cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
MUHAMMED RAHİMOKHAN II (FERUZ)'UN HORAZM'DA CEDİD HAREKETİNİN ORTAYA ÇIKIŞI SIRASINDAKİ EYLEMLERİ
Creators: name: Ismailov, Tokhirjon
Publisher: name: Zenodo
Year: 2024

description: Bu makale Muhammed Rahim Han II'ın Harezm'deki Cedidî hareketin oluşumundaki etkisini incelemektedir. 19. yüzyılın ikinci yarısında Hive Hanlığı'nın hükümdarı Muhammed Rahim Han II, yalnızca devlet yönetiminde değil, kültür ve eğitim reformlarında da aktif rol aldı. Onun bilime, edebiyata ve kültüre olan ilgisi toplumda modernist fikirlerin ortaya çıkıp yayılmasının temelini attı. Makalede Cedidci hareketin gelişiminin tarihsel koşulları ve Muhammed Rahim Han II'ın bu konudaki politikası analiz edilmektedir. Araştırma sırasında tarihi kaynaklardan ve bilimsel literatürden yararlanılmıştır.
title: Ð¡Ð¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ
title: The condition of medical rehabilitation in Saint-Petersburg
Creators: name: ÐÐ°ÐºÐ°ÑÐµÐ½ÐºÐ¾, Ð¡ÑÐ°Ð½Ð¸ÑÐ»Ð°Ð²
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2023
Subjects: ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ñ
Ð¸Ð½Ð²Ð°Ð»Ð¸Ð´Ð½Ð¾ÑÑÑ
Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ðµ Ð»ÐµÑÐµÐ½Ð¸Ðµ
Ð±Ð¾Ð»ÑÐ½Ð¸ÑÑ
rehabilitation
disability
rehabilitation treatment
hospitals

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸ Ð² Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ðµ, ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð·Ð´ÑÐ°Ð²Ð¾Ð¾ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ Ð²Ð¾ÑÑÑÐ°Ð½Ð¾Ð²Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð»ÐµÑÐµÐ½Ð¸Ñ. ÐÐ° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¡ÐÐ± ÐÐÐ£Ð Â«ÐÐ¾ÑÐ¾Ð´ÑÐºÐ°Ñ Ð±Ð¾Ð»ÑÐ½Ð¸ÑÐ° â 40Â» Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ð¹ Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¸, ÐµÐµ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ¾ÑÑÐ°Ð²Ð»ÑÑÑÐ¸Ðµ Ð¸ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ.
description: This article analyses the problems of the contemporary position of rehabilitation in St.-Petersburg as well as the existing programmes of healthcare development that focus on the questions of rehabilitation treatment. In the example of St.-Petersburg State Institution of Healthcare âCity Hospital â 40â the efficiency of the complex medical rehabilitation is shown and the main details and perspectives of its development are described.
Three-flavour neutrino oscillation update and comments on possible hints for a non-zero theta_{13}
Creators: name: Maltoni, Michele
name: Schwetz, Thomas
Publisher: name: arXiv
Year: 2008
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We provide a short summary of three-flavour neutrino oscillation parameters as determined from a global fit to 2008 data, and we comment on possible hints in favour of a non-zero value of the mixing angle theta_{13} found in arXiv:0806.2649. We do confirm a hint from solar + KamLAND data at about 1.5 sigma, which can be understood from the recent SNO CC/NC measurment. However, we show that a claimed hint from atmospheric data is much less robust. It depends on details of event rate calculations and treatment of theoretical uncertainties. We could identify two data points showing an 'excess' (at the 1 sigma level) in the SK-I multi-GeV e-like data, which seem to be the origin of the slight preference for theta_{13} > 0. We point out that once SK-I and SK-II data are combined this 'excess' disappears, and irrespective of the details of the analysis, no 'hint' from atmospheric data is obtained for the SK-I and SK-II combined data set. As a result the global fit of all data leads to a best fit value of theta_{13} consistent with zero within less than 1 sigma.
description: 8 pages, 3 figures, Talk by T. Schwetz at the idm2008 conference, Aug. 18-22, 2008, Stockholm, Sweden
Human rights and migrant deaths in settler-colonial Canada
Creators: name: Warbeck, Lauren
Publisher: name: University of British Columbia
Year: 2025

