Zobrazeno 1 - 10
of 76
pro vyhledávání: '"Bratek, Ł."'
Autor:
Góra, D., Cheminant, K. Almeida, Alvarez-Castillo, D., Bratek, Ł., Dhital, N., Duffy, A. R., Homola, P., Jagoda, P., Jałocha, J., Kasztelan, M., Kopański, K., Kovacs, P., Nazari, V., Niedźwiecki, M., Ostrogórski, D., Rzecki, K., Smołek, K., Stasielak, J., Sushchov, O., Woźniak, K. W., Zamora-Saa, J.
Publikováno v:
Universe 2018, 4(11), 111
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a project dedicated to global studies of extremely extended cosmic-ray phenomena, the cosmic-ray ensembles (CRE), beyond the capabilities of existing detectors and observatories. Up to date
Externí odkaz:
http://arxiv.org/abs/1810.10410
Autor:
Cheminant, K. Almeida, Bratek, Ł, Alvarez-Castillo, D. E., Dhital, N., Góra, D., Homola, P., Kamiński, R., Kasztelan, M., Kopański, K., Kovacs, P., Krupiński, M., Magryś, M., Marek, M., Nazari, V., Niedźwiecki, M., Noga, W., Oziomek, K., Pawlik, M., Rzecki, K., Zamora-Saa, J., Simkovic, F., Smelcerz, K., Smolek, K., Staliesak, J., Sushchov, O., Woźniak, K.
Publikováno v:
Acta Physica Polonica B Proceedings Supplement, vol. 11 (num. 3) (2018) 489
In the past few years, cosmic-rays beyond the GZK cut-off ($E > 5 \times 10^{19}$ eV) have been detected by leading collaborations such as Pierre Auger Observatory. Such observations raise many questions as to how such energies can be reached and wha
Externí odkaz:
http://arxiv.org/abs/1810.06953
Autor:
Homola, P., Bhatta, G., Bratek, Ł., Bretz, T., Cheminant, K. Almeida, Castillo, D. A., Dhital, N., Devine, J., Góra, D., Jagoda, P., Jarvis, J. F., Kasztelan, M., Kopański, K., Lemański, D., Michałek, M., Nazari, V., Poznański, P., Smelcerz, K., Smolek, K., Stasielak, J., Sułek, M., Sushchov, O., Zamora-Saa, J.
Publikováno v:
CERN Proceedings, 1 (2018) 289
Although the photon structure is most efficiently studied with the accelerator instruments, there is also a scientifically complementary potential in investigations on photons produced in the outer space. This potential is already being explored with
Externí odkaz:
http://arxiv.org/abs/1804.05614
Autor:
Dhital, N., Homola, P., Jarvis, J. F., Poznanski, P., Cheminant, K. Almeida, Bratek, Ł., Bretz, T., Gora, D., Jagoda, P., Jałocha, J., Kopanski, K., Lemanski, D., Magrys, M., Nazari, V., Niedzwiedzki, J., Nocun, M., Noga, W., Ozieblo, A., Smelcerz, K., Smolek, K., Stasielak, J., Stuglik, S., Sułek, M., Sushchov, O., Zamora-Saa, J.
Publikováno v:
PoS(ICRC2017)1078
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is an infrastructure for global analysis of extremely extended cosmic-ray phenomena, so-called super-preshowers, beyond the capabilities of existing, discrete, detectors and observatories. To d
Externí odkaz:
http://arxiv.org/abs/1709.05196
Autor:
Cheminant, K. Almeida, Gora, D., Dhital, N., Homola, P., Poznanski, P., Bratek, L., Bretz, T., Jagoda, P., Jalocha, J., Jarvis, J. F., Kopanski, K., Krupinski, M., Lemanski, D., Nazari, V., Niedzwiedzki, J., Nocun, M., Noga, W., Ozieblo, A., Smelcerz, K., Smolek, K., Stasielak, J., Stuglik, S., Sulek, M., Sushchov, O., Zamora-Saa, J.
Publikováno v:
POS(ICRC2017)860
Any considerations on propagation of particles through the Universe must involve particle interactions: processes leading to production of particle cascades. While one expects existence of such cascades, the state of the art cosmic-ray research is or
Externí odkaz:
http://arxiv.org/abs/1709.05180
Autor:
Sushchov, O., Homola, P., Dhital, N., Bratek, Ł., Poznański, P., Wibig, T., Zamora-Saa, J., Cheminant, K. Almeida, Castillo, D. Alvarez, Góra, D., Jagoda, P., Jałocha, J., Jarvis, J. F., Kasztelan, M., Kopański, K., Krupiński, M., Michałek, M., Nazari, V., Smelcerz, K., Smolek, K., Stasielak, J., Sułek, M.
The main objective of the Cosmic-Ray Extremely Distributed Observatory (CREDO) is the detection and analysis of extended cosmic ray phenomena, so-called super-preshowers (SPS), using existing as well as new infrastructure (cosmic-ray observatories, e
Externí odkaz:
http://arxiv.org/abs/1709.05230
Publikováno v:
J. Phys. A: Math. Theor. 51 (2018) 135202
We study functions related to the experimentally observed Havriliak-Negami dielectric relaxation pattern in the frequency domain $\sim[1+(i\omega\tau_{0})^{\alpha}]^{-\beta}$ with $\tau_{0}$ being some characteristic time. For $\alpha = l/k< 1$ ($l$
Externí odkaz:
http://arxiv.org/abs/1611.06433
We study numerically self-trapped (polaron) states of quasiparticles (electrons, holes or excitons) in a deformable nanotube formed by a hexagonal lattice, wrapped into a cylinder (carbon- and boron nitride-type nanotube structures). We present a Ham
Externí odkaz:
http://arxiv.org/abs/cond-mat/0510338
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
In Physica D: Nonlinear Phenomena 2007 228(2):130-139
