MOND experts: what’s the best determined value for the MOND acceleration $a_0$?
The best I found is $a_0 = 1.20 \pm 0.02 \mbox{ (rand)} \pm 0.24 \mbox{ (syst)} \times 10^{−10} h_{75}^2 \mbox{ m/s}^2$, from the 2016 paper doi: 10.1103/PhysRevLett.117.201101, with $h_{75} \equiv H_0/(75\mbox{km/s/Mpc})$.
Does anybody know of a value of $a_0$ now measured with a smaller systematic uncertainty?
Key formula for the MOND acceleration in my MOND = UAC section with the Variable Mass theory is
$$ a_0 = \frac{G M}{R^2} $$
And the following values have been plugged in for making the calculation.
Resulting in $a_0 := 1.09 \times 10^{-10}\mbox{ }m/s^2$ .
Notes.
MOND acceleration applies to the rotation curves of all disk galaxies, why use $R$ of the Milky Way?
In any case, I am asking for a measured value, not a theoretical one.
@RedshiftDrift . >MOND acceleration applies to the rotation curves of all disk galaxies, why use $R$ of the Milky Way?
Does a systematic error $\pm 0.24$ suggest that $a_0$ is a true “constant” for all galaxies ? And the Milky Way is just an example, of course. Would you rather prefer the Andromeda?
Giving $a_0 = 0.7\times 10^{-10}\mbox{ } ms^{-2}$ . >In any case, I am asking for a measured value, not a theoretical one.
Calculating $a_0$ from the definition $F= m (a^2/a_0)$ , how does that count as a “measured value” ?
@HanDeBruijn The systematic error on $a_0$ results from our inaccurate knowledge of the luminosity-to-mass ratio $\Upsilon_\star$ for all galaxies (hence it’s called ‘systematic’). Milgrom and other astronomers have shown that $a_0$ is dependent on $\Upsilon_\star$, but $a_0$ is the same for all galaxies.
Since your equation gives a result that varies with the mass and size of the specific galaxy, you are not calculating a fundamental constant in UAC theory. In any case, the measured values of $m_{galaxy}$ you use all depend on $\Upsilon_\star$ (that’s how they know the mass of galaxies). So your numbers also have the systematic uncertainty of $\Upsilon_\star$, and therefore cannot be more accurate than the $a_0$ given above.
Every measured value depends on a model or a theory. In MOND, it turns out that for whatever $F$, $m$ and $a$ observed in galaxies, the same $a_0$ comes out. Think of $F = Gmm’/r^2$ : for any measured $F$, $m$, $m’$ and $r$, the same constant $G$ comes out. $G$ is the measured value of a fundamental constant in Newtonian gravity theory.
${\rm }$ What I am asking above can be rephrased as: what’s the best known value for $\Upsilon_\star$ ? Or is there a measurement of $a_0$ that does not require the mass of galaxies?
The only “theoretical” mathematics of the (PDF) paper seems to be contained in this equation:
$$ \large g_{obs} = \frac{g_{bar}}{1-e^{-\sqrt{g_{bar}/g_\dagger}}} \qquad (4) $$
where $g=$ acceleration, obs = observed, bar = baryonic, $\dagger =$ their one fit parameter is the acceleration scale. However, I find (4) much too complicated. With a series expansion for the exponential function it may be simplified to
$$ \large g_{obs} \approx \frac{g_{bar}}{\sqrt{g_{bar}/g_\dagger}} = \sqrt{g_{bar}.g_\dagger} $$
So we have the geometric mean of two accelerations. And with MOND = UAC as before, tacitly assuming that $a_0=g_\dagger$ :
$$ g_{obs} \approx \sqrt{\frac{GM}{r^2}.\frac{GM}{R^2}} = \frac{GM}{Rr} = \frac{V_f^2}{r} $$
Resulting in a flat Velocity profile $V_f$ indeed:
$$ V_f = \sqrt{\frac{GM}{R}} $$
Remaining symbols have been defined in a previous posting and the references. But now we actually have two different theories for MOdified Newtonian Dynamics, namely
$$ F \approx m\frac{a^2}{a_0} \quad \mbox{(common)} \qquad \mbox{and} \qquad F \approx m\sqrt{a.a_0} \quad \mbox{(this thread)} $$
where $F=$ force, $m=$ mass and the acceleration $a_0$ on the left - in principle - is not the same as the $a_0$ on the right.
@HanDeBruijn there are two versions of MOND, one as a modification of gravity (with $g_\dagger$), and one as a modification of inertia (with $a_0$). $a_0$ and $g_\dagger$ have the same value. Milgrom doesn’t know which one to use. There are no experimental result that tells us which one to choose.
Milgrom’s law can be interpreted in two ways:
In the latter case $a_0 \equiv g_\dagger$. These equations do not describe the same force:
$$ F_i \approx m_i \frac{a_i^2}{a_0} \quad \mbox{ and} \quad F_g \approx m_g \sqrt{a_g \ g_\dagger}. $$
with $i$ for Newtonian ‘inertia’, and $g$ for Newtonian ‘gravity’.
The interpolation function $\mu \left( \frac {a}{a_0} \right)$ is not described by MOND. Two examples of an interpolation function are given on the Wiki page. My understanding is that McGaugh chooses
$$ \mu \left( \frac {g_{bar}}{g_\dagger} \right) g_{bar} = \large g_{obs} = \frac{g_{bar}}{1-e^{-\sqrt{g_{bar}/g_\dagger}}} $$
because it better fits the central part of galaxy RAR measurements.
“Milgrom’s law is not a complete and self-contained physical theory, but rather an ad hoc empirically motivated variant of one of the several equations that constitute classical mechanics.” - wikipedia
When you write MOND = UAC, which version of MOND is it?
Honestly, I didn’t know that there is also a gravitational version and that the latter is employed in the paper. Thanks! Whatever. Once established that $a_0=GM/R^2$, I have shown that UAC explains for both the two versions of MOND. It’s a bit fake to say this, however, because (MOND = UAC) is a completely different (i.e. Variable Mass) theory.
Oh yes and thank you too for the ( \dagger $\to \dagger$ ).
Two or three other quantities are related to Milgrom’s “constant” $a_0$. Calculation sequence:
A more precise account of the relationships, together with better physical underpinning, would be quite welcome !
I’m working on it!
“Dwarf galaxies tip the scales in favor of dark matter over modified gravity” https://phys.org/news/2025-10-dwarf-galaxies-scales-favor-dark.html and arXiv:2510.06905
But here is a finding of a dwarf galaxy where the dark matter they thought was there was actually a black hole:
https://mcdonaldobservatory.org/news/releases/20251027
Related https://tritonstation.com/2025/10/14/non-equilibrium-dynamics-in-galaxies-that-appear-to-have-lots-of-dark-matter-ultrafaint-dwarfs/
Related https://arxiv.org/abs/2510.02431 https://github.com/orgs/a-cosmology-group/discussions/342