The new proof broadly consists of three steps: derive the macroscopic theory from the mesoscopic one; derive the mesoscopic theory from the microscopic one; and then stitch them together in a single derivation of the macroscopic laws all the way from the microscopic ones.
The first step was previously understood, and even Hilbert himself contributed to it. Deriving the mesoscopic from the microscopic, on the other hand, has been much more mathematically challenging. Remember, the mesoscopic setting is about the collective behavior of vast numbers of particles. So Deng, Hani and Ma looked at what happens to Newton’s equations as the number of individual particles colliding and ricocheting grows to infinity and their size shrinks to zero. They proved that when you stretch Newton’s equations to these extremes, the statistical behavior of the system—or the likely behavior of a “typical” particle in the fluid—converges to the solution of the Boltzmann equation.
The purpose of this work is twofold. First we extend the derivation of Boltzmann’s equation in [26] to the periodic setting Td (d = 2,3). Second, we connect this kinetic limit to the hydrodynamic limit in the abovecited works, to obtain a full derivation of the fluid equations starting from Newton’s laws on the particle system, thereby completing Hilbert’s original program. We summarize the main theorems as follows: • Theorem 1: Derivation of the Boltzmann equation on Td (d = 2,3). Starting from a Newtonian hard-sphere particle system on the torus Td (d = 2,3) formed of N particles of diameter ε undergoing elastic collisions, and in the Boltzmann-Grad limit Nεd−1 = α, we derive the Boltzmann equation (1.1) as the effective equation for the one-particle density function of the particle system. • Theorem 2: Derivation of the incompressible Navier-Stokes-Fourier system from Newton’s laws. Starting from the same Newtonian hard-sphere particle system on the torus Td (d = 2,3) close to global equilibrium, and in an iterated limit where first N → ∞, ε → 0 with α = Nεd−1 f ixed and then α → ∞ separately (there are also other variants, see Theorem 2), we derive the incompressible Navier-Stokes-Fourier system as the effective equation for the macroscopic density and velocity of the particle system. • Theorem 3: Derivation of the compressible Euler equation from Newton’s laws. Starting from the same Newtonian hard-sphere particle system on the torus Td (d = 2,3), and in an iterated limit where first N → ∞, ε → 0 with α = Nεd−1 fixed and then α → ∞ separately (there are also other variants, see Theorem 3), we derive the compressible Euler equation as the effective equation for the macroscopic density, velocity, and temperature of the particle system.
My BIL was stuck in that region for a day before he and his family could return to Yangon. Pretty scary stuff.
Massive steel beams shaking like cooked spaghetti. You're not wrong.Seeing a window turn into a wall of liquid and then solid again is not something I will forget.
A good quake is as perspective-altering as a good trip.
Yikes. That's new for me.Massive steel beams shaking like cooked spaghetti. You're not wrong.
Not a particularly pleasant experience.Yikes. That's new for me.
No she was in Anchorage and Anchorage didn’t get hit by the tsunami.Was she affected by the tsunami?
Of course, when we are looking at which language is closest to Latin, we have to take into consideration what we mean by Latin. For example, there is Classical Latin and Ecclesiastical Latin. Also, Vulgar Latin has to be taken into consideration. Ecclesiastical Latin is based on Late Vulgar Latin with Italian pronunciation. Sardinian would certainly not be closest language to this version of Latin but to an earlier version of Vulgar Latin or Classical Latin. What is interesting is that there are actually many words that exist only in Sardinian and Romanian that descend from Latin, which lead us to interesting conclusions. It could be argued that they were both the most isolated versions of Latin and were in certain ways, more conservative.