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pro vyhledávání: '"KONNO K"'
Autor:
Amano, T., Kawakami, Y., Itoh, H., Konno, K., Hasegawa, Y., Aoyama, T., Imai, Y., Ohgushi, K., Takeuchi, Y., Wakabayashi, Y., Goto, K., Nakamura, Y., Kishida, H., Yonemitsu, K., Iwai, S.
Publikováno v:
Phys. Rev. Res.4 L032032(2022)
In a honeycomb-lattice spin-orbit assisted Mott insulator {\alpha}-RuCl3, an ultrafast magnetization is induced by circularly polarized excitation below the Mott gap. Photo-carriers play an important role, which are generated by turning down the syne
Externí odkaz:
http://arxiv.org/abs/2207.03877
Publikováno v:
Journal of the European Optical Society-Rapid Publications, Vol 10, p 15017 (2015)
We developed a ray tracing simulation tool for imaging systems including a Fresnel lens with a quasi-arbitrary sidewall structure. One issue with Fresnel lens is that noise in the image plane can appear from rays passing through or reflected at its s
Externí odkaz:
https://doaj.org/article/e78067b467fa4984badbd5ab5aa994b4
Publikováno v:
In Computational Materials Science 15 February 2022 203
Autor:
Nobukane, H., Inagaki, K., Ichimura, K., Yamaya, K., Takayanagi, S., Kawasaki, I., Tenya, K., Amitsuka, H., Konno, K., Asano, Y., Tanda, S.
Publikováno v:
Solid State Communications 149 (2009) 1212-1215
We observed an unconventional parity-violating vortex in single domain Sr2RuO4 single crystals using a transport measurement. The current-voltage characteristics of submicron Sr2RuO4 shows that the induced voltage has anomalous components which are e
Externí odkaz:
http://arxiv.org/abs/0806.2201
Publikováno v:
In Computational Materials Science October 2018 153:297-302
Autor:
Konno, K.
Publikováno v:
Astron.Astrophys.372:594,2001
We consider principal moments of inertia of axisymmetric, magnetically deformed stars in the context of general relativity. The general expression for the moment of inertia with respect to the symmetric axis is obtained. The numerical estimates are d
Externí odkaz:
http://arxiv.org/abs/gr-qc/0105015
Publikováno v:
Astron.Astrophys.356:234-237,2000
We calculated the ellipticity of the deformed star due to the rotation or magnetic field. These two effects are compared to each other within general relativity. It turned out that the magnetic distortion is important for recently observed candidates
Externí odkaz:
http://arxiv.org/abs/astro-ph/0001397
Publikováno v:
Astron.Astrophys.352:211-216,1999
We formulate deformation of relativistic stars due to the magnetic stress, considering the magnetic fields to be perturbations from spherical stars. The ellipticity for the dipole magnetic field is calculated for some stellar models. We have found th
Externí odkaz:
http://arxiv.org/abs/gr-qc/9910038
Publikováno v:
In Cement and Concrete Composites November 2016 74:236-243
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