So this Kurzgesagt video talks about quark stars, and how two of them colliding could send strangelets flying towards Earth or the Sun. Now it's been said that since, theoretically (as none has been actually observed), this is a more stable state of matter, this could start a "contamination" of sorts that turns any celestial body into a ball of strange matter (essentially, a new quark star). There are articles discussing these possibilities (along with other things such as the true vacuum theory) and there have been books with the plot being that a particle accelerator created strange matter that escapes (which, from my understanding, is highly unlikely).


Now let's imagine that such a collision happens and a droplet of strange matter is sent towards the Earth. Somehow, we assume it is negatively charged and it hits the ground somewhere, while being only the size – at most – of a tennis ball (and possibly much smaller).


How fast would the conversion of matter on Earth to strange matter take? This may be explained in the articles but my lack of advanced understanding of physics and my gut reaction to equations more advanced than quadratics means the more scientific articles seem like a foreign language to me and I have not found this answered anywhere else. Would this wave be noticeable? It is regularly described as fire eating through a forest, but would it move at a similar rate? Or would it be instantaneous like the true vacuum bubble expanding that spreads at the speed of light?

Could it have a similar effect to the mysterious wave that sweeps through the Earth in the 2nd Law: Isolated System video by Muse? (while not visually looking anything like it once it's turned matter to strange matter, I'm talking about a wave that you could outrun if you had enough stamina… until you run out of planet that is).

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    $\begingroup$ Hard to tell, since all of the strangelet theory remains a theory until observed. And even then it might not behalve as supposed, and even then the speed at which it can or cannot go may be affected by a pletora of conditions. $\endgroup$ Mar 12, 2020 at 19:58

1 Answer 1


The behavior of strange matter is not well understood - least of all under the conditions we're used to on Earth! Most theoretical treatments focus on places in which strange matter is likely to be produced or remain stable, like at the centers of neutron stars. If we put our mathematician hats on, we could naïvely try to apply the known equations for strange matter conversion, but the results might be meaningless. So let's instead put our physicist hats on, and work with the limited tools we have.

There are equations for how fast matter inside a neutron star will be converted into strange matter. Originally derived in the late 1980s, they're described by Dai et al. 1995. The authors note that the condition for the conversion of the entire body to strange matter is that the conversion timescale be greater than the time required for sound to propagate through the star. This makes sense; sound speed is often used as a proxy for how quickly changes can take place inside a solid body. It's a way for information to propagate internally through objects. Astronomers refer to this as the dynamic timescale, and use it when studying the collapse of stars or gas clouds - but it's also a quantity to consider here.

(As an aside, the dynamic timescale is proportional to the inverse of the square root of the mean density: $\tau\sim(G\bar{\rho})^{-1/2}$. For Earth, this is about 28 minutes. For comparison, in a neutron star, $\tau$ is about a tenth of a millisecond.)

Dai et al. tell us that the conversion to strange matter should propagate at a speed $$v=\left[\frac{D}{\tau_w}\frac{a_0^4}{2(1-a_0)}\right]^{1/2}$$ where $D=\mu/k_BT$, with $\mu$ the chemical potential of down quarks, $a_0$ is related to the relative density of strange quarks and down quarks in strange matter, and $\tau_w$ is a characteristic timescale that encodes the reaction rate and influences of the strong nuclear force. In a neutron star, the conversion happens on the scale of seconds - much longer than the dynamical timescale, as expected.

Some takeaways:

  • $v\propto T^{-1/2}$, so in cooler bodies (and Earth is cool relative to a neutron star!), the changes should propagate quicker.
  • As Earth is composed of atoms, we should consider both the electromagnetic and strong nuclear forces when computing $\tau_w$, including intermolecular interactions. I'm not aware of treatments that take this into account.
  • Our computations of the chemical potential might have to change given that all of the existing quarks are bound into protons and neutrons that are themselves the constituents of atoms.
  • The assumptions used to derive our expression for $v$ were based on the setting of a neutron star; the equation itself may be entirely invalid.

If we put our physicist hats on, we're forced to conclude that we don't have the right tools for the job. Sure, from a mathematical point of view, we have an equation for the speed of the changes, like you wanted! From a physical point of view, however, that equation is incomplete and invalid, with parameters we can't easily calculate. On the plus side, we do know that the changes will propagate slower than the speed of sound - that much we should feel sure about. We can see that they will occur at a much slower rate than you probably expected.

  • $\begingroup$ “We don’t know because nobody’s created the equation to calculate that yet” Sounds like fertile ground for a scientific paper! $\endgroup$
    – nick012000
    Mar 13, 2020 at 10:13
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    $\begingroup$ @nick012000 Could be! (Though maybe someone's already written that paper, and my literature search didn't turn enough things up. . . I'd be super interested if someone's able to dig something else up.) $\endgroup$
    – HDE 226868
    Mar 13, 2020 at 13:56

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