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91探花
Beecroft building, Department of Physics, 91探花
Credit: Jack Hobhouse

Prof. J. C. Seamus Davis

Professor of Physics

Research theme

  • Fields, strings, and quantum dynamics
  • Quantum materials

Sub department

  • Condensed Matter Physics

Research groups

  • Macroscopic Quantum Matter
seamus.davis@physics.ox.ac.uk
Telephone: +353830392937
Clarendon Laboratory, room 512.40.28
  • About
  • Publications

The Physics of Pair-Density Waves: Cuprate Superconductors and Beyond

Annual Review of Condensed Matter Physics Annual Reviews 11:1 (2020) 231-270

Authors:

Daniel F Agterberg, JC S茅amus Davis, Stephen D Edkins, Eduardo Fradkin, Dale J Van Harlingen, Steven A Kivelson, Patrick A Lee, Leo Radzihovsky, John M Tranquada, Yuxuan Wang

Fractionalized pair density wave in the pseudogap phase of cuprate superconductors

Physical Review B American Physical Society (APS) 100:22 (2019) 224511

Authors:

D Chakraborty, M Grandadam, MH Hamidian, JCS Davis, Y Sidis, C P茅pin

Magnetic monopole noise

Nature Springer Nature 571:7764 (2019) 234-239

Authors:

R Dusad, Franziska Kirschner, JC Hoke, BR Roberts, A Eyal, F Flicker, GM Luke, Stephen Blundell, James Davis

Abstract:

Magnetic monopoles1-3 are hypothetical elementary particles with quantized magnetic charge. In principle, a magnetic monopole can be detected by the quantized jump in magnetic flux that it generates upon passage through a superconducting quantum interference device (SQUID)4. Following the theoretical prediction that emergent magnetic monopoles should exist in several lanthanide pyrochlore magnetic insulators5,6, including Dy2Ti2O7, the SQUID technique has been proposed for their direct detection6. However, this approach has been hindered by the high number density and the generation-recombination fluctuations expected of such thermally generated monopoles. Recently, theoretical advances have enabled the prediction of the spectral density of magnetic-flux noise from monopole generation-recombination fluctuations in these materials7,8. Here we report the development of a SQUID-based flux noise spectrometer and measurements of the frequency and temperature dependence of magnetic-flux noise generated by Dy2Ti2O7 crystals. We detect almost all of the features of magnetic-flux noise predicted for magnetic monopole plasmas7,8, including the existence of intense magnetization noise and its characteristic frequency and temperature dependence. Moreover, comparisons of simulated and measured correlation functions of the magnetic-flux noise indicate that the motions of magnetic charges are strongly correlated. Intriguingly, because the generation-recombination time constant for Dy2Ti2O7 is in the millisecond range, magnetic monopole flux noise amplified by SQUID is audible to humans.

Evidence for a vestigial nematic state in the cuprate pseudogap phase.

Proceedings of the National Academy of Sciences of the United States of America 116:27 (2019) 13249-13254

Authors:

Sourin Mukhopadhyay, Rahul Sharma, Chung Koo Kim, Stephen D Edkins, Mohammad H Hamidian, Hiroshi Eisaki, Shin-Ichi Uchida, Eun-Ah Kim, Michael J Lawler, Andrew P Mackenzie, JC S茅amus Davis, Kazuhiro Fujita

Abstract:

The CuO2 antiferromagnetic insulator is transformed by hole-doping into an exotic quantum fluid usually referred to as the pseudogap (PG) phase. Its defining characteristic is a strong suppression of the electronic density-of-states D(E) for energies |E| < [Formula: see text], where [Formula: see text] is the PG energy. Unanticipated broken-symmetry phases have been detected by a wide variety of techniques in the PG regime, most significantly a finite-Q density-wave (DW) state and a Q = 0 nematic (NE) state. Sublattice-phase-resolved imaging of electronic structure allows the doping and energy dependence of these distinct broken-symmetry states to be visualized simultaneously. Using this approach, we show that even though their reported ordering temperatures T DW and T NE are unrelated to each other, both the DW and NE states always exhibit their maximum spectral intensity at the same energy, and using independent measurements that this is the PG energy [Formula: see text] Moreover, no new energy-gap opening coincides with the appearance of the DW state (which should theoretically open an energy gap on the Fermi surface), while the observed PG opening coincides with the appearance of the NE state (which should theoretically be incapable of opening a Fermi-surface gap). We demonstrate how this perplexing phenomenology of thermal transitions and energy-gap opening at the breaking of two highly distinct symmetries may be understood as the natural consequence of a vestigial nematic state within the pseudogap phase of Bi2Sr2CaCu2O8.

Magnetic field鈥搃nduced pair density wave state in the cuprate vortex halo

Science American Association for the Advancement of Science (AAAS) 364:6444 (2019) 976-980

Authors:

SD Edkins, A Kostin, K Fujita, AP Mackenzie, H Eisaki, S Uchida, Subir Sachdev, Michael J Lawler, E-A Kim, JC S茅amus Davis, MH Hamidian

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