Zobrazeno 1 - 10
of 25 285
pro vyhledávání: '"I. G. P."'
Autor:
Stefanus G. Kandinata, Novira Widajanti, Jusri Ichwani, Hadiq Firdausi, I. G. P. S. Aryana, Firas F. Alkaff
Publikováno v:
Scientific Reports, Vol 13, Iss 1, Pp 1-6 (2023)
Abstract Asian working group for sarcopenia (AWGS) recently introduced “possible sarcopenia” diagnosis for early identification of sarcopenia in the primary healthcare. For initial screening, 3 modalities, i.e. calf circumference (CC) measurement
Externí odkaz:
https://doaj.org/article/d69aaa38cbba46c8b769b43cd3f35f2a
Autor:
Dark, IAU Centre for the Protection of the, Interference, Quiet Sky from Satellite Constellation, Józsa, Gyula I. G., Williams, Andrew, Green, Richard, Marsh, Isabel, Antoniadis, John, Barbosa, Domingos, Barentine, John, Blanc, Guillermo, Coelho, Bruno, Cooper, Patricia, Dalledonne, Sara, Di Vruno, Federico, Diamond, Joe, Dong, Adam, Drimmel, Ronald, Eggl, Siegfried, Habeeb, Nusrin, Heim, Jessica, Hofer, Chris, Hwang, Narae, Isidro, Mathieu, Koplow, David, Lowenthal, James, Lucatello, Sara, Lyubenova, Mariya, Massey, Robert, Peel, Mike, Rawls, Meredith, Saada, Adrien, Sanchez, Alejandro, Sanhueza, Pedro, Skidmore, Warren, Sorokin, Boris, Sreekumar, P., Stevenson, Tim, Tartari, Paula, Tornatore, Vincenza, Walker, Connie, Winkel, Benjamin, Yakushina, Yana
The growing number of satellite constellations in low Earth orbit (LEO) enhances global communications and Earth observation, and support of space commerce is a high priority of many governments. At the same time, the proliferation of satellites in L
Externí odkaz:
http://arxiv.org/abs/2412.08244
We propose a concept of a superconducting photodiode - a device that transforms the energy and `spin' of an external electromagnetic field into the rectified steady-state supercurrent and develop a microscopic theory describing its properties. For th
Externí odkaz:
http://arxiv.org/abs/2412.03087
Given a graph $G$ with vertex set $V(G)$, a mapping $h : V(G) \rightarrow \lbrace 0, 1, 2, 3, 4, 5 \rbrace$ is called a quadruple Roman dominating function (4RDF) for $G$ if it holds the following. Every vertex $x$ such that $h(x)\in \{0,1,2, 3\}$ sa
Externí odkaz:
http://arxiv.org/abs/2411.18987
Autor:
Ahyoune, S., Altenmueller, K., Antolin, I., Basso, S., Brun, P., Candon, F. R., Castel, J. F., Cebrian, S., Chouhan, D., Della Ceca, R., Cervera-Cortes, M., Chernov, V., Civitani, M. M., Cogollos, C., Costa, E., Cotroneo, V., Dafni, T., Derbin, A., Desch, K., Diaz-Martin, M. C., Diaz-Morcillo, A., Diez-Ibanez, D., Pardos, C. Diez, Dinter, M., Doebrich, B., Drachnev, I., Dudarev, A., Ezquerro, A., Fabiani, S., Ferrer-Ribas, E., Finelli, F., Fleck, I., Galan, J., Galanti, G., Galaverni, M., Garcia, J. A., Garcia-Barcelo, J. M., Gastaldo, L., Giannotti, M., Giganon, A., Goblin, C., Goyal, N., Gu, Y., Hagge, L., Helary, L., Hengstler, D., Heuchel, D., Hoof, S., Iglesias-Marzoa, R., Iguaz, F. J., Iniguez, C., Irastorza, I. G., Jakovcic, K., Kaefer, D., Kaminski, J., Karstensen, S., Law, M., Lindner, A., Loidl, M., Loiseau, C., Lopez-Alegre, G., Lozano-Guerrero, A., Lubsandorzhiev, B., Luzon, G., Manthos, I., Margalejo, C., Marin-Franch, A., Marques, J., Marutzky, F., Menneglier, C., Mentink, M., Mertens, S., Miralda-Escude, J., Mirallas, H., Muleri, F., Muratova, V., Navarro-Madrid, J. R., Navick, X. F., Nikolopoulos, K., Notari, A., Nozik, A., Obis, L., Ortiz-de-Solorzano, A., O'Shea, T., von Oy, J., Pareschi, G., Papaevangelou, T., Perez, K., Perez, O., Picatoste, E., Pivovaroff, M. J., Porron, J., Puyuelo, M. J., Quintana, A., Redondo, J., Reuther, D., Ringwald, A., Rodrigues, M., Rubini, A., Rueda-Teruel, S., Rueda-Teruel, F., Ruiz-Choliz, E., Ruz, J., Schaffran, J., Schiffer, T., Schmidt, S., Schneekloth, U., Schoenfeld, L., Schott, M., Segui, L., Singh, U. R., Soffitta, P., Spiga, D., Stern, M., Straniero, O., Tavecchio, F., Unzhakov, E., Ushakov, N. A., Vecchi, G., Vogel, J. K., Voronin, D. M., Ward, R., Weltman, A., Wiesinger, C., Wolf, R., Yanes-Diaz, A., Yu, Y.
