11 results on '"Kurbatov, E."'
Search Results
2. Turbulent convection in protoplanetary discs and its role in angular momentum transfer
- Author
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Kurbatov, E. P. and Pavlyuchenkov, Ya. N.
- Subjects
Astrophysics - Solar and Stellar Astrophysics ,Astrophysics - Earth and Planetary Astrophysics ,Astrophysics - Instrumentation and Methods for Astrophysics - Abstract
We present a model for the transport of anisotropic turbulence in an accretion disc. The model uses the Reynolds stress tensor approach in the mean field approximation. To study the role of convection in a protoplanetary disc, we combine the turbulence model with a radiative transfer calculation, and also include convection using the mixing length approximation. We find that the turbulence generated by convection causes the angular momentum of the accretion disc to be directed outwards. We also confirm the conclusions of other authors that turbulent convection is unable to provide the observed disc accretion rates as well as a heat source sufficient for the convection to be self-sustaining. The reasons for the latter are the strong anisotropy of the turbulence together with the low efficiency of the energy transfer from the background velocity shear to the turbulent stress tensor., Comment: MNRAS accepted | 15 pages, 8 figures
- Published
- 2023
3. The SHiP experiment at the proposed CERN SPS Beam Dump Facility
- Author
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Ahdida, C., Akmete, A., Albanese, R., Alt, J., Alexandrov, A., Anokhina, A., Aoki, S., Arduini, G., Atkin, E., Azorskiy, N., Back, J. J., Bagulya, A., Baaltasar Dos Santos, F., Baranov, A., Bardou, F., Barker, G. J., Battistin, M., Bauche, J., Bay, A., Bayliss, V., Berdnikov, A. Y., Berdnikov, Y. A., Betancourt, C., Bezshyiko, I., Bezshyyko, O., Bick, D., Bieschke, S., Blanco, A., Boehm, J., Bogomilov, M., Boiarska, I., Bondarenko, K., Bonivento, W. M., Borburgh, J., Boyarsky, A., Brenner, R., Breton, D., Brignoli, A., Büscher, V., Buonaura, A., Buontempo, S., Cadeddu, S., Calviani, M., Campanelli, M., Casolino, M., Charitonidis, N., Chau, P., Chauveau, J., Chepurnov, A., Chernyavskiy, M., Choi, K.-Y., Chumakov, A., Climescu, M., Conaboy, A., Congedo, L., Cornelis, K., Cristinziani, M., Crupano, A., Dallavalle, G. M., Datwyler, A., D’Ambrosio, N., D’Appollonio, G., de Asmundis, R., De Carvalho Saraiva, J., De Lellis, G., de Magistris, M., De Roeck, A., De Serio, M., De Simone, D., Dedenko, L., Dergachev, P., Di Crescenzo, A., Di Giulio, L., Dib, C., Dijkstra, H., Dmitrenko, V., Dougherty, L. A., Dolmatov, A., Donskov, S., Drohan, V., Dubreuil, A., Durhan, O., Ehlert, M., Elikkaya, E., Enik, T., Etenko, A., Fedin, O., Fedotovs, F., Ferrillo, M., Ferro-Luzzi, M., Filippov, K., Fini, R. A., Fischer, H., Fonte, P., Franco, C., Fraser, M., Fresa, R., Froeschl, R., Fukuda, T., Galati, G., Gall, J., Gatignon, L., Gavrilov, G., Gentile, V., Goddard, B., Golinka-Bezshyyko, L., Golovatiuk, A., Golovtsov, V., Golubkov, D., Golutvin, A., Gorbounov, P., Gorbunov, D., Gorbunov, S., Gorkavenko, V., Gorshenkov, M., Grachev, V., Grandchamp, A. L., Graverini, E., Grenard, J.