Zobrazeno 1 - 10
of 288
pro vyhledávání: '"E. Morosan"'
Autor:
Jaime M. Moya, Alannah M. Hallas, Vaideesh Loganathan, C.-L. Huang, Lazar L. Kish, Adam A. Aczel, J. Beare, Y. Cai, G. M. Luke, Franziska Weickert, Andriy H. Nevidomskyy, Christos D. Malliakas, Mercouri G. Kanatzidis, Shiming Lei, Kyle Bayliff, E. Morosan
Publikováno v:
Communications Physics, Vol 5, Iss 1, Pp 1-10 (2022)
Quantum criticality, a process driven by non-thermal parameters such as magnetic field, doping or pressure, when combined with magnetism and electron correlations, can give rise to quantum phase transitions and novel physics. Here, the authors presen
Externí odkaz:
https://doaj.org/article/cfa06fbc3e3c405087656f6db353badc
Autor:
Y. Sato, S. Suetsugu, T. Tominaga, Y. Kasahara, S. Kasahara, T. Kobayashi, S. Kitagawa, K. Ishida, R. Peters, T. Shibauchi, A. H. Nevidomskyy, L. Qian, E. Morosan, Y. Matsuda
Publikováno v:
Nature Communications, Vol 13, Iss 1, Pp 1-9 (2022)
Charge-neutral excitations have been proposed to explain metal-like thermal transport in Kondo insulators. Here, the authors demonstrate the coupling between charge-neutral excitations and spin degrees of freedom in a Kondo insulator YbIr3Si7, which
Externí odkaz:
https://doaj.org/article/4fa2167e6c2f4392bdc459ce453c79c0
Autor:
Binod K. Rai, S. Chikara, Xiaxin Ding, Iain W. H. Oswald, R. Schönemann, V. Loganathan, A. M. Hallas, H. B. Cao, Macy Stavinoha, T. Chen, Haoran Man, Scott Carr, John Singleton, Vivien Zapf, Katherine A. Benavides, Julia Y. Chan, Q. R. Zhang, D. Rhodes, Y. C. Chiu, Luis Balicas, A. A. Aczel, Q. Huang, Jeffrey W. Lynn, J. Gaudet, D. A. Sokolov, H. C. Walker, D. T. Adroja, Pengcheng Dai, Andriy H. Nevidomskyy, C.-L. Huang, E. Morosan
Publikováno v:
Physical Review X, Vol 8, Iss 4, p 041047 (2018)
We report complex metamagnetic transitions in single crystals of the new low carrier Kondo antiferromagnet YbRh_{3}Si_{7}. Electrical transport, magnetization, and specific heat measurements reveal antiferromagnetic order at T_{N}=7.5 K. Neutron diff
Externí odkaz:
https://doaj.org/article/4c38ea754ecf45958e4bd5ec4150b27f
Autor:
Binod K. Rai, E. Morosan
Publikováno v:
APL Materials, Vol 3, Iss 4, Pp 041511-041511-8 (2015)
Single crystals of (Lu1−xY bx)3Rh4Ge13 were characterized by magnetization, specific heat, and electrical resistivity measurements. Doping Yb into the non-magnetic Lu3Rh4Ge13 compound tunes this cubic system’s properties from a superconductor wit
Externí odkaz:
https://doaj.org/article/7cf5f7ed8bde47348ecca23e819aa5be
Autor:
E. Svanidze, L. Liu, B. Frandsen, B. D. White, T. Besara, T. Goko, T. Medina, T. J. S. Munsie, G. M. Luke, D. Zheng, C. Q. Jin, T. Siegrist, M. B. Maple, Y. J. Uemura, E. Morosan
Publikováno v:
Physical Review X, Vol 5, Iss 1, p 019902 (2015)
Externí odkaz:
https://doaj.org/article/012b142600a84d02833091248f61e441
Autor:
E. Svanidze, L. Liu, B. Frandsen, B. D. White, T. Besara, T. Goko, T. Medina, T. J. S. Munsie, G. M. Luke, D. Zheng, C. Q. Jin, T. Siegrist, M. B. Maple, Y. J. Uemura, E. Morosan
Publikováno v:
Physical Review X, Vol 5, Iss 1, p 011026 (2015)
A quantum critical point (QCP) occurs upon chemical doping of the weak itinerant ferromagnet Sc_{3.1}In. Remarkable for a system with no local moments, the QCP is accompanied by non-Fermi liquid behavior, manifested in the logarithmic divergence of t
Externí odkaz:
https://doaj.org/article/01af7153f2944c59bfcc00f7ec8c52ec
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One of the sources of solar energetic particle (SEP) events is shocks that are driven by fast coronal mass ejections (CMEs). They can accelerate SEPs up to relativistic energies and are attributed to the largest SEP events. New studies suggest that C
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d8614afdef45a935fda4d204cdf113c0
Autor:
Christian Palmroos, Jan Gieseler, Nina Dresing, Diana E. Morosan, Eleanna Asvestari, Aleksi Yli-Laurila, Daniel J. Price, Saku Valkila, Rami Vainio
Publikováno v:
Frontiers in Astronomy and Space Sciences. 9
Solar Energetic Particles (SEPs) are charged particles accelerated within the solar atmosphere or the interplanetary space by explosive phenomena such as solar flares or Coronal Mass Ejections (CMEs). Once injected into the interplanetary space, they
Autor:
Bartosz Dabrowski, Katarzyna Mikuła, Paweł Flisek, Christian Vocks, PeiJin Zhang, Jasmina Magdalenić, Alexander Warmuth, Diana E. Morosan, Adam Froń, Richard A. Fallows, Mario M. Bisi, Andrzej Krankowski, Gottfried Mann, Leszek Błaszkiewicz, Eoin P. Carley, Peter T. Gallagher, Pietro Zucca, Paweł Rudawy, Marcin Hajduk, Kacper Kotulak, Tomasz Sidorowicz
The Sun is the source of different types of radio bursts that are associated with solar flares, for example. Among the most frequently observed phenomena are type III solar bursts. Their radio images at low frequencies (below 100 MHz) are relatively
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f865fab14a46c338db2e99bd431e3d6
http://arxiv.org/abs/2211.12756
http://arxiv.org/abs/2211.12756