D
Diandian Wang
Researcher at University of California, Santa Barbara
Publications - 13
Citations - 140
Diandian Wang is an academic researcher from University of California, Santa Barbara. The author has contributed to research in topics: Boundary (topology) & Black hole. The author has an hindex of 6, co-authored 13 publications receiving 100 citations. Previous affiliations of Diandian Wang include University of Cambridge.
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Journal ArticleDOI
Strong Coupling Superconductivity in a Quasiperiodic Host-Guest Structure
Philip Brown,Konstantin Semeniuk,Diandian Wang,Bartomeu Monserrat,Bartomeu Monserrat,Chris J. Pickard,Chris J. Pickard,F. Malte Grosche +7 more
TL;DR: The electronic transport and magnetization experiments establish Bi-III as a rare example of type II superconductivity in an element, with a record upper critical field of ~ 2.5 T, unusually strong electron-phonon coupling, and an anomalously large, linear temperature dependence of the electrical resistivity in the normal state.
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Descendants in celestial CFT and emergent multi-collinear factorization
TL;DR: In this article, a systematic study of conformal and Kac-Moody descendants in the OPE of celestial gluons was conducted, and the results of these OPEs were used for computing the multi-collinear limits of gluon amplitudes.
Journal ArticleDOI
Creating a traversable wormhole
TL;DR: Horowitz and Diandian as discussed by the authors constructed spacetimes in which there are instantons giving a finite probability for a test cosmic string to break and produce two particles on its ends.
Journal ArticleDOI
Descendants in celestial CFT and emergent multi-collinear factorization
TL;DR: In this article, a systematic study of conformal and Kac-Moody descendants in the OPE of celestial gluons was conducted, and the results of these OPEs were used for computing the multi-collinear limits of gluon amplitudes.
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High-energy collision of black holes in higher dimensions
TL;DR: In this paper, the authors compute the gravitational wave energy radiated in head-on collisions of equal-mass, nonspinning black holes in up to ($D=8$)-dimensional asymptotically flat spacetimes for boost velocities up to about 90% of the speed of light.