test.bib

@book{frank-kameneckiyLekciiPoFizike1968,
  title = {Лекции по физике плазмы},
  author = {Франк-Каменецкий, Д. А.},
  date = {1968},
  publisher = {{Атомиздат}},
  location = {{М.}},
  langid = {russian}
}

@book{ME,
	title = {Современная электродинамика, часть 1. Микроскопическая теория: Учебное пособие.},
	author = {Батыгин, В. В. и Топтыгин, И. Н.},
	pages = {736},
	publisher = {{Москва-Ижевск: Институт компьютерных исследований}},
	year = {2002},
	langid = {russian}
}

@incollection{sagdeevKollektivnyeProcessyUdarnye1964,
  title = {Коллективные процессы и ударные волны в разреженной плазме},
  booktitle = {Вопросы теории плазмы},
  author = {Сагдеев, Р. З.},
  date = {1964},
  publisher = {{Атомиздат}},
  location = {{М.}},
  langid = {russian}
}

@book{26Asch,
	author = {Aschwanden, M.},
	pages = {XXII, 908},
	publisher = {Springer-Verlag Berlin Heidelberg},
	title = {Physics of the Solar Corona},
	year = {2005},
}

@article{adamPlanckIntermediateResults2016,
  title = {Planck Intermediate Results - {{XLII}}. {{Large}}-Scale {{Galactic}} Magnetic Fields},
  author = {Adam, R. and Ade, P. a. R. and Alves, M. I. R. and Ashdown, M. and Aumont, J. and Baccigalupi, C. and Banday, A. J. and Barreiro, R. B. and Bartolo, N. and Battaner, E. and Benabed, K. and Benoit-Lévy, A. and Bernard, J.-P. and Bersanelli, M. and Bielewicz, P. and Bonavera, L. and Bond, J. R. and Borrill, J. and Bouchet, F. R. and Boulanger, F. and Bucher, M. and Burigana, C. and Butler, R. C. and Calabrese, E. and Cardoso, J.-F. and Catalano, A. and Chiang, H. C. and Christensen, P. R. and Colombo, L. P. L. and Combet, C. and Couchot, F. and Crill, B. P. and Curto, A. and Cuttaia, F. and Danese, L. and Davis, R. J. and de Bernardis, P. and de Rosa, A. and de Zotti, G. and Delabrouille, J. and Dickinson, C. and Diego, J. M. and Dolag, K. and Doré, O. and Ducout, A. and Dupac, X. and Elsner, F. and Enßlin, T. A. and Eriksen, H. K. and Ferrière, K. and Finelli, F. and Forni, O. and Frailis, M. and Fraisse, A. A. and Franceschi, E. and Galeotta, S. and Ganga, K. and Ghosh, T. and Giard, M. and Gjerløw, E. and González-Nuevo, J. and Górski, K. M. and Gregorio, A. and Gruppuso, A. and Gudmundsson, J. E. and Hansen, F. K. and Harrison, D. L. and Hernández-Monteagudo, C. and Herranz, D. and Hildebrandt, S. R. and Hobson, M. and Hornstrup, A. and Hurier, G. and Jaffe, A. H. and Jaffe, T. R. and Jones, W. C. and Juvela, M. and Keihänen, E. and Keskitalo, R. and Kisner, T. S. and Knoche, J. and Kunz, M. and Kurki-Suonio, H. and Lamarre, J.-M. and Lasenby, A. and Lattanzi, M. and Lawrence, C. R. and Leahy, J. P. and Leonardi, R. and Levrier, F. and Liguori, M. and Lilje, P. B. and Linden-Vørnle, M. and López-Caniego, M. and Lubin, P. M. and Macías-Pérez, J. F. and Maggio, G. and Maino, D. and Mandolesi, N. and Mangilli, A. and Maris, M. and Martin, P. G. and Martínez-González, E. and Masi, S. and Matarrese, S. and Melchiorri, A. and Mennella, A. and Migliaccio, M. and Miville-Deschênes, M.-A. and Moneti, A. and Montier, L. and Morgante, G. and Munshi, D. and Murphy, J. A. and Naselsky, P. and Nati, F. and Natoli, P. and Nørgaard-Nielsen, H. U. and Oppermann, N. and Orlando, E. and Pagano, L. and Pajot, F. and Paladini, R. and Paoletti, D. and Pasian, F. and Perotto, L. and Pettorino, V. and Piacentini, F. and Piat, M. and Pierpaoli, E. and Plaszczynski, S. and Pointecouteau, E. and Polenta, G. and Ponthieu, N. and Pratt, G. W. and Prunet, S. and Puget, J.-L. and Rachen, J. P. and Reinecke, M. and Remazeilles, M. and Renault, C. and Renzi, A. and Ristorcelli, I. and Rocha, G. and Rossetti, M. and Roudier, G. and Rubiño-Martín, J. A. and Rusholme, B. and Sandri, M. and Santos, D. and Savelainen, M. and Scott, D. and Spencer, L. D. and Stolyarov, V. and Stompor, R. and Strong, A. W. and Sudiwala, R. and Sunyaev, R. and Suur-Uski, A.-S. and Sygnet, J.-F. and Tauber, J. A. and Terenzi, L. and Toffolatti, L. and Tomasi, M. and Tristram, M. and Tucci, M. and Valenziano, L. and Valiviita, J. and Tent, F. Van and Vielva, P. and Villa, F. and Wade, L. A. and Wandelt, B. D. and Wehus, I. K. and Yvon, D. and Zacchei, A. and Zonca, A.},
  date = {2016-12-01},
  journaltitle = {A\&A},
  volume = {596},
  pages = {A103},
  publisher = {{EDP Sciences}},
  issn = {0004-6361, 1432-0746},
  doi = {10.1051/0004-6361/201528033},
  url = {https://www.aanda.org/articles/aa/abs/2016/12/aa28033-15/aa28033-15.html},
  urldate = {2021-05-23},
  abstract = {Recent models for the large-scale Galactic magnetic fields in the literature have been largely constrained by synchrotron emission and Faraday rotation measures. We use three different but representative models to compare their predicted polarized synchrotron and dust emission with that measured by the \emph{Planck {$<$}i/{$>$}satellite. We first update these models to match the \emph{Planck {$<$}i/{$>$}synchrotron products using a common model for the cosmic-ray leptons. We discuss the impact on this analysis of the ongoing problems of component separation in the \emph{Planck {$<$}i/{$>$}microwave bands and of the uncertain cosmic-ray spectrum. In particular, the inferred degree of ordering in the magnetic fields is sensitive to these systematic uncertainties, and we further show the importance of considering the expected variations in the observables in addition to their mean morphology. We then compare the resulting simulated emission to the observed dust polarization and find that the dust predictions do not match the morphology in the \emph{Planck {$<$}i/{$>$}data but underpredict the dust polarization away from the plane. We modify one of the models to roughly match both observables at high latitudes by increasing the field ordering in the thin disc near the observer. Though this specific analysis is dependent on the component separation issues, we present the improved model as a proof of concept for how these studies can be advanced in future using complementary information from ongoing and planned observational projects.}}}}},
  file = {/home/ivan/Zotero/storage/4GQW49G8/Adam et al. - 2016 - Planck intermediate results - XLII. Large-scale Ga.pdf;/home/ivan/Zotero/storage/IEZJXD5G/aa28033-15.html},
  langid = {english}
}

