Kinetic screening non-monotonically suppresses or enhances scalar quadrupolar emission from equal-mass neutron star binaries depending on screening radius versus wavelength, with a dipole re-emerging linearly with mass asymmetry.
A Transport model for heavy ion collisions at RHIC
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
citation-role summary
background 2
citation-polarity summary
verdicts
UNVERDICTED 4roles
background 2polarities
background 2representative citing papers
γ-duality in the EPRL spinfoam model determines the relation between parity-even and parity-odd terms in an effective gravity theory, allowing the Barbero-Immirzi parameter to be measured from inflationary tensor observables.
Relativistic effects dominate large-scale galaxy power spectra and grow with redshift, but are largely insensitive to k-essence microphysics in Fourier space while the angular spectrum shows clearer model distinctions, especially for the tachyon.
AMPT simulations predict power-law intermittency in normalized factorial moments for charged particles in 5.44 TeV Xe-Xe collisions, with the scaling exponent varying with transverse momentum bin width.
citing papers explorer
-
Scaling behaviour of charged particles generated in Xe$-$Xe collisions at $\sqrt{s_{\rm{NN}}}$ = 5.44 TeV using the AMPT model
AMPT simulations predict power-law intermittency in normalized factorial moments for charged particles in 5.44 TeV Xe-Xe collisions, with the scaling exponent varying with transverse momentum bin width.