activity
20192022
most citedSuperconductivity to 262 kelvin via catalyzed hydrogenation of yttrium at high pressures

271 citations · 298 across the 5 of their papers we have counts for

collaborators

5 papers

cond-mat.supr-con20223 cited

Understanding Hydrogen Rich Superconductors: Importance of Effective Mass and Dirty Limit

Andrew L. Cornelius, Keith V. Lawler, Ashkan Salamat

A class of hydrogen-rich (H-rich) systems, consistent with Type II superconductivity, are known to have very high superconducting transition temperatures Tc and upper critical magn…

cond-mat.str-el202112 cited

Decoupling lattice and magnetic instabilities in frustrated CuMnO

Keith V. Lawler, Dean Smith, Shaun R. Evans +8

The MnO delafossites (=Na, Cu), are model frustrated antiferromagnets, with triangular layers of Mn~spins. At low temperatures (=65 K), a $C2/m \rightarro…

astro-ph.EP20218 cited

Implications of an improved water equation of state for water-rich planets

Chenliang Huang, David R. Rice, Zachary M. Grande +6

Water (HO), in all forms, is an important constituent in planetary bodies, controlling habitability and influencing geological activity. Under conditions found in the interio…

cond-mat.supr-con2020271 cited

Superconductivity to 262 kelvin via catalyzed hydrogenation of yttrium at high pressures

Elliot Snider, Nathan Dasenbrock-Gammon, Raymond McBride +6

Room temperature superconductivity has been achieved under high pressure in an organically derived carbonaceous sulfur hydride with a critical superconducting transition temperatur…

cond-mat.mtrl-sci20194 cited

Bond strengthening in dense H2O and implications to planetary composition

Zachary M. Grande, Chenliang Huang, Dean Smith +5

H2O is an important constituent in planetary bodies, controlling habitability and, in geologically-active bodies, plate tectonics. At pressures within the interior of many planets,…