cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°Ð²Ð»Ð¾Ð²Ð°, Ð¡Ð²ÐµÑÐ»Ð°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: 2016
Subjects: Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÐµ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ðµ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ

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: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. ÐÐ»Ñ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ»Ð¸ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð±ÑÐ»Ð¾ ÑÐµÑÐ¸ÑÑ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸: Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°ÑÑ ÑÐ¾Ð»Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð° Ð¸ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð² ÑÑÐµÑÐµ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸; Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐ°ÐºÑÐ¾ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¹ ÑÑÐµÐ´Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ; Ð¸Ð·ÑÑÐ¸ÑÑ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÐ¹ Ð¾Ð¿ÑÑ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ; Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°ÑÑ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ; Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ ÑÐ°ÐºÑÐ¾ÑÑ ÑÑÐµÐ´Ñ, Ð¾Ð±ÑÑÐ»Ð°Ð²Ð»Ð¸Ð²Ð°ÑÑÐ¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð½Ð¾ÑÑÑ Ð² ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð¼ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸; Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ ÐÐÐ Â«ÐÐ°Ð´ÐµÐ¶Ð´Ð°Â»; Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°ÑÑ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐÐ Â«ÐÐ°Ð´ÐµÐ¶Ð´Ð°Â»; Ð¾Ð¿ÑÐµÐ´ÐµÐ»Ð¸ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ; ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°ÑÑ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÐÐÐ Â«ÐÐ°Ð´ÐµÐ¶Ð´Ð°Â». Ð¦ÐµÐ»Ñ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ ÐºÐ°Ðº Ð²Ð½ÑÑÑÐ¸ÑÐ¸ÑÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð¼Ð¾ÑÐ¸Ð²Ð°ÑÐ¸Ð¸ ÑÑÑÐ´Ð° ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð² ÑÐ¾Ð¼, ÑÑÐ¾Ð±Ñ Ð¿Ð¾Ð±ÑÐ´Ð¸ÑÑ ÑÐ°Ð±Ð¾ÑÐ½Ð¸ÐºÐ° ÑÐ°Ð±Ð¾ÑÐ°ÑÑ Ð±Ð¾Ð»ÐµÐµ Ð¸Ð½Ð¸ÑÐ¸Ð°ÑÐ¸Ð²Ð½Ð¾, ÑÐ²Ð¾ÑÑÐµÑÐºÐ¸ Ð¸ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¸Ð²Ð½Ð¾ - Ñ Ð¼Ð°ÐºÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¾ÑÐ´Ð°ÑÐµÐ¹ Ð´Ð»Ñ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ.
Weinberg operator contribution to the CP-odd nuclear force in the quark model
Creators: name: Yamanaka, Nodoka
name: Oka, Makoto
Publisher: name: arXiv
Year: 2022
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Experiment (hep-ex)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: The contribution of the CP violating three-gluon interaction, proposed by Weinberg, to the short-range CP-odd nuclear force is evaluated in the nonrelativistic quark model. We first show that the naive leading contribution generated by the quark exchange process vanishes at sufficiently short distance within the resonating group method, by considering the one-loop level gluon exchange CP-odd interquark potential induced by the Weinberg operator with massive quarks and gluons. We then estimate the true leading contribution by evaluating the gluonic correction to the CP-odd interquark potential in the closure approximation. It is found that the resulting irreducible CP-odd nuclear force is comparable to that generated by the chiral rotation of the CP-even short-range nuclear force, where the CP-odd mass calculated with QCD sum rules is used as input. The explicit calculation of the electric dipole moment (EDM) of the $^3$He nucleus yields $d_{^3{\rm He}}^{\rm (irr)} (w) = - 1.5 \, w\, e $ MeV. The total $^3$He EDM, accounting for the intrinsic nucleon EDM, the pion-exchange and the short-range CP-odd nuclear force, is $d_{^3{\rm He}}^{\rm (tot)} (w) = 20_{-11}^{+14} \, w\, e $ MeV, with the dominant effect coming from the intrinsic nucleon EDM.
description: 17 pages, 8 figures
Il regolare respiro di Cygnus X-3
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2009

