activity
20102019
most citedFuture Physics Programme of BESIII

566 citations · 579 across the 3 of their papers we have counts for

collaborators

8 papers

hep-ex2019★ 566 cited

Future Physics Programme of BESIII

M. Ablikim, M. N. Achasov, P. Adlarson +482

There has recently been a dramatic renewal of interest in the subjects of hadron spectroscopy and charm physics. This renaissance has been driven in part by the discovery of a plet…

cond-mat.mes-hall2015★ 5 cited

Generalized Landau level representation: Effect of static screening in the quantum Hall effect in graphene

Igor A. Shovkovy, Lifang Xia

By making use of the generalized Landau level representation (GLLR) for the quasiparticle propagator, we study the effect of screening on the properties of the quantum Hall states…

hep-ph2014★ 8 cited

Chiral asymmetry in cold QED plasma in a strong magnetic field

Lifang Xia, E. V. Gorbar, V. A. Miransky +1

The interaction induced chiral asymmetry is calculated in cold QED plasma beyond the weak-field approximation. By making use of the recently developed Landau-level representation f…

hep-ex2014

Planning the Future of U.S. Particle Physics (Snowmass 2013): Chapter 8: Instrumentation Frontier

M. Demarteau, R. Lipton, H. Nicholson +211

These reports present the results of the 2013 Community Summer Study of the APS Division of Particles and Fields ("Snowmass 2013") on the future program of particle physics in the…

astro-ph.GA2013

High-Redshift Galaxies with Large Ionization Parameters

Mark L. A. Richardson, Emily M. Levesque, Emily M. McLinden +3

Motivated by recent observations of galaxies dominated by emission lines, which show evidence of being metal poor with young stellar populations, we present calculations of multipl…

astro-ph.CO2012

Metallicities of Emission-Line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4

Lifang Xia, Sangeeta Malhotra, James Rhoads +9

Galaxies selected on the basis of their emission line strength show low metallicities, regardless of their redshifts. We conclude this from a sample of faint galaxies at redshifts…