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I've looked at the following pages:

I don't think any of the posts in the links quite answer what I have in my mind. I understand why people would say acceleration is an absolute quantity: An accelerometer can clearly tell us which person is accelerating and which is not.

However, if we imagine the entire universe with every particle accelerating in one direction, then the accelerometer will not be able to distinguish this from a universe that is not accelerating. The appeal to a physical accelerometer fails in this thought experiment. With this in mind, can we really say acceleration is absolute?

Perhaps we should distinguish between "global acceleration" and "relative acceleration" and say that only "relative acceleration" is absolute, but this way of phrasing things can be mapped identically to the notion of velocity ("global velocity" is not absolute and "relative velocity" is absolute). Since the validity of every statement ends up being preserved under this mapping, we find that we fail to distinguish between the situation involving velocity and the situation involving acceleration. So then my question is, how could we accurately distinguish between relativity of velocity and relativity of acceleration that satisfyingly takes into account the above thought experiment?

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    Ernst Mach had that same question. – M. Enns Jan 07 '23 at 21:26
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    What experiment do you propose to test this? – John Doty Jan 07 '23 at 21:28
  • Acceleration is absolute because to accelerate a thing you must apply a force to it, and the fact that there is an interaction between a closed system and something external to it is an absolute. See my answer here. – Stéphane Rollandin Jan 08 '23 at 00:47
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    Your thought experiment throws the baby with the bath water. For example, let's construct a similar one: 'Imagine that the whole universe ceases to exist every few seconds for a million years and then pops-up unchanged - nobody would notice'. Would that mean that the continuity of time is relative, not absolute? – Stéphane Rollandin Jan 08 '23 at 00:55
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    This post seems very closely related to my confusion. – Maximal Ideal Jan 09 '23 at 23:09
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    "Of we imagine the entire universe with every particle accelerating in one direction, then the accelerometer will not be able to distinguish this from a universe that is not accelerating. " This is a (famous) speculation that can't be checked.

    – Ján Lalinský Jan 17 '23 at 13:05
  • @JánLalinský It is true. It's similar to Einstein's thought experiment. Experiments in free fall are indistinghishable from experiments in inertial frames (inertial in the Newtonian definition). – Ryder Rude Jan 17 '23 at 15:49
  • @RyderRude it is an interesting speculation, you can assume it is true, but you have no proof. I am not sure what you mean by Newtonian definition of inertial frame, but in the frame of freely falling body, all bodies in the universe do not have the same acceleration, so the situation is not similar to the hypothetical one. – Ján Lalinský Jan 17 '23 at 15:59
  • On the contrary acceleration is more frame dependent. Upon frame or instance of its measurement due to non-linearity of its motion. Suppose if one observer measure it from time t and other from time t', then both disagree about its value. – Neil Libertine Jan 17 '23 at 16:30
  • @JánLalinský A freely falling room, under the influence of a uniform gravitational field, is a non-inertial frame in the Newtonian sense. But there is no experiment that can be done inside that room which determines its acceleration. – Ryder Rude Jan 18 '23 at 11:10
  • @JánLalinský This is very similar to OP's thought experiment. An accelerometer can only measure relative acceleration. If you drop a ball inside an accelerating train, what happens is that there's a force on the train but there's no force on the ball mid-flight (except gravity). The relative acceleration between the ball and the train is what enables you to figure out that the train is an accelerated frame. If the relative acceleration is zero, like in the case of uniform gravity, there is no experiment that can determine the acceleration of the frame. – Ryder Rude Jan 18 '23 at 11:19
  • @RyderRude > "A freely falling room, under the influence of a uniform gravitational field, is a non-inertial frame in the Newtonian sense. But there is no experiment that can be done inside that room which determines its acceleration." Actually there is: measuring changing Doppler shift of incoming radiation from distant sources. You have restricted the allowed experiments to those working only with nearby objects that experience the same gravity acceleration. OK, with that assumption, acceleration can't be determined. – Ján Lalinský Jan 18 '23 at 14:50
  • @JánLalinský That logic does not work because an inertial observer will also observe a changing Doppler shift in the light from an accelerating source. You won't be able to determine whether you are in the non-inertial frame or the source is. – Ryder Rude Jan 18 '23 at 14:54
  • @RyderRude In OP's thought experiment, observing distant objects is allowed, and it is assumed this observation reveals no acceleration of the whole even if it all accelerates in some absolute sense. This is a very strong assumption on its own, because we can't prepare the system and check its behaviour. And it is not similar to scenarios where small room accelerates due to gravity, or (!) train accelerates due to friction forces due to rails. – Ján Lalinský Jan 18 '23 at 15:19
  • "an inertial observer will also observe a changing Doppler shift in the light from an accelerating source. You won't be able to determine whether you are in the non-inertial frame or the source is." Yes, for one source and one observer it is hard to decide between the two. But we have billions of sources (distant stars), and rate of change of their Doppler shift in any frame can be tracked as function of spherical angles. When this function in observer's frame looks like "clear dipole pattern" , it's clear the observer is accelerating.

