most citedSubsolar Al/Si and Mg/Si ratios of non-carbonaceous chondrites reveal planetesimal formation during early condensation in the protoplanetary disk

49 citations

17 papers

cs.LO2020★ 6 cited

A Complete Axiomatisation for Quantifier-Free Separation Logic

Stéphane Demri, Étienne Lozes, Alessio Mansutti

We present the first complete axiomatisation for quantifier-free separation logic. The logic is equipped with the standard concrete heaplet semantics and the proof system has no ex…

math.PR2020★ 5 cited

Cumulant-cumulant relations in free probability theory from Magnus' expansion

A. Celestino, K. Ebrahimi-Fard, F. Patras +1

Relations between moments and cumulants play a central role in both classical and non-commutative probability theory. The latter allows for several distinct families of cumulants c…

astro-ph.EP2020★ 49 cited

Subsolar Al/Si and Mg/Si ratios of non-carbonaceous chondrites reveal planetesimal formation during early condensation in the protoplanetary disk

A. Morbidelli, G. Libourel, H. Palme +2

The Al/Si and Mg/Si ratios in non-carbonaceous chondrites are lower than the solar (i.e., CI-chondritic) values, in sharp contrast to the non-CI carbonaceous meteorites and the Ear…

physics.flu-dyn2020

Steady states in dual-cascade wave turbulence

V. N. Grebenev, S. B. Medvedev, S. V. Nazarenko +1

We study stationary solutions in the differential kinetic equation, which was introduced in for description of a local dual cascade wave turbulence. We give a full classification o…

math.AG2020★ 5 cited

The Hitchin connection in arbitrary characteristic

Thomas Baier, Michele Bolognesi, Johan Martens +1

We give an algebro-geometric construction of the Hitchin connection, valid also in positive characteristic (with a few exceptions). A key ingredient is a substitute for the Narasim…

astro-ph.HE2020★ 6 cited

Magnetic field screening in strong crossed electromagnetic fields

S. Campion, J. A. Rueda, R. Ruffini +1

We consider crossed electric and a magnetic fields , with , in presence of some initial number of pairs. We do…