description: At least twenty migrants, many of them refugee claimants, have died while in the custody of the Canada Border Services Agency (CBSA) since 1995. Despite the rigorous regulation of migration and detention via international humanitarian law, research indicates that anti-migrant hostility and inhumane conditions of detention have contributed to these deaths (Razack, 2015; Pratt, 2005) and the Canadian state has neither assumed nor been assigned liability for these deaths. This study asks how laws that protect life can produce and legitimate migrant deaths by conducting a case study of the coronial inquest into the 2013 death of a Mexican woman and failed refugee claimant named Lucia Vega Jimenez in in CBSA custody. A critical discourse analysis of the inquest transcript revealed that humanitarian legal principles embedded in Canadian migration law played a causal role in Vega Jimenez’ death and functioned to legitimate it in the inquest that followed, implying that humanitarian law is imbued with violent potential. I posit that humanitarian law and the liberal legal principles that inform it are a mechanism of colonial violence that operate through racial logics. Through a geolegal and archival analysis of the formation of Canadian migration law, I trace the emergence of the legal discourses that most profoundly shaped Vega Jimenez’ death – sovereignty and humanity – from their colonial origins to the present. I argue that modern notions of both the ‘sovereign’ and the ‘human’ that arise in Canadian law, and that functioned to produce and legitimate Vega Jimenez’ death, are constitutive of and through settler-colonial violence. I conceptualize Canadian migration law and the colonial inquest as a mechanisms of biopower that function to reproduce settler-colonial sovereignty by integrating migrant deaths into the life of the white settler population.
title: ÐÐ¿ÑÐ¸Ð¼Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾ÑÐ¾ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ° Ð½Ð¸Ð·ÐºÐ¾Ð³Ð¾ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾Ð¹ ÑÐ¸Ñ Ð¾Ñ Ð¾Ð´Ð½Ð¾Ð¹ Ð¿Ð°ÑÐ¾Ð²Ð¾Ð¹ ÑÑÑÐ±Ð¸Ð½Ñ Ð´Ð»Ñ ÐÐ­Ð¡
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð»Ð¾Ð¿ÐºÐ¾Ð²Ð°, Ð£Ð»ÑÑÐ½Ð°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐÐ°ÑÐ¾Ð²ÑÐµ ÑÑÑÐ±Ð¸Ð½Ñ
Ð¼Ð½Ð¾Ð³Ð¾ÑÑÑÐ¿ÐµÐ½ÑÐ°ÑÐ°Ñ Ð¿Ð°ÑÐ¾Ð²Ð°Ñ ÐºÐ¾Ð½Ð´ÐµÐ½ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÐ±Ð¸Ð½Ð°
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description: Ð¦ÐµÐ»Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ:Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ðµ ÐÐÐ Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¦ÐÐ. Ð ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ñ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð¾ÑÐ½ÑÐµ Ð³Ð°Ð·Ð¾Ð´Ð¸Ð½Ð°Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¦ÐÐ, Ð¿ÑÐ¾ÑÐ¸Ð»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð»Ð¾Ð¿Ð°ÑÐºÐ¸ Ð¿Ð¾ÑÐ»ÐµÐ´Ð½ÐµÐ¹ ÑÑÑÐ¿ÐµÐ½Ð¸, Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÑÐ¸Ð»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµÐ¹ Ð»Ð¾Ð¿Ð°ÑÐºÐ¸ Ð¦ÐÐ.
Thermodynamic instability of rotating black holes
Creators: name: Monteiro, Ricardo
name: Perry, Malcolm J.
name: Santos, Jorge E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We show that the quasi-Euclidean sections of various rotating black holes in different dimensions possess at least one non-conformal negative mode when thermodynamic instabilities are expected. The boundary conditions of fixed induced metric correspond to the partition function of the grand-canonical ensemble. Indeed, in the asymptotically flat cases, we find that a negative mode persists even if the specific heat at constant angular momenta is positive, since the stability in this ensemble also requires the positivity of the isothermal momentum of inertia. We focus in particular on Kerr black holes, on Myers-Perry black holes in five and six dimensions, and on the Emparan-Reall black ring solution. We go on further to consider the richer case of the asymptotically AdS Kerr black hole in four dimensions, where thermodynamic stability is expected for a large enough cosmological constant. The results are consistent with previous findings in the non-rotation limit and support the use of quasi-Euclidean instantons to construct gravitational partition functions.
description: 36 pages, 11 figures; v2: corrections to match published version
title: Review and accountability mechanisms of selected international agreements to inform the development of the post-2020 global biodiversity framework
Creators: name: United Nations Environment Programme World Conservation Monitoring Centre
Publisher: name: United Nations Environment Programme World Conservation Monitoring Centre
Year: 2019

description: ​This briefing document presents an overview of a number of review and accountability mechanisms developed under a range of international agreements. By sharing lessons relating to their design and implementation, it seeks to help inform discussions on review and accountability mechanisms for the post-2020 global biodiversity framework. The following treaties are included: UN Framework Convention on Climate Change, UN human rights treaty system, the Aarhus Convention, the Ramsar Convention, and the World Heritage Convention.
title: ÐÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÑÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸ÑÐµÐ»ÑÐ²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð°Ñ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÑ
Ð¿ÑÐ¾Ð²ÐµÑÐºÐ° ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸
Ð²Ð½ÐµÑÐ½Ð¸Ð¹ Ð°ÑÐ´Ð¸Ñ

