speed and components of the motion – eagle275 Feb 10 '20 at 14:02
  • 1
    Thanks Anna for your detailed answer. I may be confused, but I'm with Ryan's objection. I'm not talking about objects expanding in an explosion-type way, this is directly observed by the redshift. I'm talking about how we can tell that "space itself" is expanding (as is often said by physicists). I've done an edit. – Mike S Feb 10 '20 at 15:22
  • Let's put some numbers to this. Suppose every $i$th star is moving classically according to $x_i(t) = \lambda(t) u_{i}$. Then the distance between each star is $\lambda(t) |u_i - u_j|$, or in other words every distance is scaling with every other. That's a purely classical explanation for the observations of the inhabitants of the raisins: in fact, it is accurate, because bread rising is classical. Nothing in the analogy distinguishes changes in the shape of space from regular old motion. – Display Name Feb 10 '20 at 16:09
  • @MikeS I have said in the edit: it is General Relativity Theory that gives the geometry of space time curving due to masses. Putting a Big Bang at time =0 fits the data of an expanding in three dimensions uniformly universe, and because it has not been falsified,, it is the mainstream cosmology model. You have to study the mathematics of GR to understand it, as you have to study the mathematics of special relativity to understand time dilation. – anna v Feb 10 '20 at 16:32
  • @annav right, so there must be growing (and measurable) spacetime expansion forces trying to tear apart atoms (and eventually they will succeed). There must also be measurable orbital expansion on planets too then. – Mike S Feb 10 '20 at 16:38
  • There are no forces expanding atoms with strength able to split strong, electromagnetic and even gravitational attraction, in the present model of an expanding universe. The accelerated expansion measured in recent years is still very very weak. How the universe ends is a matter of research for cosmologists – anna v Feb 10 '20 at 16:58
  • @annav thanks for the update - it helped. Another thing that made it click for me was that the red-shift is the same in all directions, and since we can't happen to be in the middle of the universe, it must be everything expanding in all directions, and not just an explosion (which would have directional vectors). – Mike S Feb 11 '20 at 01:24
  • Correction of any misunderstanding here is welcome, but I think the grenade analogy doesn't take account of the spatial expansion having resulted from gravitation, which is (-as per another analogy, that of a toy magnet having a more powerful attraction, when it lifts a pin from the ground, than our entire planet has) an EXTREMELY weak force: Like Andrea was implying, there has to be a lot of matter beyond what we can see (without exhausting our resources for magnification) for it to have the observed effect, which is spatial expansion (over time) rather than relative motion. – Edouard Mar 07 '20 at 18:21
  • I don't think the bread-raisin analogy explains how the forces holding the raisins together “know” not to adjust their strength to take into account the new distance metric. For instance, the electric force is $F=kq_1 q_2/r^2$ — how does it “know” not to change its understanding of $r$ as space expands? – BallpointBen Aug 31 '23 at 22:06
  • @BallpointBen you are giving anthropic feeling to raisins. The mainstream mathematical model of classical mechanics and electrodynamics ( i.e. that fits and predicts datat) gives the answer, – anna v Sep 01 '23 at 03:47
22

NB: The nature of the question has changed since I placed this answer. This answer does not address the current version of the question. This answer addresses how we distinguish expansion of space from a model where galaxies move away from us through space (which is not straightforward).

At the moment it is Hubble's law, some indirect measurements and a bit of philosophy.

We observe that galaxies appear to move away from us, in an isotropic fashion, at a rate that is proportional to their distance from us.

Whilst one could argue that we are at (or near) the centre of this very uniform expansion it begs the question as to why Hubble's law should exist and why the universe appears isotropic to us, but wouldn't from a different position in the universe. The simplest explanation is that General Relativity applies (as we observe in a number of other cases) and we live in an expanding universe - this then means we do not need to occupy some privileged position in the universe (an erroneous assumption that has proved wrong every other time it has been made).

In such a universe, the redshift of distant galaxies is not caused by relative motion, but by the expansion of space. At high redshifts, these phenomena become distinct in that the relationship between "velocity" and redshift is different, for instance allowing "faster than light" (apparent) speeds.

So basically at present, expansion fits the facts (far) better and more simply than any of the alternatives.

A further piece of indirect evidence comes from a careful analysis of the physical conditions of gas at high redshifts, illuminated by background quasars and subtle alterations to the cosmic microwave background (CMB) spectrum, caused by the Sunyaev-Zel'dovich effect, towards galaxy clusters at low redshifts. Both of these methods give the temperature of the CMB at those locations.