-L., Grenier, D., Grichine, V., Gruzinskii, N., Guler, A. M., Guz, Yu., Haefeli, G. J., Hagner, C., Hakobyan, H., Harris, I. W., van Herwijnen, E., Hessler, C., Hollnagel, A., Hosseini, B., Hushchyn, M., Iaselli, G., Iuliano, A., Jacobsson, R., Joković, D., Jonker, M., Kadenko, I., Kain, V., Kaiser, B., Kamiscioglu, C., Karpenkov, D., Kershaw, K., Khabibullin, M., Khalikov, E., Khaustov, G., Khoriauli, G., Khotyantsev, A., Kim, Y. G., Kim, V., Kitagawa, N., Ko, J.-W., Kodama, K., Kolesnikov, A., Kolev, D. I., Kolosov, V., Komatsu, M., Kono, A., Konovalova, N., Kormannshaus, S., Korol, I., Korol’ko, I., Korzenev, A., Koukovini Platia, E., Kovalenko, S., Krasilnikova, I., Kudenko, Y., Kurbatov, E., Kurbatov, P., Kurochka, V., Kuznetsova, E., Lacker, H. M., Lamont, M., Lantwin, O., Lauria, A., Lee, K. S., Lee, K. Y., Leonardo, N., Lévy, J.-M., Loschiavo, V. P., Lopes, L., Lopez Sola, E., Lyons, F., Lyubovitskij, V., Maalmi, J., Magnan, A.-M., Maleev, V., Malinin, A., Manabe, Y., Managadze, A. K., Manfredi, M., Marsh, S., Marshall, A. M., Mefodev, A., Mermod, P., Miano, A., Mikado, S., Mikhaylov, Yu., Mikulenko, A., Milstead, D. A., Mineev, O., Montesi, M. C., Morishima, K., Movchan, S., Muttoni, Y., Naganawa, N., Nakamura, M., Nakano, T., Nasybulin, S., Ninin, P., Nishio, A., Obinyakov, B., Ogawa, S., Okateva, N., Osborne, J., Ovchynnikov, M., Owtscharenko, N., Owen, P. H., Pacholek, P., Park, B. D., Pastore, A., Patel, M., Pereyma, D., Perillo-Marcone, A., Petkov, G. L., Petridis, K., Petrov, A., Podgrudkov, D., Poliakov, V., Polukhina, N., Prieto Prieto, J., Prokudin, M., Prota, A., Quercia, A., Rademakers, A., Rakai, A., Ratnikov, F., Rawlings, T., Redi, F., Reghunath, A., Ricciardi, S., Rinaldesi, M., Rodin, Volodymyr, Rodin, Viktor, Robbe, P., Rodrigues Cavalcante, A. B., Roganova, T., Rokujo, H., Rosa, G., Ruchayskiy, O., Ruf, T., Samoylenko, V., Samsonov, V., Sanchez Galan, F., Santos Diaz, P., Sanz Ull, A., Sato, O., Savchenko, E. S., Schliwinski, J. S., Schmidt-Parzefall, W., Schumann, M., Serra, N., Sgobba, S., Shadura, O., Shakin, A., Shaposhnikov, M., Shatalov, P., Shchedrina, T., Shchutska, L., Shevchenko, V., Shibuya, H., Shihora, L., Shirobokov, S., Shustov, A., Silverstein, S. B., Simone, S., Simoniello, R., Skorokhvatov, M., Smirnov, S., Soares, G., Sohn, J. Y., Sokolenko, A., Solodko, E., Starkov, N., Stoel, L., Stramaglia, M. E., Sukhonos, D., Suzuki, Y., Takahashi, S., Tastet, J. L., Teterin, P., Than Naing, S., Timiryasov, I., Tioukov, V., Tommasini, D., Torii, M., Treille, D., Tsenov, R., Ulin, S., Ursov, E., Ustyuzhanin, A., Uteshev, Z., Uvarov, L., Vankova-Kirilova, G., Vannucci, F., Venkova, P., Venturi, V., Vidulin, I., Vilchinski, S., Vincke, Heinz, Vincke, Helmut, Visone, C., Vlasik, K., Volkov, A., Voronkov, R., van Waasen, S., Wanke, R., Wertelaers, P., Williams, O., Woo, J.-K., Wurm, M., Xella, S., Yilmaz, D., Yilmazer, A. U., Yoon, C. S., Zaytsev, Yu., Zelenov, A., and Zimmerman, J.