C’è del metodo, dietro all’apparente follia di Cygnus X-3, il buco nero più «pazzo» della galassia. Per decenni ha sconcertato gli astrofisici, con il suo comportamento bizzarro e apparentemente imprevedibile. Ora non più. Un articolo pubblicato oggi su Nature da un team internazionale di astrofisici, guidati da Marco Tavani dell’INAF, analizza le emissioni di Cygnus X-3 in varie bande e vi individua un pattern che si ripete: una sequenza regolare, per quanto in larga parte ancora non spiegata.
3D comparative evaluation and correlation of condylar morphology in bruxers and non-bruxers
Creators: name: Aakanksha Tiwari1, Suwarna Dangore Khasbage2
Publisher: name: Zenodo
Year: 2023
Subjects: Temporomandibular joint, TMJ, Bruxers, CBCT, Condyle, Condylar morphology

description: Parafunctional habits like bruxism may have a deleterious effect on the temporomandibular joint. It can lead to the alteration of condylar morphology which can further lead to temporomandibular joint disorders. The early 3-Dimensional evaluation may help detect morphological changes in the condyle and reduce the risk of developing temporomandibular disorders[DJ1] . It will also help to make patients aware of the condition and encourage prompt treatment of parafunctional habits. To do a 3-Dimensional comparative evaluation and correlation of condylar morphology in bruxers and non-bruxers. 90 patients with parafunctional habits will be evaluated on Cone Beam Computed Tomography [DJ2] [A3] in two groups (control group, study group) of 45 each, for alteration in condylar morphology based on the suggested classification. Results will be formulated based on the classification of condylar morphology. Evaluation of condylar morphology will be done on Cone Beam Computed Tomography based on the amount of variation in condylar morphology in bruxers as compared to non-bruxers. Thorough clinical examination and early evaluation of condylar morphology on Cone Beam Computed Tomography will help early detection of changes in the morphology of condyle and prompt treatment to reduce the risk of development of temporomandibular disorders.
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ½Ð°ÑÐ¾Ð²Ð°, ÐÐµÑÐ¾Ð½Ð¸ÐºÐ°
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: ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÐÐÐ Â«ÐÐµÑÑÐ°Â». ÐÑÐµÐ´Ð¼ÐµÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ â ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ ÐÐÐ Â«ÐÐµÑÑÐ°Â».
 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°Ð½Ð°Ð»Ð¸Ð· ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð¾Ð¼ ÐÐÐ Â«ÐÐµÑÑÐ°Â» Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹ Ð¿Ð¾ ÐµÑ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ.
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 Ð¢Ð°ÐºÐ¶Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¸ Ð¿ÐµÑÑÐ¸Ð¼Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾Ð³Ð½Ð¾Ð·Ñ, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ð° ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ð¹.
Restricting UHECRs and cosmogenic neutrinos with Fermi-LAT
Creators: name: Berezinsky, V.
name: Gazizov, A.
name: Kachelriess, M.
name: Ostapchenko, S.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: FOS: Physical sciences

description: Ultrahigh energy cosmic ray (UHECR) protons interacting with the cosmic microwave background (CMB) produce UHE electrons and gamma-rays that in turn initiate electromagnetic cascades on CMB and infrared photons. As a result, a background of diffuse isotropic gamma radiation is accumulated in the energy range $E\lsim 100$ GeV. The Fermi-LAT collaboration has recently reported a measurement of the extragalactic diffuse background finding it less intense and softer than previously measured by EGRET. We show that this new result constrains UHECR models and the flux of cosmogenic neutrinos. In particular, it excludes models with cosmogenic neutrino fluxes detectable by existing neutrino experiments, while next-generation detectors as e.g. JEM-EUSO can observe neutrinos only for extreme parameters.
description: 7 pages, 6 eps figures; v2: minor changes, v3: final version, added discussion of EGMF influence
L’astronauta Edward Michael a Merate
Creators: admin
Publisher: name: Media Inaf
Year: 2009

Evento organizzato dall’Osservatorio Astronomico di Brera, con il patrocinio dell’Assessorato alla Cultura del Comune di Merate, in collaborazione con l’Ensemble “Archinti”, in occasione della chiusura dell’Anno Interanzionale dell’Astronomia proclamato per il 2009 dall’Unesco. Programma: benvenuto del Sindaco di Merate Andrea Ambrogio Robbiani e del Direttore dell’Osservatorio Astronomico Dr. Giovanni Pareschi; resoconto attività dell’Osservatorio per l’Anno Internazionale dell’Astronomia; esibizione… Leggi tutto »
MЕHNATNING INSON VA JAMIYATNING RIVOJLANISHIDAGI O`RNI
Creators: name: Shokirov, Humoyiddin
Publisher: name: Zenodo
Year: 2023

description: Hozirgi kunda mеhnat o`zining tarkibiy rivoji jarayonida jiddiy ravishda murakkablashdi: inson tobora murakkabroq va xilma-xil opеratsiyalarni bajara boshladi, tobora uyushgan mеhnat vositalarini ishlatib, o`z oldiga ancha yuksakroq maqsadlar qo`yish va ularga erishishga intildi. Buning o‘ziga xos sabablari mavjud bolib, ularni maqolada ko’rishingiz mumkin.
A protocol of a rapid systematic review of workplace equity and inclusion initiatives for sexual and gender minority populations.
Creators: name: Williams, Lisa A.
name: Harvey-Smith, Lisa
name: Ratcliffe, Sarah
name: Bergman, Jessica
Publisher: name: OSF Registries
Year: 2024
Subjects: subject: Work, Economy and Organizations
subject: Public Affairs, Public Policy and Public Administration
subject: Gender and Sexuality
subject: Social and Behavioral Sciences
subject: Inequality and Stratification
subject: Sociology
subject: FOS: Sociology
subject: protocol
subject: rapid review
subject: workplace equity and inclusion

description: This is the registration of a protocol for a rapid systematic review of workplace equity and inclusion initiatives for sexual and gender minority populations.
Accelerating cosmology in Rastall's theory
Creators: name: Capone, Monica
name: Cardone, Vincenzo Fabrizio
name: Ruggiero, Matteo Luca
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: In an attempt to look for a viable mechanism leading to a present-day accelerated expansion, we investigate the possibility that the observed cosmic speed up may be recovered in the framework of the Rastall's theory, relying on the non-conservativity of the stress-energy tensor, i.e. $T^μ_{ν; μ} \neq 0$. We derive the modified Friedmann equations and show that they correspond to Cardassian-like equations. We also show that, under suitable assumptions on the equation of state of the matter term sourcing the gravitational field, it is indeed possible to get an accelerated expansion, in agreement with the Hubble diagram of both Type Ia Supernovae (SNeIa) and Gamma Ray Bursts (GRBs). Unfortunately, to achieve such a result one has to postulate a matter density parameter much larger than the typical $Ω_M \simeq 0.3$ value inferred from cluster gas mass fraction data.
description: 8 pages, 1 eps figure; revised to match the version accepted for publication in Il Nuovo Cimento B
Le immagini di VIRTIS della Terra raccolte durante l’ultimo fly-by di Rosetta
Creators: admin
Publisher: name: Media Inaf
Year: 2009

Il 13 Novembre 2009, la missione Rosetta dell’ESA ha effettuato l’ultimo fly-by della Terra permettendo a VIRTIS di raccogliere interessanti immagini e dati del nostro pianeta.
Cosmic-ray driven dynamo in the interstellar medium of irregular galaxies
Creators: name: Siejkowski, H.
name: Soida, M.
name: Otmianowska-Mazur, K.
name: Hanasz, M.
name: Bomans, D. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Irregular galaxies are usually smaller and less massive than their spiral, S0, and elliptical counterparts. Radio observations indicate that a magnetic field is present in irregular galaxies whose value is similar to that in spiral galaxies. However, the conditions in the interstellar medium of an irregular galaxy are unfavorable for amplification of the magnetic field because of the slow rotation and low shearing rate. We investigate the cosmic-ray driven dynamo in the interstellar medium of an irregular galaxy. We study its efficiency under the conditions of slow rotation and weak shear. The star formation is also taken into account in our model and is parametrized by the frequency of explosions and modulations of activity. The numerical model includes a magnetohydrodynamical dynamo driven by cosmic rays that is injected into the interstellar medium by randomly exploding supernovae. In the model, we also include essential elements such as vertical gravity of the disk, differential rotation approximated by the shearing box, and resistivity leading to magnetic reconnection. We find that even slow galactic rotation with a low shearing rate amplifies the magnetic field, and that rapid rotation with a low value of the shear enhances the efficiency of the dynamo. Our simulations have shown that a high amount of magnetic energy leaves the simulation box becoming an efficient source of intergalactic magnetic fields.
description: 9 pages, 6 figures
Compact single-seed, module-based laser system on a transportable high-precision atomic gravimeter
Creators: name: Oon, Fong En
name: Dumke, Rainer
Publisher: name: arXiv
Year: 2022
Subjects: subject: Atomic Physics (physics.atom-ph)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: A single-seed, module-based compact laser system is demonstrated on a transportable $^{87}\text{Rb}$-based high-precision atomic gravimeter. All the required laser frequencies for the atom interferometry are provided by free-space acousto-optic modulators (AOMs) and resonant electro-optic phase modulators (EOMs). The optical phase-locked loop between the two optical paths derived from the same laser provides an easy frequency manipulation between two laser frequencies separated by the hyperfine frequency of 6.835 GHz using an AOM and an EOM, respectively. Our scheme avoids parasite Raman transitions present in the direct EOM modulation scheme (modulating directly at the frequency of the hyperfine splitting), which have detrimental effects on the accuracy of the gravity measurements. The optical phase-locked loop also provides a convenient way for vibration compensation through the Raman lasers' phase offset. Furthermore, the modular design approach allows plug-and-play nature on each individual optic module and also increases the mechanical stability of the optical systems. We demonstrate high-precision gravity measurements with 17.8 $μ\text{Gal}$ stability over 250 seconds averaging time and 2.5 $μ\text{Gal}$ stability over 2 h averaging time.
description: 8 pages, 9 figures
title: ÐÑÐµÐ½ÐºÐ° Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð² Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð½ÐµÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð² Ð¼ÐµÐ³Ð°Ð¿Ð¾Ð»Ð¸ÑÐµ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐºÐ¾Ð²Ð°, Ð®Ð»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: 2018
Subjects: Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÐµ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ ÑÐ½ÐµÑÐ³Ð¸Ð¸
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸, Ð´Ð¾ÐºÐ°Ð·Ð°Ð²ÑÐ¸Ðµ ÑÐ²Ð¾Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÑÑ, ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÑÑ Ð¸ ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÑÑ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¿ÑÐ¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð² Ð¼ÐµÐ³Ð°Ð¿Ð¾Ð»Ð¸ÑÐ°Ñ.
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Ð ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ»Ð° Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¾Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¸ ÑÐ¾Ð»Ñ Ð²Ð¾Ð·Ð¾Ð±Ð½Ð¾Ð²Ð»ÑÐµÐ¼ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸ (ÐÐÐ­) Ð² Ð¼Ð¸ÑÐµ, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð¹ Ð¾Ð¿ÑÑ ÑÑÐ¸Ð¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿Ð¾Ð´Ð´ÐµÑÐ¶ÐºÐ¸ Ð°Ð»ÑÑÐµÑÐ½Ð°ÑÐ¸Ð²Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ½ÐµÑÐ³Ð¸Ð¸ Ð¸ Ð´Ð°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð¸ÑÑÑÑÐ¸Ñ Ð½Ð° Ð½ÐµÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸, Ð² ÑÐ°Ð¼ÐºÐ°Ñ ÑÐ½ÐµÑÐ³Ð¾Ð´ÐµÑÐ¸ÑÐ¸ÑÐ½ÑÑ Ð³Ð¾ÑÐ¾Ð´ÑÐºÐ¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ² Ð Ð¤. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð¿ÑÐ¸Ð²Ð»ÐµÐºÐ°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð½Ð° ÐÐÐ­, ÐºÐ°Ðº Ð´Ð»Ñ Ð¼ÐµÐ³Ð°Ð¿Ð¾Ð»Ð¸ÑÐ¾Ð² Ñ Ð¾ÑÐµÐ½Ñ Ð½Ð¸Ð·ÐºÐ¸Ð¼, Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸ Â«Ð½ÑÐ»ÐµÐ²ÑÐ¼Â» Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ð¾Ð¼ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¾Ð½Ð½ÑÑ ÐÐÐ­, ÑÐ°Ðº Ð¸ Ð´Ð»Ñ Ð¼ÐµÐ³Ð°Ð¿Ð¾Ð»Ð¸ÑÐ¾Ð², Ð³Ð´Ðµ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð» Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ½ÐµÑÐ³Ð¸Ð¸ ÐÐÐ­ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ Ð²ÑÑÐµ. ÐÐ»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð´Ð°Ð»ÑÐ½ÐµÐ¹ÑÐ¸Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¿Ð¾ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹, ÑÐ°Ð±Ð¾ÑÐ°ÑÑÐ¸Ñ Ð½Ð° ÐÐÐ­ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¼ÐµÐ³Ð°Ð¿Ð¾Ð»Ð¸ÑÐ¾Ð², Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÐºÐ°ÑÑÐ° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¹ Ð Ð¤ Ð¿Ð¾ Ð¿Ð¾ÑÐµÐ½ÑÐ¸Ð°Ð»Ñ Ð²Ð½ÐµÐ´ÑÐµÐ½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÐºÑÐ¾ÑÐ°Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÐÐÐ­.
A Finite-Volume Version of Aizenman-Higuchi Theorem for the 2d Ising Model
Creators: name: Coquille, Loren
name: Velenik, Yvan
Publisher: name: arXiv
Year: 2010
Subjects: subject: Probability (math.PR)
subject: Mathematical Physics (math-ph)
subject: FOS: Mathematics
subject: FOS: Physical sciences

description: In the late 1970s, in two celebrated papers, Aizenman and Higuchi independently established that all infinite-volume Gibbs measures of the two-dimensional ferromagnetic nearest-neighbor Ising model are convex combinations of the two pure phases. We present here a new approach to this result, with a number of advantages: (i) We obtain an optimal finite-volume, quantitative analogue (implying the classical claim); (ii) the scheme of our proof seems more natural and provides a better picture of the underlying phenomenon; (iii) this new approach might be applicable to systems for which the classical method fails.
description: A couple of typos corrected. To appear in Probab. Theory Relat. Fields
CAN LEARNING SITUATION AND ITEM’S HINT BE FACTORS THAT DETERMINE THE KNOWLEDGE TYPE AND COGNITIVE PROCESS ASSESSED BY MULTIPLE-CHOICE ITEMS?
Creators: name: Nyamgerel Ch.
Publisher: name: Вестник науки
Year: 2023
Subjects: BLOOM’S TAXONOMY
KNOWLEDGE TYPE
COGNITIVE PROCESS
LEARNING SITUATION
ITEM’S HINT

description: In this article presents result of the study on knowledge types and cognitive process levels of chemistry four parallel test items of GEE-2013, based on previously done two studies. Each test (2013-A, B, C, D) consisted of 31 selected-response items. Tests were administrated in June 2013 to N=2930-2964 examinees. The Educational Evaluation Center of Mongolia using parallel tests to ensure that measures the same knowledge, skills, or abilities. According to the methodology we developed, each item was determined that refers to which of the Knowledge type of Bloom’s Taxonomy. Due to the difference of “the learning situation”, only item 2 belongs to different knowledge type. Items 2, 6, and 12 of the tests depend on different cognitive process level due to differences in learning status and hints. The result of this study suggests retaining “the learning situation” and “item’s hint” as an important part of the test construction procedure.
Kosmos: l’Universo tra Scienza e Fede
Creators: admin
Publisher: name: Media Inaf
Year: 2009

Un incontro sul dibattito millenario tuttora aperto, alla luce delle ultime scoperte scientifiche in campo Cosmologico che, se  da un lato gettano luce su vecchi interrogativi, dall'altro ne aprono continuamente di nuovi.
title: Ð¤Ð¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ
title: Ð¿ÑÐ°ÐºÑÐ¸ÐºÑÐ¼
titleType: Subtitle
Creators: name: ÐÐ½ÑÐ¾Ð½ÐµÐ½ÐºÐ¾Ð²Ð°, Ð.
name: ÐÐµÐºÑÑÐ¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸Ñ
name: ÐÐ¸Ð³Ð´Ð°Ð¹, ÐÐ»ÐµÐ½Ð°
name: ÐÐ¾Ð»ÑÐ±ÐµÐ², Ð.
name: ÐÐ¸Ð»Ð¸Ð¼Ð½Ð¸Ðº, ÐÑÑÐµÑÐ»Ð°Ð²
name: ÐÐ¾ÑÐ¾Ð»ÐµÐ², Ð®.
name: Ð¡Ð°Ð²Ð¾ÐºÐ¸Ð½Ð°,  Ð. Ð.
name: Ð¡Ð°Ð¼Ð¾Ð¹Ð»Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: Ð¤Ð¸Ð»Ð¸Ð¿Ð¿Ð¾Ð²Ð°, Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÐÐ¸Ð¾ÑÐ¸Ð·Ð¸ÐºÐ°
ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñ
Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ð°

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð±Ð°Ð·Ð¾Ð²Ð¾Ð¼Ñ Ð²ÑÐ·Ð¾Ð²ÑÐºÐ¾Ð¼Ñ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ ÐÐ.Ð4, ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð¹ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ 223200.62 âÐ¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°â, ÐµÐµ ÐºÐ¾Ð¼Ð¿Ð¾Ð½ÐµÐ½ÑÑ âÐ¤Ð¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸Ñâ, Ð¿Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»Ñ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸: Ð°) âÐÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ°Ñ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°â; Ð±) âÐÑÐ¸ÐºÐ»Ð°Ð´Ð½Ð°Ñ ÑÐ¸Ð·Ð¸ÐºÐ° ÑÐµÐ°Ð±Ð¸Ð»Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñâ. Ð¡Ð¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¿Ð»Ð°Ð½Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð·Ð°Ð½ÑