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pro vyhledávání: '"Daligault J"'
Autor:
Grabowski, P. E., Hansen, S. B., Murillo, M. S., Stanton, L. G., Graziani, F. R., Zylstra, A. B., Baalrud, S. D., Arnault, P., Baczewski, A. D., Benedict, L. X., Blancard, C., Certik, O., Clerouin, J., Collins, L. A., Copeland, S., Correa, A. A., Dai, J., Daligault, J., Desjarlais, M. P., Dharma-wardana, M. W. C., Faussurier, G., Haack, J., Haxhimali, T., Hayes-Sterbenz, A., Hou, Y., Hu, S. X., Jensen, D., Jungman, G., Kagan, G., Kang, D., Kress, J. D., Ma, Q., Marciante, M., Meyer, E., Rudd, R. E., Saumon, D., Shulenburger, L., Singleton Jr., R. L., Sjostrom, T., Stanek, L. J., Starrett, C. E., Ticknor, C., Valaitis, S., Venzke, J., White, A.
We present the results of the first Charged-Particle Transport Coefficient Code Comparison Workshop, which was held in Albuquerque, NM October 4-6, 2016. In this first workshop, scientists from eight institutions and four countries gathered to compar
Externí odkaz:
http://arxiv.org/abs/2007.00744
The diffusion of elements is a key process in understanding the unusual surface composition of white dwarfs stars and their spectral evolution. The diffusion coefficients of Paquette et al. (1986) have been widely used to model diffusion in white dwa
Externí odkaz:
http://arxiv.org/abs/2005.05891
Autor:
Nordet, G., Gorny, C., Mayi, Y., Daligault, J., Dal, M., Effernelli, A., Blanchet, E., Coste, F., Peyre, P.
Publikováno v:
In Optics and Laser Technology March 2022 147
Publikováno v:
Phys. Rev. X 6, 021021 (2016)
We present a study of the collisional relaxation of ion velocities in a strongly coupled, ultracold neutral plasma on short timescales compared to the inverse collision rate. Non-exponential decay towards equilibrium for the average velocity of a tag
Externí odkaz:
http://arxiv.org/abs/1512.02288
Models of diffusion in white dwarfs universally rely on the coefficients calculated by Paquette et al. (1986). We present new calculations of diffusion coefficients based on an advanced microscopic theory of dense plasmas and a numerical simulation a
Externí odkaz:
http://arxiv.org/abs/1410.7645
In Starrett and Saumon [Phys. Rev. E 87, 013104 (2013)] a model for the calculation of electronic and ionic structures of warm and hot dense matter was described and validated. In that model the electronic structure of one "atom" in a plasma is deter
Externí odkaz:
http://arxiv.org/abs/1408.3548
A new approach to simulating warm and hot dense matter that combines density functional theory based calculations of the electronic structure to classical molecular dynamics simulations with pair interaction potentials is presented. The new method, w
Externí odkaz:
http://arxiv.org/abs/1408.2861
Autor:
Daligault, J., Gupta, S.
Publikováno v:
Astrophys.J.703:994-1011,2009
The thermal conductivity of a dense {\it multi-component} plasma is critical to the modeling of accreting neutron stars. To this end, we perform large-scale molecular dynamics simulations to calculate the static structure factor of the dense multi-co
Externí odkaz:
http://arxiv.org/abs/0905.0027
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Akademický článek
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