- Published
- 2022
- Full Text
- View/download PDF
4. Biological Activity study of the Melampyrum sylvaticum Extract
- Author
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Galishevskaya, E. E., primary, Polyakova, E. N., additional, Bombela, T. V., additional, Agafontseva, A. V., additional, Anisimova, A. G., additional, Krotkova, O. A., additional, Yagontseva, T. A., additional, Luzhanin, V. G., additional, and Kurbatov, E. R., additional
- Published
- 2023
- Full Text
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5. Analysis and Evaluation of Prospects for the Development of New Drugs Derived from Benzodiazepines
- Author
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Porseva, N. Yu., primary, Sobin, F. V., additional, Soloninina, A. V., additional, Pulina, N. A., additional, Kurbatov, E. R., additional, and Dvorskaya, O. N., additional
- Published
- 2023
- Full Text
- View/download PDF
6. Turbulent convection in protoplanetary discs and its role in angular momentum transfer
- Author
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Kurbatov, E P, primary and Pavlyuchenkov, Ya N, additional
- Published
- 2023
- Full Text
- View/download PDF
7. Turbulent convection in protoplanetary discs and its role in angular momentum transfer.
- Author
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Kurbatov, E P and Pavlyuchenkov, Ya N
- Subjects
- *
PROTOPLANETARY disks , *ANGULAR momentum (Mechanics) , *MOMENTUM transfer , *REYNOLDS stress , *ACCRETION disks - Abstract
We present a model for the transport of anisotropic turbulence in an accretion disc. The model uses the Reynolds stress tensor approach in the mean field approximation. To study the role of convection in a protoplanetary disc, we combine the turbulence model with a radiative transfer calculation, and also include convection using the mixing length approximation. We find that the turbulence generated by convection causes the angular momentum of the accretion disc to be directed outwards. We also confirm the conclusions of other authors that turbulent convection is unable to provide the observed disc accretion rates as well as a heat source sufficient for the convection to be self-sustaining. The reasons for the latter are the strong anisotropy of the turbulence together with the low efficiency of the energy transfer from the background velocity shear to the turbulent stress tensor. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
- View/download PDF
8. Validation Testing of Sabouraud Liquid Medium in Determining the Antifungal Activity of Newly Synthesized compounds by the Method of Two-fold Serial Dilutions
- Author
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Novikova, V. V., primary, Pulina, N. A., additional, Luzhanin, V. G., additional, and Kurbatov, E. R., additional
- Published
- 2022
- Full Text
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9. The turbulent convection in protoplanetary disks and its role in the angular momentum transfer
- Author
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Kurbatov, E. P. and Pavlyuchenkov, Ya. N.
- Subjects
Earth and Planetary Astrophysics (astro-ph.EP) ,Astrophysics - Solar and Stellar Astrophysics ,FOS: Physical sciences ,Astrophysics - Instrumentation and Methods for Astrophysics ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,Solar and Stellar Astrophysics (astro-ph.SR) ,Astrophysics - Earth and Planetary Astrophysics - Abstract
A model for the transport of anisotropic turbulence in an accretion disk is presented. This model is based on the mean field approximation and is designed to study turbulence of various nature and its role in the redistribution of the angular momentum of the accretion disk. The mean field approach makes it possible to take into account various types of instabilities by adding appropriate sources in the form of moments of fluctuations of hydrodynamic quantities. We used the model to study the role of convective instability in a gaseous and dusty circumstellar disk in the framework of a one-dimensional approximation. To do this, it was combined with the calculation of radiative transfer and with the calculation of the convective flow in the mixing length theory approximation. Within this framework, we confirm the conclusions of other authors that the turbulence generated by convection does not provide the observable disk accretion rates and sufficient heat source for which convection would be self-sustaining. The reasons for this are the strong anisotropy of turbulence in the disk, as well as the fact that convection turns out to be too weak source for turbulence., Comment: Submitted to MNRAS | 12 pages, 4 figures