    – Ján Lalinský Jan 18 '23 at 15:39
  • One can easily change frames and change the dipole pattern in a rocket. By changing direction of exhaust, we observe different orientation of the radiation pattern from the distant stars. I don't believe rocket engine can make distant stars accelerate in an absolute sense. Similarly for planets or Sun, which can also provide such plethora of different frames. When observer changes frames, it is reasonable to say that absolute observer acceleration changes. It is not reasonable to say all distant stars' absolute accelerations change. – Ján Lalinský Jan 18 '23 at 15:50
  • @JánLalinský I know it's two months later and this question is closed, but I thought you might be interested in my own answer to my question. I tried to analyze the question from within Galilean spacetime and Minkowski spacetime (both mainstream ideas). I agree with what you have to say (and I agree my original question is poorly formulated... although that doesn't automatically mean it is a bad one). – Maximal Ideal Mar 11 '23 at 12:04
  • We need a background relative to which acceleration happens. The entire universe can't accelerate because the universe is all. If you mean a universe within which all matter constituents of the universe uniformly accelerate then there should be a symmetry loss which we can measure. – Duke William Jun 21 '23 at 16:05

2 Answers2

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This is not actually a physics question, but a question of semantics. What do people mean when they use the word "absolute" in this context?

Many authors use the term "absolute" as a synonym of "invariant". They use those words to indicate any quantity which does not depend on the choice of reference frame or coordinate system. Such authors would indeed correctly consider proper acceleration to be absolute.

Other authors use the term "absolute" to refer to quantities that are uniquely real in some metaphysical sense. Often it is in the context of some sort of aether frame or other "absolute time and space" theory. Such authors could indeed correctly consider proper acceleration to not be absolute for the reason you suggest.

So whether proper acceleration is absolute or not depends on the individual author's usage of the term. Either meaning is valid, and hopefully any given author is sufficiently clear to distinguish their meaning.

Personally, because of this ambiguity, I avoid the term "absolute" altogether except to respond to someone else using the term. I don't like the potential aether-related connotation of the second meaning and I can just use the word "invariant" instead for the first meaning. When I do use the term "absolute" I often clarify by saying "absolute or invariant" just to be explicit about my intended usage.

Dale
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I'm answering my own question to jot some thoughts of my own down. I'm not completely sure I have the right understanding, so the info here shouldn't be taken authoritatively. @Dale is largely right in saying,

This is not actually a physics question, but a question of semantics. What do people mean when they use the word "absolute" in this context?

In physics, when one says "$x$ is absolute" what is meant is "quantity $x$ is invariant under such-and-such class of transformations." I'm trying to be as general as possible so I'm not necessarily limiting myself to coordinate transformations (for example we can consider gauge transformations as well), but coordinates is what I mainly have in mind.

The key here is that generally speaking we want to restrict ourselves to transformations that keep the form of the laws/formulas of physics the same. Even if we find a transformation that changes quantity $x$, that's not enough to conclude that $x$ is relative (because those transformations that change $x$ can be accompanied by changes in the form of the laws/formulas of physics).

Short Summary

To those who will find the text below too much to read, I'll just put my conclusions here. To say it as briefly as possible,

  • The spacetime of Galilean relativity alone does not discriminate between inertial and non-inertial reference frames. You need to go to the level of Newtonian mechanics and appeal to Newton's third law: Inertial reference frames are the unique frames in which Newton's third law holds.
  • The spacetime of special relativity does allow you to discriminate between inertial and non-inertial reference frames.

In classical mechanics, relativity of acceleration breaks at the level of mechanics. In special relativity, relativity of acceleration breaks at the level of spacetime.

Newtonian Mechanics / Galilean Relativity

As far as I can tell, there is nothing in the structure of Galilean spacetime that rules out the notion that "acceleration is relative." You can in principle formulate a theory where acceleration is relative that exhibits Galilean invariance with no trouble (this is in contrast to special relativity where the spacetime structure does prevent acceleration from being relative). However, it turns out that Newtonian mechanics does not allow acceleration to be relative for different reasons.

In Newtonian mechanics, if you try to frame acceleration as relative, then you run into a contradiction with Newton's three laws (which one exactly depends on how you want to describe and phrase your model of the universe). In particular, my thought experiment where the entire universe with every particle is accelerating in one direction violates Newton's first law. If I tried to salvage my thought experiment by saying there is some force causing this uniform acceleration, then this violates Newton's third law. Daniel Kleppner says something to this effect in An Introduction to Mechanics in Section 2.6 when he writes,

Newton's third law is essential if the second law is to be meaningful: without it, there would be no way to know whether an acceleration results from a real force, or is merely an artifact of being in a non-inertial system. If the acceleration is due to a force, then somewhere in the universe there must be an equal and opposite force acting on some other body.

Really, this is the key to distinguishing inertial frames from uniformly accelerated frames. Newton's first law postulates the existence of an inertial frame, then Newton's second law describes the relationship between force and acceleration that ought to hold, and Newton's third law places a constraint on what kinds of "real forces" there can be. This in turn determines what is the class of reference frame transformations that can affect the three laws.

If the class of transformations we are considering is the class of Galilean boosts $\vec{x}\,' = \vec{x} - \vec{V}t$, then acceleration is invariant. If the class of transformations is the class of changes to linearly accelerated reference frames $\vec{x}\,' = \vec{x} - \frac{1}{2}\vec{A}t^{2}$, then acceleration is not invariant. We want to restrict ourselves to transformations that keep the form of the laws/formulas of physics the same. The transformations in the former class preserve Newton's three laws whereas the transformations in the latter class do not, because in an accelerating reference frame we either have to modify Newton's first law (as particles would accelerate without any force acting upon them) or we have to modify Newton's third law (as we would have a fictitious force that is unpaired with any other equal and opposite force). In this precise sense, it does seem that "acceleration is absolute."

Special Relativity

In special relativity, we find that acceleration fails to be relative due to the structure of spacetime (which is surprisingly different than what we found in Galilean relativity). The fact is that particles that are undergoing constant proper acceleration attain a Rindler horizon from the point of view of Rindler coordinates, so for each particle there will be a region of Minkowski space that will be rendered inaccessible to the particle as long as it is in acceleration. This is enough to distinguish whether every particle in the universe is being uniformly accelerated (like in the thought experiment) or not.

Consider an inertial reference frame with coordinates $(x^{0}, x^{1})$. If we had two objects that are at rest but at different positions, then their worldlines would be straight vertical lines in a Minkowski diagram for $x^{\mu}$-coordinates, and the particles are able to send light signals to each other without any problems. If, however, the two objects were undergoing constant proper acceleration $A\ne 0$, their worldlines would be hyperbolas in $x^{\mu}$-coordinates. If the two hyperbolas don't intersect each other, then past a certain time there will be a point where one object is no longer able to send messages to the other even though it is able to receive messages from the other. This is enough to tell whether the objects are accelerating or not.