BabyIAXO is the intermediate stage of the International Axion Observatory (IAXO) to be hosted at DESY. Its primary goal is the detection of solar axions following the axion helioscope technique. Axions are converted into photons in a large magnet tha
Externí odkaz:
http://arxiv.org/abs/2411.13915
Autor:
Saraogi, Divita, Bala, Suman, Joshi, Jitendra, Iyyani, Shabnam, Bhalerao, Varun, Aditya, J Venkata, Svinkin, D. S., Frederiks, D. D., Lysenko, A. L., Ridnaia, A. V., Kozyrev, A. S., Golovin, D. V., Mitrofanov, I. G., Litvak, M. L., Sanin, A. B., Chattopadyay, Tanmoy, Gupta, Soumya, Waratkar, Gaurav, Bhattacharya, Dipankar, Vadawal, Santosh, Dewangan, Gulab
We present results of a comprehensive analysis of the polarization characteristics of GRB 200503A and GRB 201009A observed with the Cadmium Zinc Telluride Imager (CZTI) on board AstroSat. Despite these GRBs being reasonably bright, they were missed b
Externí odkaz:
http://arxiv.org/abs/2411.00410
The results of studies on the properties of ordinary and heavy water subjected to sharp mechanical impacts at acoustic repetition frequency are presented. Experimental evidence for the phenomenon of acoustically induced nuclear processes in water is
Externí odkaz:
http://arxiv.org/abs/2410.16213
Autor:
Ruz, J., Todarello, E., Vogel, J. K., Giannotti, M., Grefenstette, B., Hudson, H. S., Hannah, I. G., Irastorza, I. G., Kim, C. S., O'Shea, T., Regis, M., Smith, D. M., Taoso, M., Bueno, J. Trujillo
The nature of dark matter in the Universe is still an open question in astrophysics and cosmology. Axions and axion-like particles (ALPs) offer a compelling solution, and traditionally ground-based experiments have eagerly, but to date unsuccessfully
Externí odkaz:
http://arxiv.org/abs/2407.03828
Autor:
Artemenkov, D. A., Bradnova, V., Britvich, G. I., Zaitsev, A. A., Zarubin, P. I., Zarubina, I. G., Kalinin, V. A., Kattabekov, R. R., Kornegrutsa, N. K., Kostin, M. Yu., Maksimov, A. V., Mamatkulov, K. Z., Mitseva, E., Neagu, A., Pikalov, V. A., Polkovnikov, M. K., Rukoyatkin, P. A., Rusakova, V. V., Sarkisyan, V. R., Stanoeva, R., Firu, E., Haiduc, M., Kharlamov, S. P.
Publikováno v:
Physics of Atomic Nuclei, 2017, Vol. 80, No. 6, pp. 1126-1132
The results obtained by estimating the contribution of $^8$Be and $^9$B nuclei to the coherent dissociation of $^{10}$C, $^{10}$B, and $^{12}$C relativistic nuclei in nuclear track emulsions (``white'' stars) are presented. The selection of ``white''
Externí odkaz:
http://arxiv.org/abs/2409.16164
Autor:
Zaitsev, A. A., Artemenkov, D. A., Bradnova, V., Zarubin, P. I., Zarubina, I. G., Kattabekov, R. R., Kornegrutsa, N. K., Mamatkulov, K. Z., Mitsova, E. K., Neagu, A., Rukoyatkin, P. A., Rusakova, V. V., Sarkisyan, V. R., Stanoeva, R., Haiduc, M., Firu, E.
Publikováno v:
Physics of Particles and Nuclei, 2017, Vol. 48, No. 6, pp. 960-963
The structural features of $^{10}$B are studied by analyzing the dissociation of nuclei of this isotope at an energy of 1 A GeV in nuclear track emulsion. The fraction of the $^{10}$B $\to$ 2He + H channel in the charge state distribution of fragment
Externí odkaz:
http://arxiv.org/abs/2409.15002