- Published
- 2023
- Full Text
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10. BDF/SHiP at the ECN3 high-intensity beam facility
- Author
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Aberle, O, Ahdida, C, Albanese, R, Alt, J, Alexandrov, A, Aoki, S, Aritunov, D, Arrutia, P, Bay, A, Balazs, K, Betancourt, C, Bezshyiko, I, Bezshyyko, O, Bick, D, Blanco, A, Bogomilov, M, Boiarska, I, Bondarenko, K, Bonivento, W M, Boyarsky, A, Bohles, M, Breton, D, Brignoli, A, Buonaura, A, Buontempo, S, Calviani, M, Campanelli, M, Centanni, D, Choi, K-Y, Climescu, M, Conaboy, A, Congedo, L, Cristinziani, M, Crupano, A, Dallavalle, G M, D'Ambrosio, N, de Asmundis, R, de Bryas, P, De Carvalho Saraiva, J, De Lellis, G, de Magistris, M, De Roeck, A, De Serio, M, De Simone, D, Dergachev, P, Deucher, P, Di Crescenzo, A, Dijkstra, H, Durhan, O, Dutheil, Y, Elikkaya, E, Esposito, L S, Fedotovs, F, Ferrillo, M, Ferro-Luzzi, M, Fini, R A, Fiorillo, G, Fischer, H, Fonte, P, Franqueira Ximenes, R, Fraser, M, Fresa, R, Fukuda, T, Galati, G, Galleazzi, F, Gilardoni, S, Golinka-Bezshyyko, L, Golovatiuk, A, Golutvin, A, Gorkavenko, V, Graverini, E, Grenard, J-L, Grewing, C, Griesemer, T, Guler, A M, Haefeli, G J, Hagner, C, Helo, J C, van Herwijnen, E, Hollnagel, A, Iuliano, A, Jacobsson, R, Jonker, M, Kadenko, I, Kain, V, Kamiscioglu, C, Kim, Y G, Kitagawa, N, Kodama, K, Kolev, D I, Komatsu, M, Kostyukhin, V, Krzempek, L, Kuleshov, S, Kurbatov, E, Lacker, H M, Lafarge, D, Lantwin, O, Lauria, A, Lee, K S, Lee, K Y, Leonardo, N, Loschiavo, V P, Lopes, L, Lyons, F, Maalmi, J, Magnan, A-M, Marsh, S, Marshall, A M, Martin Ruiz, J M, Mazzola, G, Mena Andrade, R F, Miano, A, Mikado, S, Mikulenko, A, Montesi, M C, Morishima, K, Muttoni, Y, Naganawa, N, Nakamura, M, Nakano, T, Navascues Cornago, A, Ninin, P, Ogawa, S, Osborne, J, Ovchynnikov, M, Owtscharenko, N, Park, B D, Pastore, A, Patel, M, Petridis, K, Prota, A, Quercia, A, Rademakers, A, Ramjiawan, R, Ratnikov, F, Redi, F, Reghunath, A, Rokujo, H, Ruchayskiy, O, Ruf, T, Sanchez Galan, F, Santos Dias, P, Sato, O, Schmidt-Parzefall, W, Schumann, M, Serra, N, Shaposhnikov, M, Shchutska, L, Shibuya, H, Simone, S, Soares, G, Sohn, J Y, Sokolenko, A, Soto, O, Takahashi, S, Tastet, J L, Timiryasov, I, Tioukov, V, Tommasini, D, Treille, D, Tsenov, R, Ulloa, P, Ursov, E, Vankova-Kirilova, G, Velotti, F, Vilchinski, S, Vincke, H, Visone, C, van Waasen, S, Vojtyla, P, Wertelaers, P, Wurm, M, Xella, S, Yilmaz, D, Yoon, C S, and Zamora Saa, J
- Subjects
Detectors and Experimental Techniques - Abstract
The BDF/SHiP collaboration has proposed a general-purpose intensity-frontier experimental facility operating in beam-dump mode at the CERN SPS accelerator to search for feebly interacting GeV-scale particles and to perform measurements in neutrino physics. BDF/SHiP complements the world-wide program of New Physics searches by exploring a large region of parameter space which cannot be addressed by other experiments, and which reaches several orders of magnitude below existing bounds. The SHiP detector is sensitive both to decay and scattering signatures of models with heavy neutral leptons, dark photons, dark scalars, axion-like particles, light dark matter and other feebly interacting particles. In neutrino physics, BDF/SHiP can perform unprecedented measurements with tau neutrinos and neutrino-induced charm production. Following the Technical Proposal submitted in 2015, the subsequent three-year Comprehensive Design Study (CDS), and the recent study of BDF/SHiP in existing beam facilities around the SPS, this paper restates the motivation and reports on the implementation and physics performance of BDF/SHiP in the SPS ECN3 high-intensity beam facility.