In the expanding universe model, the temperature should increase as $1+z$, where $z$ is the redshift. If one instead has a non-expanding universe, and explain the CMB as due to some expanding shell of material, then the average temperature wouldn't change for distant galaxies unless the shell gas has been uniformly cooling by an amount that just happens to agree with redshift of that galaxy.

Avgoustidis et al. (2015) review the evidence for the temperature evolution of the CMB and conclude that it agrees with an adiabatic expansion to better than 1%.

Direct evidence for the expansion is on the horizon though. In an expanding universe, the speed at which galaxies move away from us can change slowly with time (and with distance) by of order 10 cm/s per year, despite their being no force on them. This is known as the redshift drift. There are plans to measure this tiny effect with the European Extremely Large Telescope over the course of a decade.

ProfRob
  • 130,455
  • Did you just imply that "something of infinite size getting bigger" is the simplest explanation...? – Sod Almighty Feb 09 '20 at 22:06
  • 1
    @SodAlmighty when you put something in quotes it usually means you are citing something that was written. – ProfRob Feb 09 '20 at 22:23
  • Good post +1. “Direct evidence for the expansion is on the horizon though.” - Assuming there is a horizon. What if the metric is not Friedmann, space expands, but there is no horizon? – safesphere Feb 10 '20 at 00:34
  • 10 cm/s per what? 10 cm/s^2? 10 cm/s per year? – CJ Dennis Feb 10 '20 at 02:10
  • 1
    @CJDennis The linked question says 10 cm/s/yr, but yes, that should be editing into the question. – Michael Feb 10 '20 at 02:51
  • 1
    @CJDennis fixed, thanks. – ProfRob Feb 10 '20 at 07:26
  • But does not checking Hubble's law require some way to measure distances to galaxies independently of redshift? Because if so, one could in principle also observe gradual increase of these distances - or are these measurements too imprecise for that? – მამუკა ჯიბლაძე Feb 10 '20 at 09:22
  • 1
    @მამუკაჯიბლაძე Measuring redshift drift isn't checking Hubble's law. It is finding whether the recession velocities of galaxies are changing with time. It does not require the distance to be known. Establishing Hubble's law does require distance measurements and there are obviously many ways to do that. Distances would increase with time whether the universe is expanding or galaxies are simply moving away, so this does not provide a test between the two ideas, and as you correctly surmise, the distance measurements are insufficiently precise anyway. – ProfRob Feb 10 '20 at 09:43
  • @safesphere at least someone spotted the pun. – ProfRob Feb 10 '20 at 09:52
  • "we do not need to occupy some privileged position in the universe (an erroneous assumption that has proved wrong every other time it has been made)" This interests me. Can you provide a link to some examples of where this assumption has been made and proven wrong? – LarsH Feb 10 '20 at 18:37
  • 2
    @LarsH The Greeks, Ptolemy, almost the whole of pre-renaissance astronomy, the debate about the "nature of spiral nebulae" 100 years ago, assuming that the solar system was typical only 30 years ago. If one includes the assumption that we are the centre of things, then you could even include the nature of gamma ray bursts (although many suspected these were cosmological). – ProfRob Feb 10 '20 at 19:28
  • @Rob thanks for these. Can you provide a link to something about specific assumptions being proven wrong? "The Greeks, Ptolemy, almost the whole of pre-renaissance astronomy" is very vague, and includes widespread beliefs that the earth was not at a central or "privileged" position in the universe (e.g. it was at the "bottom"). So specificity would be helpful here. – LarsH Feb 11 '20 at 15:38
  • @LarsH https://www.princeton.edu/~hos/mike/texts/ptolemy/ptolemy.html – ProfRob Feb 11 '20 at 17:03
  • Besides having failed historically over the millennia is there any experimental/observational evidence that would contradict our privileged position regarding the Hubble expansion? – hyportnex Mar 07 '20 at 20:06
  • @hyportnex well there's the CMB dipole. – ProfRob Mar 07 '20 at 21:01
  • does that cover both isotropy and homogeneity? – hyportnex Mar 07 '20 at 22:37
  • @hyportnex surely it shows the we aren't at the (exact) centre of anything. I'm not sure where homogeneity comes into it. I guess I don't understand your question. – ProfRob Mar 07 '20 at 23:05
  • Even if radar pulse is reflected indirectly (multipath, not line-of -sight) from a target I can derive useful information about the target from several simultaneous reflections. Is there an experimental way to figure out how would a distant galaxy "see" the CMB? – hyportnex Mar 07 '20 at 23:13
3

Take the model that the space has a net positive curvature so that it is like a 3-sphere. Then take a cross-section through that 3-sphere, and you get a 2-sphere, which we can picture as the surface (N.B. the surface only, not the interior) of a spherical balloon located in an abstract Euclidean space.

