output
20022024
most citedGW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

9.8k citations

Showing 2018Show all

16 papers · 1 filter

cond-mat.soft201821 cited

Bending to kinetic energy transfer in adhesive peel front micro-instability

V. De Zotti, K. Rapina, P. -P. Cortet +2

We report an extensive experimental study of a detachment front dynamics instability, appearing at microscopic scales during the peeling of adhesive tapes. The amplitude of this in…

hep-ph2018

Basics of doubly heavy tetraquarks

A. Valcarce, J. -M. Richard, J. Vijande

We outline the most important results regarding the stability of doubly heavy tetraquarks with an adequate treatment of the four-body dynamics. We consider both co…

hep-ph20182 cited

Supersymmetry, direct and indirect constraints

F. Mahmoudi

We present an overview of direct and indirect constraints in the MSSM, in CP-conserving and CP-violating MSSM scenarios, with some emphasis on the importance of combining the const…

astro-ph.GA2018115 cited

The large and small scale properties of the intergalactic gas in the Slug Ly-alpha nebula revealed by MUSE HeII emission observations

Sebastiano Cantalupo, Gabriele Pezzulli, Simon J. Lilly +11

With a projected size of about 450 kpc at z~2.3, the Slug Ly-alpha nebula is a rare laboratory to study, in emission, the properties of the intergalactic gas in the Cosmic Web. Sin…

physics.geo-ph201821 cited

Small-Scale Metal/Silicate Equilibration During Core Formation: The Influence of Stretching Enhanced Diffusion on Mixing

Victor Lherm, Renaud Deguen

Geochemical data provide key information on the timing of accretion and on the prevailing physical conditions during core/mantle differentiation. However, their interpretation depe…

astro-ph.SR201849 cited

SPHERE dynamical and spectroscopic characterization of HD142527B

R. Claudi, A. -L. Maire, D. Mesa +50

We detect the accreting low-mass companion HD142527B at a separation of 73 mas (11.4 au) from the star. No other companions with mass greater than 10 MJ are visible in the field of…