Indeed, even though coordinate acceleration is not invariant under general spacetime coordinate transformations (apart from e.g. Lorentz transformations and translations), in special relativity you can define proper acceleration, which turns out to be invariant under all possible coordinate transformations.

Also, you don't even need to appeal to Rindler horizons. If two comoving observers are uniformly accelerating, they would observe Doppler redshifting/blueshifting when they send light to each other as they accelerate. So you can't use light to tell "absolute velocity" but you can use it to tell "absolute acceleration," so to speak.

No Global Accelerating Reference Frame in SR?

Lastly, I want to point out something else that is interesting with special relativity. As far as I understand, there is no notion of an accelerated reference frame at least in the following sense:

Given an inertial reference frame $(x^{0}, x^{1})$ there is no coordinate transformation $(x^{0}, x^{1})\rightarrow(\xi^{0}, \xi^{1})$ such that the following conditions hold:

  1. The coordinate transformation is global, i.e. every point in Minkowski space is assigned a unique coordinate $(\xi^{0}, \xi^{1})$.
  2. (a) It sends worldlines of the form $x^{\mu}(t) = (t, vt+x_{0}^{1})$ with $v\in(-1, 1)$ to worldlines of the form $$ \xi^{\mu}(t) = (\tfrac{1}{A}\sinh\lambda(t, v, x_{0}^{1}) - \xi_{0}^{0}, \tfrac{1}{A}\cosh\lambda(t, v, x_{0}^{1}) - \xi_{0}^{1}), $$ i.e. it sends constant velocity worldlines to hyperbolic motion worldlines. (b) Also, $\lambda(t, v, x_{0}^{1})$ is strictly increasing with respect to $t$ if $v$ and $x_{0}^{1}$ are kept constant (this is just to fix an orientation of our $\xi^{\mu}$-coordinates relative to the $x^{\mu}$-coordinates).

These two conditions are already contradictory.

Proof. Assume $(x^{0}, x^{1})\rightarrow (\xi^{0}, \xi^{1})$ satisfies these two conditions $(1)$ and $(2)$. Without loss of generality, we may assume it sends $(0, 0)\rightarrow (0, 0)$. We can use condition $(2)$ to deduce the form of the transformation on the quadrant $Q = \{(x^{0}, x^{1}) \,|\, 0 < x^{0},\, |x^{1}|<|x^{0}|\}$. Given a worldline $x^{\mu}(\tau) = (\tau\cosh\phi, \tau\sinh\phi)$, this ought to transform to $$ \xi^{\mu}(\lambda) = (\tfrac{1}{A}\sinh\lambda - \xi_{0}^{0}, \tfrac{1}{A}\cosh\lambda - \xi_{0}^{1}). $$ By using the fact that $(0, 0)\rightarrow(0, 0)$, rescaling the worldline parameter to normalize the derivative, shifting the parameter, and taking condition $(\text{2b})$ into account, our worldline ends up in the form $$ \xi^{\mu}(\tau) = (\tfrac{1}{A}\sinh(A\tau+\lambda_{0}(\phi)) - \tfrac{1}{A}\sinh\lambda_{0}(\phi), \tfrac{1}{A}\cosh(A\tau+\lambda_{0}(\phi)) - \tfrac{1}{A}\cosh\lambda_{0}(\phi)) $$ for some strictly increasing or decreasing function $\lambda_{0} = \lambda_{0}(\phi)$.