The statement that space is expanding corresponds to the statement that this sphere is getting larger. What it means is that if you take an ordinary steel ruler, and lay it down on the surface of the sphere, and another one next to it etc., until you go all the way around, so as to measure the circumference, then if you did the same experiment again after some time has passed, then you will need more of these steel rulers. The reason is that the space expanded but the steel rulers did not.

To do such an experiment in our universe, the rulers would have to be millions of lightyears long, and you would have to wait a billion years to get an appreciable effect, but these are mere technical details....

Finally, I used the circumference of a closed universe to make the point. One could instead measure other properties, such as the distances between a large enough collection of galaxies. Then the observations can be made for a spatially flat or open universe too. But even such universes can also have a finite circumference if they have an unusual topology (though in that case they would not be isotropic).

Andrew Steane
  • 58,183
  • 1
    Would a flat 3-torus not be isotopic? – safesphere Feb 08 '20 at 09:59
  • @safesphere locally isotropic; globally not – Andrew Steane Feb 08 '20 at 10:53
  • Can you please elaborate? Why not globally isotopic? To explain my doubt, let us consider the reduced number of dimensions by 2. A 1-torus is a circular line. If the 1+1 dimensional universe is an expanding circle, why would it not be globally isotopic? All matter points around this line can be and always remain equally spaced. This symmetry persists in higher dimensions. Why do you think it would break? – safesphere Feb 08 '20 at 17:31
  • 3
    Stand on a 2-torus; walk along a geodesic in some direction. Depending on your direction of travel, you may come back on yourself after going once around, or only after winding many times around. – Andrew Steane Feb 08 '20 at 17:47
  • 2
    Got it. Thank you! +1 – safesphere Feb 08 '20 at 19:50
  • @FacingDownZ it is a thought-experiment, serving to clarify a physical concept – Andrew Steane Feb 10 '20 at 14:36
  • 1
    So to say "space itself" is expanding is also to say that the speaker believes space is finite. If space was already infinite (as in a nothingness waiting for matter to expand into it), physicists wouldn't be talking about "space itself" expanding. They must be talking about some sort of "quantum foam" substrate that has to expand to host an ever-growing universe within. In their world view, what would happen when an object hit the edge of the "space" and space stopped expanding? – Mike S Feb 10 '20 at 15:46
  • 2
    "The reason is that the space expanded but the steel rulers did not." So in your balloon analogy, the surface of the balloon is space, and the rulers are ... what? And why did they not expand? – LarsH Feb 10 '20 at 19:13
  • 1
    In the analogy the rulers correspond directly to ordinary steel rulers: collections of atoms held together by electromagnetic forces. They do not expand because those electromagnetic forces (covalent and metallic bonds) prevent the atoms from being in free fall with respect to one another. The increase in the amount of space does not exert any force. It is just makes more room. The galaxy-clusters get further apart because they are on diverging trajectories (geodesics) which they follow in free fall. – Andrew Steane Feb 10 '20 at 23:52
  • @LarsH see also https://physics.stackexchange.com/questions/2110/why-does-space-expansion-not-expand-matter/441211#441211 – Andrew Steane Feb 10 '20 at 23:58
  • Thanks, I think that's helping, though I don't completely get it yet. If "space itself is expanding" simply means "the increase in the amount of space", which "just makes more room," then I don't see how it contributes anything to explaining phenomena like "the distances between a large enough collection of galaxies." Why should the distances between galaxies increase, just because there is more room? – LarsH Feb 11 '20 at 15:47
  • @LarsH It is because of the link between matter and spacetime. The Einstein field equation says that if all the matter is moving apart with no preferred centre, then spacetime is also dynamic in a way which stays in step with that motion. What set it all in motion is the initial conditions---which remain a profound mystery. – Andrew Steane Feb 11 '20 at 17:41
1

You could say that the closest galaxies are accelerating away from us, and the next ones are accelerating even faster, and the next ones faster still, and so on that the galaxies very far away are moving away even faster than the speed of light (well, we can only assume, because and the universe is not old enough for us to see those galaxies accelerating to FTL speed) so close to the speed of light they would be invisible.

The problem with this model is the that it would put us squarely on the center of the universe, which would be quite unlikely. It seems much more likely that, symmetrically, every galaxy sees every other accelerating away just like we see it (on average). Add to it that we expect that nothing can accelerate to FTL speed, and you get that the most likely explanation is that space itself expanding is. The simplest model that fits that scenario -- where there is no preferred center to the outwards accelerating galaxies -- is to consider that the distances is increasing everywhere and in every direction, what we summarize as "the universe is expanding".

EDIT: as Rob Jeffries comment implied, the FTL argument doesn't really makes sense, so I struck it out.

lvella
  • 979
  • Why would (impossible) acceleration to light speed be required? – ProfRob Feb 10 '20 at 15:44
  • On a second thought, it is not really necessary. If we live enough to see the farthest galaxies fall outside the observable universe, they will simply redshift into oblivion, looking to us like they have fallen through the event horizon of a black hole. – lvella Feb 10 '20 at 16:29
  • It's possible to imagine that if you were something tiny in a big enough explosion, your view point from any location in that explosion might show redshift in all directions (aka the redshift we see). The direction vector we are on from the centre of the bigbang explosion would be invisible to us. The universe is too vast to see to other sides of the explosion. – Mike S Feb 11 '20 at 01:44
  • @MikeS Well, in an explosion, the solid particles are accelerated by the expanding hot gas medium. The difference between an explosion and the expansion of the universe is that the we don't see the expanding spacetime "cooling down" and stop accelerating the galaxies away. I believe the observational evidence suggests we are still accelerating, like if the "gas medium" is getting even hotter.

    About the size, you are right, we can't see beyond CMB, so we just assume the same distribution of matter/galaxies everywhere.

    – lvella Feb 11 '20 at 09:24
1

The answer by anna v is already great, but it might be worth to elaborate on the following point. In the latest edit (v3), OP has added the following sentence:

If "space itself" is expanding, then the sizes of the atoms, planets, stars would also be expanding along with the space between them, which would make us oblivious to the "space itself" expanding.

This is wrong. Why would atoms, planets or stars expand along with the space between them? The most likely distance between the proton and the electron in a Hydrogen atom is given by the Bohr radius $a_0 = \frac{\hbar}{m_e c \alpha} \approx 5 \cdot 10^{-11} m$, it is fixed by the electromagnetic force and none of these elementary constants are changing over time.

The expanding space "inside the atom" (assuming general relativity remains valid here) does introduce a slight "drift", pulling proton and electron apart. The speed of this drift can be approximated by calculating the product of the Bohr radius and the Hubble constant, which gives a speed of approximately $10^{-28} m/s$ - way too slow to have any effect. (This is where the raisin analogy of the other answers comes into play.)

Similar considerations apply to planets and stars.

Noiralef
  • 7,238
  • 1
    "Why would atoms, planets or stars expand along with the space between them?" The premise of the question is that "space itself," not just "the space between (objects)," is expanding. If space is 3-dimensional extent, and space is expanding, then the extent of everything in space would presumably be expanding, whether it's the extent of distance between objects, or the extent (size) of an atom, planet or star. That's my intuitive understanding, and I suspect it's what lies behind the original question. If space is not simply 3-dimensional extent, clarifying that concept would be most helpful. – LarsH Feb 10 '20 at 19:07
  • 1
    Yes. Quantum space and its derivatives (location, electron shell radius etc) is an informational property linked to whatever the hell "space" is made of. it sounds strange for space to be expanding and the nuclear forces holding together the quarks to be continually adjusting like that. I guess atomic forces have to have a certain discrete quantum threshold to overcome, and therefore that explains why energy isn't draining from the atoms holding themselves together against the space expansion. G attraction isn't quantized and so why aren't all orbits slowly decaying from the expanding space? – Mike S Feb 11 '20 at 01:35
0

Yes spacetime itself is expanding, and even on the smallest scales. It is the effect of this expansion, that is almost negligible on the smallest scales (and experimentally very hard to measure), at the size of atoms for example.

Why does space expansion not expand matter?

You are basically asking how we know that it is not just the objects that are getting farther from each other (like in the famous raisinbread example), but it is the very fabric of spacetime itself that is expanding.

The answer to your question is cosmological redshift. The very quanta of light, photons, as they travel through the expanding spacetime fabric, are getting stretched, because they exist in a fabric that is being stretched, that is expanding itself.

This is how beautifully the quantum object, the photon and its wavelength shows its wave nature when traveling inside a expanding fabric, gets stretched itself, giving us the very proof.

So if you could tie two objects together with a string many light years long, to keep them at rest relative to each other, there really would be a tension in that string. That tension arises because you are forcing the objects to accelerate away from the geodesics they would otherwise follow, and it arises in the same way as the tension in the string if you suspend an object in Earth's gravity.

On the expansion of space on small distances