Zobrazeno 1 - 10
of 1 782
pro vyhledávání: '"Marković, D."'
Publikováno v:
Phys. Rev. Applied 15, 034067 (2021)
Exploiting the physics of nanoelectronic devices is a major lead for implementing compact, fast, and energy efficient artificial intelligence. In this work, we propose an original road in this direction, where assemblies of spintronic resonators used
Externí odkaz:
http://arxiv.org/abs/2011.07885
Publikováno v:
In Journal of Cleaner Production 1 February 2023 386
Autor:
Fedortchenko, S., Felicetti, S., Marković, D., Jezouin, S., Keller, A., Coudreau, T., Huard, B., Milman, P.
Publikováno v:
Phys. Rev. A 95, 042313 (2017)
The ground state of a pair of ultrastrongly coupled bosonic modes is predicted to be a two-mode squeezed vacuum. However, the corresponding quantum correlations are currently unobservable in condensed matter where such a coupling can be reached, sinc
Externí odkaz:
http://arxiv.org/abs/1612.05542
Autor:
Wilgus, M.L., Abtin, F., Markovic, D., Tashkin, D.P., Phillips, J.E., Buhr, R.G., Flynn, M.J., Dembek, M., Cooper, C.B., Barjaktarevic, I.
Publikováno v:
In Respiratory Medicine February 2022 192
Autor:
Markovic, D., Lamb, F. K.
We investigate the suggestion that the frequencies of the kilohertz and other QPOs in the emission from neutron stars in low-mass X-ray binaries are generated by geodesic motion of gas clumps around the star. First we assume, following previous work,
Externí odkaz:
http://arxiv.org/abs/astro-ph/0009169
Autor:
Marković, D.1 dean.markovic@uniri.hr, Meštrović, E.2, Tomašić, V.3, Tomišić, V.4, Djaković, S.5, Namjesnik, D.4
Publikováno v:
Kemija u Industriji. 2022, Vol. 71 Issue 5/6, p386-389. 4p.
Autor:
Markovic, D.
We study the use of parallax microlensing to separate the effects of the mass function of dark massive halo objects (MHOs or `machos') on the one hand and their spatial distribution and kinematics on the other. This disentanglement is supposed to all
Externí odkaz:
http://arxiv.org/abs/astro-ph/9708100
Autor:
Markovic, D., Sommer-Larsen, J.
We study the accuracy of inference of the massive halo objects' (MHO or `Macho') mass function from microlensing events observed toward LMC. Assuming the spatial distribution and kinematics of the objects are known, the slope and the range of the MHO
Externí odkaz:
http://arxiv.org/abs/astro-ph/9609187
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Akademický článek
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