Using this info, we know that our transformation (if it exists) maps points $(x^{0}, x^{1})\in Q$ to $(\xi^{0}, \xi^{1})$ by \begin{align*} \xi^{0} &= \frac{1}{A}\left[ \sinh\left(A\sqrt{(x^{0})^{2} - (x^{1})^{2}} + \lambda_{0}\left(\operatorname{arctanh}\frac{x^{1}}{x^{0}}\right)\right) - \sinh\left(\lambda_{0}\left(\operatorname{arctanh}\frac{x^{1}}{x^{0}}\right)\right) \right], \\ \xi^{1} &= \frac{1}{A}\left[ \cosh\left(A\sqrt{(x^{0})^{2} - (x^{1})^{2}} + \lambda_{0}\left(\operatorname{arctanh}\frac{x^{1}}{x^{0}}\right)\right) - \cosh\left(\lambda_{0}\left(\operatorname{arctanh}\frac{x^{1}}{x^{0}}\right)\right) \right]. \end{align*}

Consider the worldline $x^{\mu}(t) = (t, b)\in Q$ for $t\in(|b|, \infty)$ where $b$ is a constant. Plugging this into what we have so far gives \begin{align}\tag{$*$} \xi^{0}(t) &= \frac{1}{A}\left[ \sinh\left(A\sqrt{t^{2} - b^{2}} + \lambda_{0}\left(\operatorname{arctanh}\frac{b}{t}\right)\right) - \sinh\left(\lambda_{0}\left(\operatorname{arctanh}\frac{b}{t}\right)\right) \right], \\ \xi^{1}(t) &= \frac{1}{A}\left[ \cosh\left(A\sqrt{t^{2} - b^{2}} + \lambda_{0}\left(\operatorname{arctanh}\frac{b}{t}\right)\right) - \cosh\left(\lambda_{0}\left(\operatorname{arctanh}\frac{b}{t}\right)\right) \right]. \end{align} By condition $(2)$, this worldline $x^{\mu}(t)$ must be sent to (a portion of) a hyperbolic path, so \begin{align}\tag{$\dagger$} \xi^{0}(t) &= \frac{1}{A}\sinh\lambda(t) - \xi_{0}^{0}, \\ \xi^{1}(t) &= \frac{1}{A}\cosh\lambda(t) - \xi_{0}^{1}. \end{align} We set the corresponding expressions to be equal. Then we consider the expression $(A\xi^{1}+A\xi_{0}^{1})^{2}-(A\xi^{0}+A\xi_{0}^{0})^{2}$. By $(\dagger)$ and the $\cosh^{2}-\sinh^{2}=1$ identity, we conclude that our expression is constant. However, using the expressions in $(*)$, if $b\ne 0$ one can show that our expression is not constant for any choice of $\xi_{0}^{0}, \xi_{0}^{1}$. This is a contradiction and so no coordinate transformation can satisfy conditions $(1)$ and $(2)$ simultaneously. $\blacksquare$

If we can't have a global uniformly accelerating reference frame in SR, then we can't say there is any symmetry between inertial frames and accelerating frames to begin with. This is somewhat surprising, because this doesn't happen in Newtonian mechanics / Galilean relativity. Rindler coordinates are often invoked to stand in for what we mean by an accelerated reference frame in SR, but they have two undesirable properties for the purposes of my question. First, they only cover a quadrant of Minkowski space, so they fail condition $(1)$. Second, each hyperbolic worldline that they describe has a different proper acceleration, so they fail condition $(2)$.

  • Kleppner's argument is not very convincing. Second law is meaningful even if we forget about the 3rd law - e.g. we can use it together with Newton's gravity law to understand planetary orbits in our solar system (and derive Kepler's laws), without ever detecting the reaction force on the Sun. The meaning is in being a useful model, both explanatory and predictive. Whether the observed Venus orbit is due to gravity force being real or apparent due to Earth being a non-inertial frame is secondary issue; this ambiguity does not rob the second law of meaning. – Ján Lalinský Mar 11 '23 at 16:02
  • A better way to point out the issue is that forces we use in the second law can be classified as "real" and "apparent". The real forces are those we identified as being due to presence of some source physical object or field. The apparent forces are those due to using a "wrong frame" - which means they can be eliminated by proper choice of frame, i.e. all Coriolis forces vanish when the frame does not rotate with respect to stars. I.e. if a class of forces (such as gravity force) can't be get rid of by changing frame, then we won't classify it as apparent and we would say it is a real force. – Ján Lalinský Mar 11 '23 at 16:09