- Published
- 2022
11. Track reconstruction and matching between emulsion and silicon pixel detectors for the SHiP-charm experiment
- Author
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Ahdida, C., Akmete, A., Albanese, R., Alt, J., Alexandrov, A., Anokhina, A., Aoki, S., Arduini, G., Atkin, E., Azorskiy, N., Back, J.J., Bagulya, A., Baaltasar Dos Santos, F., Baranov, A., Bardou, F., Barker, G.J., Battistin, M., Bauche, J., Bay, A., Bayliss, V., Bencivenni, G., Berdnikov, A.Y., Berdnikov, Y.A., Bertani, M., Betancourt, C., Bezshyiko, I., Bezshyyko, O., Bick, D., Bieschke, S., Blanco, A., Boehm, J., Bogomilov, M., Boiarska, I., Bondarenko, K., Bonivento, W.M., Borburgh, J., Boyarsky, A., Brenner, R., Breton, D., Brignoli, A., Büscher, V., Buonaura, A., Buonocore, L., Buontempo, S., Cadeddu, S., Calcaterra, A., Calviani, M., Campanelli, M., Casolino, M., Charitonidis, N., Chau, P., Chauveau, J., Chepurnov, A., Chernyavskiy, M., Choi, K.Y., Chumakov, A., Ciambrone, P., Cicero, V., Climescu, M., Conaboy, A., Congedo, L., Cornelis, K., Cristinziani, M., Crupano, A., Dallavalle, G.M., Datwyler, A., D'ambrosio, N., D'appollonio, G., De Asmundis, R., De Carvalho Saraiva, J., De Lellis, G., De Magistris, M., De Roeck, A., De Serio, M., De Simone, D., Dedenko, L., Dergachev, P., Di Crescenzo, A., Di Giulio, L., Di Marco, N., Dib, C., Dijkstra, H., Dmitrenko, V., Dougherty, L.A., Dolmatov, A., Domenici, D., Donskov, S., Drohan, V., Dubreuil, A., Durhan, O., Ehlert, M., Elikkaya, E., Enik, T., Etenko, A., Fabbri, F., Fedin, O., Fedotovs, F., Felici, G., Ferrillo, M., Ferro-Luzzi, M., Filippov, K., Fini, R.A., Fischer, H., Fonte, P., Franco, C., Fraser, M., Fresa, R., Froeschl, R., Frugiuele, C., Fukuda, T., Galati, G., Gall, J., Gatignon, L., Gavrilov, G., Gentile, V., Goddard, B., Golinka-Bezshyyko, L., Golovatiuk, A., Golovtsov, V., Golubkov, D., Golutvin, A., Gorbounov, P., Gorbunov, D., Gorbunov, S., Gorkavenko, V., Gorshenkov, M., Grachev, V., Grandchamp, A.L., Graverini, E., Grenard, J.L., Grenier, D., Grichine, V., Gruzinskii, N., Guler, A.M., Guz, Yu, Haefeli, G.J., Hagner, C., Hakobyan, H., Harris, I.W., Van Herwijnen, E., Hessler, C., Hollnagel, A., Hosseini, B., Hushchyn, M., Iaselli, G., Iuliano, A., Jacobsson, R., Joković, D., Jonker, M., Kadenko, I., Kain, V., Kaiser, B., Kamiscioglu, C., Karpenkov, D., Kershaw, K., Khabibullin, M., Khalikov, E., Khaustov, G., Khoriauli, G., Khotyantsev, A., Kim, Y.G., Kim, V., Kitagawa, N., Ko, J.W., Kodama, K., Kolesnikov, A., Kolev, D.I., Kolosov, V., Komatsu, M., Kono, A., Konovalova, N., Kormannshaus, S., Korol, I., Korol'ko, I., Korzenev, A., Kostyukhin, V., Koukovini Platia, E., Kovalenko, S., Krasilnikova, I., Kudenko, Y., Kurbatov, E., Kurbatov, P., Kurochka, V., Kuznetsova, E., Lacker, H.M., Lamont, M., Lanfranchi, G., Lantwin, O., Lauria, A., Lee, K.S., Lee, K.Y., Leonardo, N., Lévy, J.M., Loschiavo, V.P., Lopes, L., Lopez Sola, E., Maltoni, F., Lyons, F., Lyubovitskij, V., Maalmi, J., Magnan, A.M., Maleev, V., Malinin, A., Manabe, Y., Managadze, A.K., Manfredi, M., Marsh, S., Marshall, A.M., Mattelaer, O., Mefodev, A., Mermod, P., Miano, A., Mikado, S., Mikhaylov, Y.U., Mikulenko, A., Milstead, D.A., Mineev, O., Montanari, A., Montesi, M.C., Morishima, K., Movchan, S., Muttoni, Y., Naganawa, N., Nakamura, M., Nakano, T., Nasybulin, S., Ninin, P., Nishio, A., Novikov, A., Obinyakov, B., Ogawa, S., Okateva, N., Opitz, B., Osborne, J., Ovchynnikov, M., Owtscharenko, N., Owen, P.H., Pacholek, P., Paoloni, A., Park, B.D., Pastore, A., Patel, M., Pereyma, D., Perillo-Marcone, A., Petkov, G.L., Petridis, K., Petrov, A., Podgrudkov, D., Poliakov, V., Polukhina, N., Prieto Prieto, J., Prokudin, M., Prota, A., Quercia, A., Rademakers, A., Rakai, A., Ratnikov, F., Rawlings, T., Redi, F., Reghunath, A., Ricciardi, S., Rinaldesi, M., Rodin, Volodymyr, Rodin, Viktor, Robbe, P., Rodrigues Cavalcante, A.B., Roganova, T., Rokujo, H., Rosa, G., Rovelli, T., Ruchayskiy, O., Ruf, T., Samoylenko, V., Samsonov, V., Sanchez Galan, F., Santos Diaz, P., Sanz Ull, A., Saputi, A., Sato, O., Savchenko, E.S., Schliwinski, J.S., Schmidt-Parzefall, W., Schumann, M., Serra, N., Sgobba, S., Shadura, O., Shakin, A., Shaposhnikov, M., Shatalov, P., Shchedrina, T., Shchutska, L., Shevchenko, V., Shibuya, H., Shihora, L., Shirobokov, S., Shustov, A., Silverstein, S.B., Simone, S., Simoniello, R., Skorokhvatov, M., Smirnov, S., Soares, G., Sohn, J.Y., Sokolenko, A., Solodko, E., Starkov, N., Stoel, L., Stramaglia, M.E., Sukhonos, D., Suzuki, Y., Takahashi, S., Tastet, J.L., Teterin, P., Than Naing, S., Timiryasov, I., Tioukov, V., Tommasini, D., Torii, M., Tosi, N., Tramontano, F., Treille, D., Tsenov, R., Ulin, S., Ursov, E., Ustyuzhanin, A., Uteshev, Z., Uvarov, L., Vankova-Kirilova, G., Vannucci, F., Venkova, P., Venturi, V., Vidulin, I., Vilchinski, S., Vincke, Heinz, Vincke, Helmut, Visone, C., Vlasik, K., Volkov, A., Voronkov, R., Van Waasen, S., Wanke, R., Wertelaers, P., Williams, O., Woo, J.K., Wurm, M., Xella, S., Yilmaz, D., Yilmazer, A.U., Yoon, C.S., Zaytsev, Y.U., Zelenov, A., Zimmerman, J., Ahdida, C., Akmete, A., Albanese, R., Alt, J., Alexandrov, A., Anokhina, A., Aoki, S., Arduini, G., Atkin, E., Azorskiy, N., Back, J. J., Bagulya, A., Baaltasar Dos Santos, F., Baranov, A., Bardou, F., Barker, G. J., Battistin, M., Bauche, J., Bay, A., Bayliss, V., Bencivenni, G., Berdnikov, A. Y., Berdnikov, Y. A., Bertani, M., Betancourt, C., Bezshyiko, I., Bezshyyko, O., Bick, D., Bieschke, S., Blanco, A., Boehm, J., Bogomilov, M., Boiarska, I., Bondarenko, K., Bonivento, W. M., Borburgh, J., Boyarsky, A., Brenner, R., Breton, D., Brignoli, A., Buscher, V., Buonaura, A., Buontempo, S., Cadeddu, S., Calcaterra, A., Calviani, M., Campanelli, M., Casolino, M., Charitonidis, N., Chau, P., Chauveau, J., Chepurnov, A., Chernyavskiy, M., Choi, K. -Y., Chumakov, A., Ciambrone, P., Cicero, V., Climescu, M., Conaboy, A., Congedo, L., Cornelis, K., Cristinziani, M., Crupano, A., Dallavalle, G. M., Datwyler, A., D'Ambrosio, N., D'Appollonio, G., De Asmundis, R., De Carvalho Saraiva, J., De Lellis, G., De Magistris, M., De Roeck, A., De Serio, M., De Simone, D., Dedenko, L., Dergachev, P., Di Crescenzo, A., Di Giulio, L., Di Marco, N., Dib, C., Dijkstra, H., Dmitrenko, V., Dougherty, L. A., Dolmatov, A., Domenici, D., Donskov, S., Drohan, V., Dubreuil, A., Durhan, O., Ehlert, M., Elikkaya, E., Enik, T., Etenko, A., Fabbri, F., Fedin, O., Fedotovs, F., Felici, G., Ferrillo, M., Ferro-Luzzi, M., Filippov, K., Fini, R. A., Fischer, H., Fonte, P., Franco, C., Fraser, M., Fresa, R., Froeschl, R., Fukuda, T., Galati, G., Gall, J., Gatignon, L., Gavrilov, G., Gentile, V., Goddard, B., Golinka-Bezshyyko, L., Golovatiuk, A., Golovtsov, V., Golubkov, D., Golutvin, A., Gorbounov, P., Gorbunov, D., Gorbunov, S., Gorkavenko, V., Gorshenkov, M., Grachev, V., Grandchamp, A. L., Graverini, E., Grenard, J. -L., Grenier, D., Grichine, V., Gruzinskii, N., Guler, A. M., Guz, Y., Haefeli, G. 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- Subjects
sources ,Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,Detector alignment and calibration methods (lasers, sources, particle-beams) ,FOS: Physical sciences ,Accelerator Physics and Instrumentation ,cluster finding ,Pattern recognition ,ddc:610 ,Detectors and Experimental Techniques ,Nuclear Experiment ,Instrumentation ,physics.ins-det ,QC ,Mathematical Physics ,Particle tracking detectors (Solid-state detectors) ,Pattern recognition, cluster finding, calibration and fitting methods ,pattern recognition ,Acceleratorfysik och instrumentering ,Instrumentation and Detectors (physics.ins-det) ,particle-beams) ,calibration and fitting methods ,detector alignment and calibration methods (lasers ,Detector alignment and calibration methods (lasers ,High Energy Physics::Experiment - Abstract
In July 2018 an optimization run for the proposed charm cross section measurement for SHiP was performed at the CERN SPS. A heavy, moving target instrumented with nuclear emulsion films followed by a silicon pixel tracker was installed in front of the Goliath magnet at the H4 proton beamline. Behind the magnet, scintillating-fibre, drift-tube and RPC detectors were placed. The purpose of this run was to validate the measurement's feasibility, to develop the required analysis tools and fine-tune the detector layout. In this paper, we present the track reconstruction in the pixel tracker and the track matching with the moving emulsion detector. The pixel detector performed as expected and it is shown that, after proper alignment, a vertex matching rate of 87 % is achieved., 10 pages, 5 figures; for replacement: added detector efficiencies and track resolution, updated description of moving pattern and detector orientation, all opening angles now in cartesian coordinate system; Editor: Nikolaus Owtscharenko; to be published in JINST
- Published
- 2022
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