description: Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð Ð°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ñ ÑÐ¾ÑÐºÐ¸ Ð·ÑÐµÐ½Ð¸Ñ Ð²Ð½ÐµÑÐ½ÐµÐ³Ð¾ Ð°ÑÐ´Ð¸ÑÐ°. ÐÑÐ½Ð¾Ð²Ð½ÑÐ¼Ð¸ Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸ ÑÐ²Ð»ÑÑÑÑÑ: Ð¸Ð·ÑÑÐ¸ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸; ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÑÑ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð°ÑÐ¿ÐµÐºÑÑ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸; ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð¾Ð² Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸. ÐÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÑÑÑÐ¿Ð¸Ð»Ð¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð½Ð°ÑÑÐ½Ð¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÑ, ÐºÐ¾ÑÑÑÐ¸ÑÐ¸ÐµÐ½ÑÐ½ÑÐ¹ Ð¼ÐµÑÐ¾Ð´, Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÑÑÐ´ÐºÐ° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ°Ð±Ð¾ÑÐ¸Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸, ÑÐ»Ð¸ÑÐµÐ½Ð¸Ðµ Ð¿ÐµÑÐ²Ð¸ÑÐ½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð² Ð¸ Ñ.Ð´. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¾ÑÐ¼ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«Ð Ð°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ°Â» Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ°, Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð½ÑÐµ Ð¾Ð±ÑÐ¸Ð¼ Ð¿Ð»Ð°Ð½Ð¾Ð¼ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸, Ð° Ð¸Ð¼ÐµÐ½Ð½Ð¾: Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÑÐ° Ð¸ ÑÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°; ÑÐ¾ÑÐ¼Ñ Ð³Ð¾Ð´Ð¾Ð²Ð¾Ð¹ Ð¾ÑÑÐµÑÐ½Ð¾ÑÑÐ¸; Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ¸Ð·Ð°ÑÐ¸Ñ Ð¸Ð¼ÑÑÐµÑÑÐ²Ð° Ð¸ ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÑÑÐ²; Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÑÐµÐ´ÑÑÐ²Ð°; Ð´ÐµÐ±Ð¸ÑÐ¾ÑÑÐºÐ°Ñ Ð·Ð°Ð´Ð¾Ð»Ð¶ÐµÐ½Ð½Ð¾ÑÑÑ; Ð¾Ð±ÑÐ·Ð°ÑÐµÐ»ÑÑÑÐ²Ð°; ÑÐ¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ. Ð ÑÐ¾Ð´Ðµ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð²ÐµÑÐºÐ¸ Ð¿Ð¾ Ð¾ÑÐ´ÐµÐ»ÑÐ½ÑÐ¼ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÐ¼ Ð¾Ð¿ÐµÑÐ°ÑÐ¸ÑÐ¼ Ð±ÑÐ»Ð¸ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ñ Ð¾ÑÐ¸Ð±ÐºÐ¸ Ð¸ Ð½ÐµÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ Ð¸Ñ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð¸Ñ Ð² Ð±ÑÑÐ³Ð°Ð»ÑÐµÑÑÐºÐ¾Ð¼ ÑÑÐµÑÐµ. Ð ÑÐ°ÑÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐ¸Ð±ÐºÐ¸ Ð±ÑÐ»Ð¸ Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð² ÑÐµÐºÑÐ¸Ð¸ Â«Ð¤Ð¸Ð½Ð°Ð½ÑÐ¾Ð²ÑÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°Ñ. Ð Ð°ÑÑÐ¾Ð´ÑÂ».
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ "Ð¨ÐµÑÑÐµÑÐ½Ñ" Ñ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÐ¶ÑÑÐµÐ³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÐºÐ°ÑÐ¾Ð², ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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description: Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«Ð¨ÐµÑÑÐµÑÐ½ÑÂ»: Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ÑÑÐ¾Ð´Ð½ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ, Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¼ÐµÑÐ¾Ð´Ð° Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±Ð¾Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÐ½Ð°ÑÑÐºÐ¸, ÑÐµÐ¶ÑÑÐµÐ³Ð¾ Ð¸ Ð²ÑÐ¿Ð¾Ð¼Ð¾Ð³Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ°, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð½Ð¾ÑÐ¼Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð´Ð»Ñ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð¸ ÑÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ð¸. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ° Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÑÐ¸ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»Ð°: Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ°ÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¸Ð·Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐµÐ·ÑÐ°, Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¼ÐµÑÑÐ¸ÐºÐ¾Ð² Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÑÐ½Ð¾Ð²Ð¾Ð¹ ÑÐµÑÐ²ÑÑÐ½Ð¾Ð¹ ÑÑÐµÐ·Ñ Ð´Ð»Ñ Ð½Ð°ÑÐµÐ·Ð°Ð½Ð¸Ñ ÑÐ¸Ð»Ð¸Ð½Ð´ÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·ÑÐ±ÑÐ°ÑÑÑ ÐºÐ¾Ð»ÑÑ. Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾-ÑÐ°Ð·Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸Ð·Ð°ÑÐ¸Ð¸ ÑÐ¾ÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾ÑÐ¾ÑÐºÐ¸ Ð½Ð° Ð´ÐµÑÐ°Ð»Ð¸ ÑÐ¸Ð¿Ð° Â«ÐÑÑÐ»ÐºÐ°Â». ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ñ ÑÑÑÑÐºÑÑÑÐ½ÑÑ ÑÑÐµÐ¼ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ², ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÐµÐ¼Ð° Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¿Ð¾ÑÑÑÑÐ½Ð¾Ð¹ Ð²ÑÐ´Ð°ÑÐ¸ Ð¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° Ð´Ð¾ÑÑÐ»Ð°ÑÐµÐ»Ñ, Ð²ÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ ÑÐ±Ð¾ÑÐ° Ð³Ð¾ÑÐ¾Ð²ÑÑ Ð¸Ð·Ð´ÐµÐ»Ð¸Ð¹. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° ÑÐ¸ÐºÐ»Ð¾Ð³ÑÐ°Ð¼Ð¼Ð° ÑÐ°Ð±Ð¾ÑÑ Ð·Ð°Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾-ÑÐ°Ð·Ð³ÑÑÐ·Ð¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°.
title: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ Ð½ÐµÑÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð° Ð½Ð° ÑÐ¿ÑÑÐ³Ð¾Ð¼ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð®Ð³Ð¾Ð², ÐÐ²Ð°Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¢Ð²ÐµÑÐ´ÑÐµ ÑÐµÐ»Ð°
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¿ÑÑÐ³Ð¾Ðµ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ¸ Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð° Ð½Ð° ÑÐ¿ÑÑÐ³Ð¾Ð¼ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ â Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ðµ Ð´Ð¾Ð¿ÑÑÑÐ¸Ð¼Ð¾Ð³Ð¾ Ð´Ð¸ÑÐ±Ð°Ð»Ð°Ð½ÑÐ° Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð° Ð¿ÑÐ¸ Ð·Ð°Ð´Ð°Ð½Ð½ÑÑ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¸Ñ, ÑÐ¿ÑÑÐ³Ð¸Ñ Ð¸ Ð¸Ð½ÐµÑÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ñ. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð° Ð·Ð°Ð´Ð°ÑÐ° Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð½ÐµÑÑÐ°Ð²Ð½Ð¾Ð²ÐµÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ ÐºÐ¾Ð»ÐµÐ±Ð°Ð½Ð¸Ð¹ Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð° Ð½Ð° ÑÐ»ÐµÐ´ÑÑÑÐ¸Ñ ÑÐ¿ÑÑÐ³Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸ÑÑ: ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð°Ñ Ð¼Ð°ÑÐ¸Ð½Ð°, Ð¿ÐµÑÐµÐ´Ð²Ð¸Ð¶Ð½Ð°Ñ Ð²ÑÑÐºÐ°. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾Ð±Ð»Ð°ÑÑÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐ°Ð±Ð¸Ð»ÑÐ½Ð¾ÑÑÐ¸ Ð²ÑÐ°ÑÐ°ÑÑÐµÐ³Ð¾ÑÑ ÑÐ²ÑÑÐ´Ð¾Ð³Ð¾ ÑÐµÐ»Ð° Ð¿ÑÐ¸ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐµ Ð½Ð° ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ Ð½Ð° Ð¿ÐµÑÐµÐ´Ð²Ð¸Ð¶Ð½ÑÑ Ð²ÑÑÐºÑ.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð½Ð¸Ð·ÐºÐ¾ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¼Ð° Ð² Ð¡ÐÐ§-ÑÑÐ¸Ð»Ð¸ÑÐµÐ»ÑÑ Ð½Ð° GaAs-Ð¿Ð¾Ð»ÐµÐ²ÑÑ ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°Ñ Ð¸ GaN-Ð³ÐµÑÐµÑÐ¾ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: Ð§ÐµÑÐ½Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð£ÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸ ÑÐ²ÐµÑÑ Ð²ÑÑÐ¾ÐºÐ¸Ñ ÑÐ°ÑÑÐ¾Ñ
ÐÐ¾Ð»ÑÐ¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð²ÑÐµ Ð¿ÑÐ¸Ð±Ð¾ÑÑ

description: ÐÐ·ÑÑÐ°ÑÑÑÑ ÑÐ»ÑÐºÑÑÐ°ÑÐ¸Ð¸ ÑÐ°Ð·Ñ Ð¸ Ð°Ð¼Ð¿Ð»Ð¸ÑÑÐ´Ñ Ð² Ð¡ÐÐ§-ÑÑÐ¸Ð»Ð¸ÑÐµÐ»ÑÑ Ð½Ð° GaAs-Ð¿Ð¾Ð»ÐµÐ²ÑÑ ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°Ñ Ð¸ GaN-Ð³ÐµÑÐµÑÐ¾ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð½Ð¸Ð·ÐºÐ¾ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¼Ð°, Ð¿Ð¾ÑÐ¾Ð¶Ð´Ð°ÑÑÐ¸Ðµ ÑÑÐ¸ ÑÐ»ÑÐºÑÑÐ°ÑÐ¸Ð¸. ÐÐ±Ð½Ð°ÑÑÐ¶ÐµÐ½ Ð¸ Ð¾Ð±ÑÑÑÐ½ÐµÐ½ ÑÑÑÐµÐºÑ ÑÐ²ÐµÐ»Ð¸ÑÐµÐ½Ð¸Ñ ÑÐ°Ð·Ð¾Ð²ÑÑ ÑÑÐ¼Ð¾Ð² Ð½Ð° 10 Ð´Ð Ð² ÑÐµÐ¶Ð¸Ð¼Ðµ Ð½Ð°ÑÑÑÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ Ð½Ð¸Ð·ÐºÐ¾ÑÐ°ÑÑÐ¾ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ¼Ð° Ð² Ð³ÐµÑÐµÑÐ¾ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°Ñ Ñ Ð²ÑÑÐ¾ÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½Ð¾ÑÑÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð². Ð£ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ñ Ð´Ð²Ð° Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ° ÐÐ§-ÑÑÐ¼Ð°: ÑÐ»ÑÐºÑÑÐ°ÑÐ¸Ð¸ Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð² Ð² ÐºÐ°Ð½Ð°Ð»Ðµ Ð¸ ÑÐ»ÑÐºÑÑÐ°ÑÐ¸Ð¸ Ð·Ð°ÑÑÐ´Ð° Ð² Ð¿Ð¾Ð´Ð·Ð°ÑÐ²Ð¾ÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÐ¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÑÐ°Ð½Ð·Ð¸ÑÑÐ¾ÑÐ°, Ð² ÐºÐ¾ÑÐ¾ÑÑÑ ÑÐºÐ°Ð·Ð°Ð½Ð½ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¿ÑÐ¾ÑÐ²Ð»ÑÑÑÑÑ Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÑÑÐ¸Ð¼ Ð²ÐµÑÐ¾Ð¼. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÐÐ§-ÑÐ»ÑÐºÑÑÐ°ÑÐ¸Ð¹ Ð¿Ð¾Ð´Ð²Ð¸Ð¶Ð½Ð¾ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð², Ð¾Ð±ÑÑÑÐ½ÑÑÑÐ°Ñ ÑÐ»Ð¸ÐºÐºÐµÑÐ½ÑÐ¹ Ð²Ð¸Ð´ Ð¸Ñ ÑÐ¿ÐµÐºÑÑÐ¾Ð². Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð²ÑÐ²Ð¾Ð´Ñ Ð² Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¼ Ð¿Ð¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ñ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð¼.
4TU.ResearchData Community Call: Managing Health and Technology Research Data
Creators: name: Clare, Connie
name: Aarts, Anne
name: Nizamis, Kostas
Publisher: name: Zenodo
Year: 2021

description: About the Speakers:
 Connie Clare, Community Manager, 4TU.ResearchData
 Anne Aarts, Data Steward (Biomedical Engineering), TU/Eindhoven
 Kostas Nizamis, Assistant Professor of Multidisciplinary Design, University of Twente` About the community
 4TU.ResearchData is an international data repository for science, engineering and design disciplines. Built around the technical infrastructure, the online community comprises researchers, research data supporters (data stewards, data managers, research software engineers, IT and communications specialists) and technical experts (repository back office staff). The goal of the community is to provide an inclusive space for members to connect and exchange knowledge about best practices for the creation and reuse of FAIR data within diverse scientific domains. This includes the development and provision of discipline-specific guidance, training and resources to support researchers in making their data Findable, Accessible, Interoperable and Reusable (The FAIR Principles). Community call: Managing Health and Technology Research Data (Agenda)  11:00 - 11:05  Welcome and housekeeping Connie Clare (4TU) 11:05 - 11:15 Getting to know you! (Menti) Anne Aarts (TU/e) 11:15 - 11:25 LCRDM Medical device regulation Anne Aarts  11:25 - 11:35 Q&A: Medical devices (chat) Anne Aarts  11:35 - 11:45  Publishing medical data  Kostas Nizamis (UT) 11:45 - 11:55  Q&A: Medical data (chat) Kostas Nizamis  11:55 - 12:00 Reflections (Menti) & closing  Anne/Connie
Efficient Offline Algorithmic Techniques for Several Packet Routing Problems in Distributed Systems
Creators: name: Andreica, Mugurel Ionut
name: Tapus, Nicolae
Publisher: name: arXiv
Year: 2009
Subjects: subject: Data Structures and Algorithms (cs.DS)
subject: Distributed, Parallel, and Cluster Computing (cs.DC)
subject: Discrete Mathematics (cs.DM)
subject: FOS: Computer and information sciences
subject: F.2.2; G.2.1

description: In this paper we consider several problems concerning packet routing in distributed systems. Each problem is formulated using terms from Graph Theory and for each problem we present efficient, novel, algorithmic techniques for computing optimal solutions. We address topics like: bottleneck paths (trees), optimal paths with non-linear costs, optimal paths with multiple optimization objectives, maintaining aggregate connectivity information under a sequence of network link failures, and several others.
title: Ð¡Ð¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¸Ð´Ñ Ð»Ð¸ÑÑÑ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÑÐ»ÑÐµÐ²Ð°, Ð¢Ð°ÑÑÑÐ½Ð°
name: ÐÐ¼ÐµÐ»ÑÑÐ½Ð¾Ð², ÐÐ°Ð´Ð¸Ð¼
name: ÐÐ°ÑÑÑÐ½Ð¾Ð², ÐÐ¾Ð½ÑÑÐ°Ð½ÑÐ¸Ð½
name: ÐÑÐµÑÐºÐ¾, ÐÑÐºÐ°Ð´Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐÐÐ°Ñ
Year: 2007
Subjects: ÐÐ¸ÑÑÐµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¾ÑÐ²ÐµÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐµÐ¾ÑÐ¸Ð¸, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð²Ð¸Ð´Ð¾Ð² Ð»Ð¸ÑÑÑ: Ð¿Ð¾ Ð²ÑÐ¿Ð»Ð°Ð²Ð»ÑÐµÐ¼ÑÐ¼ Ð¼Ð¾Ð´ÐµÐ»ÑÐ¼, Ð² Ð¾Ð±Ð¾Ð»Ð¾ÑÐºÐ¾Ð²ÑÐµ ÑÐ¾ÑÐ¼Ñ, ÐºÐ¾ÐºÐ¸Ð»ÑÐ½Ð¾Ð³Ð¾ Ð»Ð¸ÑÑÑ, Ð¿Ð¾Ð´ Ð´Ð°Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼, ÑÐµÐ½ÑÑÐ¾Ð±ÐµÐ¶Ð½Ð¾Ð³Ð¾, Ð²Ð°ÐºÑÑÐ¼Ð½Ð¾Ð³Ð¾ Ð²ÑÐ°ÑÑÐ²Ð°Ð½Ð¸Ñ Ð¸ Ð½ÐµÐ¿ÑÐµÑÑÐ²Ð½ÑÑ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð² Ð»Ð¸ÑÑÑ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°Ñ, Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð¹ Ð¾ÑÐ½Ð°ÑÑÐºÐµ, ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð¾Ð±Ð»Ð°ÑÑÐ¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ ÑÐ¿Ð¾ÑÐ¾Ð±Ð¾Ð². ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ âÐÐ°ÑÐ¸Ð½Ñ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°â, Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑ âÐ¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð»Ð¸ÑÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°â.
Aperture-corrected spectroscopic type Ia supernova host galaxy properties
Creators: name: Galbany, Lluís
name: Smith, Mat
name: Puertas, Salvador Duarte
name: González-Gaitán, Santiago
name: Pessa, Ismael
name: Sako, Masao
name: Iglesias-Páramo, Jorge
name: López-Sánchez, A. R.
name: Mollá, Mercedes
name: Vílchez, José M.
Publisher: name: arXiv
Year: 2021
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: We use type Ia supernovae (SNe Ia) data obtained by the Sloan Digital Sky Survey-II Supernova Survey (SDSS-II/SNe) in combination with the publicly available SDSS DR16 fiber spectroscopy of their host galaxies to correlate SNe Ia light-curve parameters and Hubble residuals to several host galaxy properties. Fixed-aperture fiber spectroscopy suffers from aperture effects: the fraction of the galaxy covered by the fiber varies depending on its projected size on the sky, thus measured properties are not representative of the whole galaxy. The advent of Integral Field Spectroscopy has provided a way for correcting the missing light, by studying how these galaxy parameters change with the aperture size. Here we study how the standard SN host galaxy relations change once global host galaxy parameters are corrected for aperture effects. We recover previous trends on SN Hubble residuals with host galaxy properties, but we find that discarding objects with poor fiber coverage instead of correcting for aperture loss introduces biases in the sample that affect SN host galaxy relations. The net effect of applying the commonly used $g$-band fraction criterion is discarding intrinsically faint \mbox{SNe~Ia} in high-mass galaxies, thus artificially increasing the height of the mass step by 0.02 mag and its significance. Current and next generation of fixed-aperture fiber spectroscopy surveys, such as DES, DESI or TiDES in 4MOST, that aim at study SN and galaxy correlations must consider, and correct for, these effects.
description: Accepted in A&A. 16 pages, 12 Figures
Spontaneous supersymmetry breaking in large-$N$ matrix models with slowly varying potential
Creators: name: Kuroki, Tsunehide
name: Sugino, Fumihiko
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We construct a class of matrix models, where supersymmetry (SUSY) is spontaneously broken at the matrix size $N$ infinite. The models are obtained by dimensional reduction of matrix-valued SUSY quantum mechanics. The potential of the models is slowly varying, and the large-$N$ limit is taken with the slowly varying limit. First, we explain our formalism, introducing an external field to detect spontaneous SUSY breaking, analogously to ordinary (bosonic) symmetry breaking. It is observed that SUSY is possibly broken even in systems in less than one-dimension, for example, discretized quantum mechanics with a finite number of discretized time steps. Then, we consider spontaneous SUSY breaking in the SUSY matrix models with slowly varying potential, where the external field is turned off after the large-$N$ and slowly varying limit, analogously to the thermodynamic limit in statistical systems. On the other hand, without taking the slowly varying limit, in the SUSY matrix model with a double-well potential whose SUSY is broken due to instantons for finite $N$, a number of supersymmetric behavior is explicitly seen at large $N$. It convinces us that the instanton effect disappears and the SUSY gets restored in the large-$N$ limit.
description: 46 pages, LaTeX
The challenges of non-identifiability and a penalized maximum likelihood estimator for the beta mixture model
Creators: name: Tang, Tom
Publisher: name: University of British Columbia
Year: 2025

description: This thesis explores statistical inference for the finite mixture models, with a particular focus on beta mixture models, which are widely used in biostatistics, bioinformatics, and computer science. It addresses significant issues such as unbounded likelihood and non-identifiability, which can complicate parameter estimation. To overcome the obstacle caused by the unbounded likelihood, we propose a penalized maximum likelihood estimation approach by adding a penalty term to the log-likelihood function, leading to stable parameter estimation. Additionally, we derive a closed-form expression for testing non-identifiability in beta mixture models. The effectiveness of our penalized approach is evaluated through simulation studies and compared with alternative approaches, such as the method of moments. Practical applicability is demonstrated through applications to DNA methylation analysis and local false discovery rate estimation. Finally, we suggest several directions for future research.
The Deep SWIRE Field. IV. First properties of the sub-mJy galaxy population: redshift distribution, AGN activity and star formation
Creators: name: Strazzullo, Veronica
name: Pannella, Maurilio
name: Owen, Frazer N.
name: Bender, Ralf
name: Morrison, Glenn E.
name: Wang, Wei-Hao
name: Shupe, David L.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present a study of a 20cm selected sample in the Deep SWIRE VLA Field, reaching a limiting flux density of ~13.5 uJy at the image center. In a 0.6x0.6 square degrees field, we are able to assign an optical/IR counterpart to 97% of the radio sources. Up to 11 passbands from the NUV to 4.5um are then used to sample the spectral energy distribution (SED) of these counterparts in order to investigate the nature of the host galaxies. By means of an SED template library and stellar population synthesis models we estimate photometric redshifts, stellar masses, and stellar population properties, dividing the sample in three sub-classes of quiescent, intermediate and star-forming galaxies. We focus on the radio sample in the redshift range 0.3
description: 18 pages, 16 figures, accepted for publication in ApJ
Cosmology in scalar-tensor $f(R,T)$ gravity
Creators: name: Gonçalves, Tiago B.
name: Rosa, João Luís
name: Lobo, Francisco S. N.
Publisher: name: arXiv
Year: 2021
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In this work, we use reconstruction methods to obtain cosmological solutions in the recently developed scalar-tensor representation of $f(R,T)$ gravity. Assuming that matter is described by an isotropic perfect fluid and the spacetime is homogeneous and isotropic, i.e., the Friedmann-Lemaître-Robsertson-Walker (FLRW) universe, the energy density, the pressure, and the scalar field associated with the arbitrary dependency of the action in $T$ can be written generally as functions of the scale factor. We then select three particular forms of the scale factor: an exponential expansion with ${a(t)\propto e^t}$ (motivated by the de Sitter solution); and two types of power-law expansion with ${a(t)\propto t^{1/2}}$ and ${a(t)\propto t^{2/3}}$ (motivated by the behaviors of radiation- and matter-dominated universes in general relativity, respectively). A complete analysis for different curvature parameters ${k=\{-1,0,1\}}$ and equation of state parameters ${w=\{-1,0,1/3\}}$ is provided. Finally, the explicit forms of the functions $f\left(R,T\right)$ associated with the scalar-field potentials of the representation used are deduced.
description: 14 pages, 18 figures
title: ÐÑÐ¸ÐºÐ»Ð°Ð´Ð½ÑÐµ ÑÐ°ÑÑÑÑÑ Ð½Ð°Ð´ÑÐ¶Ð½Ð¾ÑÑÐ¸ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐµÐ½Ð¸ÑÐ¾Ð², ÐÐ°ÐºÑÐ¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐÑÑÐ¸ÑÐ»Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»ÑÐ½ÑÐµ

description: Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¾ ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ðµ Ð¿Ð°ÐºÐµÑÐ° ÑÑÐ½ÐºÑÐ¸Ð¹ Ð½Ð° ÑÐ·ÑÐºÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ MATLAB, Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÐ¼Ð¾Ð³Ð¾ Ð´Ð»Ñ Ð¾ÑÐµÐ½ÐºÐ¸ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ ÑÑÐµÐ¼ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÐµÐ¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÑÐµÐ¼Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÐ°ÑÑÐµÑÐ° Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»ÐµÐ¹ Ð½Ð°Ð´ÐµÐ¶Ð½Ð¾ÑÑÐ¸ ÑÐ¸ÑÑÐµÐ¼Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´ÑÑÐ¸Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð° Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°ÑÐ¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ. Ð¡Ð¾Ð·Ð´Ð°Ð½ Ð¸ Ð¸ÑÐ¿ÑÑÐ°Ð½ ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÐ¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ ÑÐµÑÐµÐ½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾ÑÑÐ°Ð½Ñ ÑÑÑÐ´Ð°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð¸ ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¸ ÑÑÐµÑÐ±Ð° Ð¾Ñ Ð¾ÑÐºÐ°Ð·Ð¾Ð². ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½ Ð¿ÑÐ¸Ð¼ÐµÑ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²ÑÐ±Ð¾ÑÐ° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ° ÑÑÐµÐ¼Ñ ÑÑÐ°ÑÑÐºÐ° ÑÐµÑÐ¸
Cross-Section Fluctuations in Chaotic Scattering
Creators: name: Dietz, B.
name: Harney, H. L.
name: Richter, A.
name: Schaefer, F.
name: Weidenmueller, H. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Chaotic Dynamics (nlin.CD)
subject: FOS: Physical sciences

description: For the theoretical prediction of cross-section fluctuations in chaotic scattering, the cross-section autocorrelation function is needed. That function is not known analytically. Using experimental data and numerical simulations, we show that an analytical approximation to the cross-section autocorrelation function can be obtained with the help of expressions first derived by Davis and Boose. Given the values of the average S-matrix elements and the mean level density of the scattering system, one can then reliably predict cross-section fluctuations.
Additional file 1 of Desferrioxamine alleviates UHMWPE particle-induced osteoclastic osteolysis by inhibiting caspase-1-dependent pyroptosis in osteocytes
Creators: name: Zhao, Shenli
name: Ge, Chen
name: Li, Yao
name: Chang, Leilei
name: Dan, Zhou
name: Tu, Yihui
name: Deng, Lianfu
name: Kang, Hui
name: Li, Changwei
Publisher: name: figshare
Year: 2023
Subjects: subject: Biophysics
subject: Space Science
subject: Physical Sciences not elsewhere classified
subject: Microbiology
subject: FOS: Biological sciences
subject: Cell Biology
subject: Molecular Biology
subject: Physiology
subject: Biotechnology
subject: Geology
subject: FOS: Earth and related environmental sciences
subject: Environmental Sciences not elsewhere classified
subject: Ecology
subject: Science Policy
subject: Immunology
subject: FOS: Clinical medicine
subject: Marine Biology
subject: Cancer
subject: Hematology

description: Additional file 1: Fig.S1. Rankl and Opg expression induced by UHMWPE particles. (A&B) The relative mRNA expression of RANKL and OPG in calvarial bone induced by UHMWPE implantation (n=3). (C&D) The relative mRNA expression of RANKL and OPG in MLO-Y4 cells induced by 50 μg/ml UHMWPE particles for 24 hours. *P<0.05, ***P<0.001. P-values were analyzed by two-tailed t tests.
Flat and almost flat bands in the quasi-one-dimensional Josephson junction array
Creators: name: Bukatova, Daryna
name: Zolotaryuk, Yaroslav
Publisher: name: arXiv
Year: 2021
Subjects: subject: Pattern Formation and Solitons (nlin.PS)
subject: FOS: Physical sciences

description: The dispersion law for the linear waves in the quasi-one-dimensional array of inductively coupled Josephson junctions (JJ) is derived. The array has a multiladder structure that consists of the finite number of rows ($N\ge 2$) in $Y$ direction and is infinite in $X$ direction. The spectrum of the linear waves (Josephson plasmons) consists of $2N-1$ branches. Among these branches there is a $N$-fold completely flat degenerate one that coincides with the Josephson plasma frequency. The remaining $N-1$ branches have a standard Josephson plasmon dispersion law typical for 1D JJ arrays. Application of the uniform dc bias on the top of each vertical column of junctions lifts the degeneracy and only one flat branch remains unchanged. The rest of the previously flat branches become weakly dispersive. The parameter range where the flatness of these branches is maximal has been discussed.
description: 14 pages, 6 figures
Significant Limb-Brightening in the Inner Parsec of Markarian 501
Creators: name: Piner, B. Glenn
name: Pant, Niraj
name: Edwards, Philip G.
name: Wiik, Kaj
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present three 43 GHz images and a single 86 GHz image of Markarian 501 from VLBA observations in 2005. The 86 GHz image shows a partially resolved core with a flux density of about 200 mJy and a size of about 300 Schwarzschild radii, similar to recent results by Giroletti et al. Extreme limb-brightening is found in the inner parsec of the jet in the 43 GHz images, providing strong observational support for a `spine-layer' structure at this distance from the core. The jet is well resolved transverse to its axis, allowing Gaussian model components to be fit to each limb of the jet. The spine-layer brightness ratio and relative sizes, the jet opening angle, and a tentative detection of superluminal motion in the layer are all discussed.
description: Astrophysical Journal Letters, accepted for January 1, 2009 issue
Orbital quantum magnetism in spin dynamics of strongly interacting magnetic lanthanide atoms
Creators: name: (:Unkn) Unknown
Publisher: name: My University
Year: 2018
Subjects: physics.atom-ph
quant-ph

description: © 2018 American Physical Society. Laser-cooled lanthanide atoms are ideal candidates with which to study strong and unconventional quantum magnetism with exotic phases. Here, we use state-of-the-art closed-coupling simulations to model quantum magnetism for pairs of ultracold spin-6 erbium lanthanide atoms placed in a deep optical lattice. In contrast to the widely used single-channel Hubbard model description of atoms and molecules in an optical lattice, we focus on the single-site multichannel spin evolution due to spin-dependent contact, anisotropic van der Waals, and dipolar forces. This has allowed us to identify the leading mechanism, orbital anisotropy, that governs molecular spin dynamics among erbium atoms. The large magnetic moment and combined orbital angular momentum of the 4f-shell electrons are responsible for these strong anisotropic interactions and unconventional quantum magnetism. Multichannel simulations of magnetic Cr atoms under similar trapping conditions show that their spin evolution is controlled by spin-dependent contact interactions that are distinct in nature from the orbital anisotropy in Er. The role of an external magnetic field and the aspect ratio of the lattice site on spin dynamics is also investigated.
A New Local Distance-Based Outlier Detection Approach for Scattered Real-World Data
Creators: name: Zhang, Ke
name: Hutter, Marcus
name: Jin, Huidong
Publisher: name: arXiv
Year: 2009
Subjects: subject: Machine Learning (cs.LG)
subject: Information Retrieval (cs.IR)
subject: FOS: Computer and information sciences

description: Detecting outliers which are grossly different from or inconsistent with the remaining dataset is a major challenge in real-world KDD applications. Existing outlier detection methods are ineffective on scattered real-world datasets due to implicit data patterns and parameter setting issues. We define a novel "Local Distance-based Outlier Factor" (LDOF) to measure the {outlier-ness} of objects in scattered datasets which addresses these issues. LDOF uses the relative location of an object to its neighbours to determine the degree to which the object deviates from its neighbourhood. Properties of LDOF are theoretically analysed including LDOF's lower bound and its false-detection probability, as well as parameter settings. In order to facilitate parameter settings in real-world applications, we employ a top-n technique in our outlier detection approach, where only the objects with the highest LDOF values are regarded as outliers. Compared to conventional approaches (such as top-n KNN and top-n LOF), our method top-n LDOF is more effective at detecting outliers in scattered data. It is also easier to set parameters, since its performance is relatively stable over a large range of parameter values, as illustrated by experimental results on both real-world and synthetic datasets.
description: 15 LaTeX pages, 7 figures, 2 tables, 1 algorithm, 2 theorems
The nature of compact groups of galaxies from cosmological simulations
Creators: name: Mamon, G. A.
name: Diaz-Gimenez, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: The nature of compact groups (CGs) of galaxies, apparently so dense that the galaxies often overlap, is still a subject of debate: Are CGs roughly as dense in 3D as they appear in projection? Or are they caused by chance alignments of galaxies along the line-of-sight, within larger virialized groups or even longer filamentary structures? The nature of CGs is re-appraised using the z=0 outputs of three galaxy formation models, applied to the dissipationless Millennium Simulation. The same selection criteria are applied to mock galaxy catalogs from these models as have been applied by Hickson and co-workers in redshift space. We find 20 times as many mock CGs as the `HCGs' found by Hickson within a distance corresponding to 9000 km/s. This very low (5%) HCG completeness is caused by Hickson missing groups that were either faint, near the surface brightness threshold, of small angular size, or with a dominant brightest galaxy. We find that most velocity-filtered CGs are physically dense, regardless of the precise threshold used in 3D group size and line-of-sight elongation, and of the galaxy formation model used. This result also holds for mock CGs with the same selection biases as was found for the HCGs.
description: 4 pages, talk given at "Galaxies in Isolation: Exploring Nature vs. Nurture" meeting held in Granada, Spain 12-15 May 2009, ASP. Final version. HCG completness is now 5% at v<9000 km/s
Two-orbital model for possible superconductivity pairing mechanism in nickelates
Creators: name: Lu, Chen
name: Hu, Lun-Hui
name: Wang, Yu
name: Yang, Fan
name: Wu, Congjun
Publisher: name: arXiv
Year: 2021
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: The newly synthesized strontium doped RNiO$_2$ (R=Nd, La) superconductors have stimulated extensive interests in understanding their pairing mechanism and pairing nature. Here we study the pairing mechanism in this family from a two-orbital model comprising the Ni- $3d_{x^2-y^2}$- and $3d_{xy}$- orbitals, equipped with extended Hubbard interactions and induced low-energy effective superexchange interactions. We then study the pairing symmetry in this system by using large scale variational Monte Carlo approach. Our results yield the intraorbital $d_{x^2-y^2}$-wave singlet pairing as the leading pairing symmetry in the nickelates, which is analogous to the cuprates. However, there exist two important differences between the physical properties of the two families due to the fact that at the low Sr-doping regime, while the Ni-$3d_{x^2-y^2}$ orbitals remain half-filled and singly-occupied to form a Mott-insulating background, the Ni-$3d_{xy}$ orbitals accommodate nearly all the extra doped holes, which move freely on this background. The first difference lies in the single-particle aspect: while the $3d_{x^2-y^2}$ degree of freedom remains Mott insulating with spectra weight pinned down at zero at low dopings, the $3d_{xy}$ one behaves as Fermi liquid with spectra weight near 1. The second difference lies in the pairing aspect: while the huge intra-$3d_{x^2-y^2}$-orbital pairing gap is actually a pseudo gap which has nothing to do with the SC, the small intra-$3d_{xy}$-orbital pairing gap serves as the true superconducting pairing gap, which is related to the $T_c$ via the BCS relation. Both differences can be verified by the angle-resolved photo-emission spectrum.
description: 12 pages, 3 figures, 2 appendixes
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ»ÑÑÐ°, ÑÐ¾Ð¿ÑÑÐ¶ÑÐ½Ð½Ð¾Ð³Ð¾ Ñ ÑÐ¸ÑÑÐµÐ¼Ð¾Ð¹ Ð²ÐµÑÑ Ð½ÐµÐ³Ð¾ ÑÑÐ¾Ð²Ð½Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÑÑÐµÐ½ÐºÐ¾, ÐÐ½ÑÐ¾Ð½
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ»ÑÑ
ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ
ÑÐ°ÑÑÑÑ Ð¸ Ð²ÑÐ±Ð¾Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð²
Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð» Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ MODBUS

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ»ÑÑÐ° Ð´Ð»Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÑÐ½ Ð¾Ð±Ð·Ð¾Ñ ÑÑÑÑÐºÑÑÑÑ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»Ñ Ð¸ ÐµÐ³Ð¾ ÑÑÐ½ÐºÑÐ¸Ð¸. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½ Ð¿ÑÐ»ÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð¾ Ð¼Ð¾Ð´ÐµÑÐ½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ðº ÑÐ°Ð·ÑÐ°Ð±Ð°ÑÑÐ²Ð°ÐµÐ¼Ð¾Ð¼Ñ ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÑÐ½ ÑÐ°ÑÑÑÑ Ð¸ Ð²ÑÐ±Ð¾Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÐ¾Ð², ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ð¸Ð°Ð»ÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¸Ð½ÑÐµÑÑÐµÐ¹Ñ RS-485 Ð¸ Ð¿ÑÐ¾ÑÐ¾ÐºÐ¾Ð» Ð¿ÐµÑÐµÐ´Ð°ÑÐ¸ MODBUS. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ ÑÐºÑÑÐ¿Ð½ÑÐ½Ð½ÑÐ¹ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ°Ð±Ð¾ÑÑ Ð¼Ð¸ÐºÑÐ¾ÐºÐ¾Ð½ÑÑÐ¾Ð»Ð»ÐµÑÐ° Ð¿ÑÐ»ÑÑÐ°. ÐÑÐ¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐµ, Ð² Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ð¼, Ð±ÑÐ»Ð¸ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ Ð¾ÑÐµÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð² ÑÐµÐ»ÑÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸Ð¼Ð¿Ð¾ÑÑÐ¾Ð½ÐµÐ·Ð°Ð²Ð¸ÑÐ¸Ð¼Ð¾ÑÑÐ¸.
Topological quantum phase transition in the BEC-BCS crossover phenomena
Creators: name: Arikawa, Mitsuhiro
name: Maruyama, Isao
name: Hatsugai, Yasuhiro
Publisher: name: arXiv
Year: 2010
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: A crossover between the Bose Einstein condensation (BEC) and BCS superconducting state is described topologically in the chiral symmetric fermion system with attractive interaction. Using a local Z_2 Berry phase, we found a quantum phase transition between the BEC and BCS phases without accompanying the bulk gap closing.
description: 4 pages, 5 figures
Rem2 stabilizes intrinsic excitability and spontaneous firing in visual circuits
Creators: name: (:Unkn) Unknown
Publisher: name: My University
Year: 2018
Subjects: Rem2
activity-dependent
homeostasis
intrinsic excitability
mouse
neuroscience
plasticity
Action Potentials
Animals
Female
Gene Expression Regulation
Male
Mice
Mice, Knockout
Monomeric GTP-Binding Proteins
Nerve Net
Neuronal Plasticity
Primary Cell Culture
Pyramidal Cells
Rats
Sensory Receptor Cells
Synapses
Visual Cortex

description: © Moore et al. Sensory experience plays an important role in shaping neural circuitry by affecting the synaptic connectivity and intrinsic properties of individual neurons. Identifying the molecular players responsible for converting external stimuli into altered neuronal output remains a crucial step in understanding experience-dependent plasticity and circuit function. Here, we investigate the role of the activity-regulated, non-canonical Ras-like GTPase Rem2 in visual circuit plasticity. We demonstrate that Rem2 -/- mice fail to exhibit normal ocular dominance plasticity during the critical period. At the cellular level, our data establish a cell-autonomous role for Rem2 in regulating intrinsic excitability of layer 2/3 pyramidal neurons, prior to changes in synaptic function. Consistent with these findings, both in vitro and in vivo recordings reveal increased spontaneous firing rates in the absence of Rem2. Taken together, our data demonstrate that Rem2 is a key molecule that regulates neuronal excitability and circuit function in the context of changing sensory experience.