@article{maldacenaLargeNLimitSuperconformal1999,
  title = {The {{Large}}-{{N Limit}} of {{Superconformal Field Theories}} and {{Supergravity}}},
  author = {Maldacena, Juan},
  date = {1999-04-01},
  journaltitle = {International Journal of Theoretical Physics},
  volume = {38},
  pages = {1113--1133},
  issn = {1572-9575},
  doi = {10.1023/A:1026654312961},
  url = {https://doi.org/10.1023/A:1026654312961},
  urldate = {2021-05-23},
  abstract = {We show that the large-N limits of certainconformal field theories in various dimensions includein their Hilbert space a sector describing supergravityon the product of anti-de Sitter spacetimes, spheres, and other compact manifolds. This is shown bytaking some branes in the full M/string theory and thentaking a low-energy limit where the field theory on thebrane decouples from the bulk. We observe that, in this limit, we can still trust thenear-horizon geometry for large N. The enhancedsupersymmetries of the near-horizon geometry correspondto the extra supersymmetry generators present in thesuperconformal group (as opposed to just the super-Poincaregroup). The 't Hooft limit of 3 + 1 N = 4 super-Yang–Mills at the conformal pointis shown to contain strings: they are IIB strings. Weconjecture that compactifications of M/string theory on various anti-de Sitterspacetimes is dual to various conformal field theories.This leads to a new proposal for a definition ofM-theory which could be extended to include fivenoncompact dimensions.},
  file = {/home/ivan/Zotero/storage/V7LL8ZII/Maldacena - 1999 - The Large-N Limit of Superconformal Field Theories.pdf},
  langid = {english},
  number = {4}
}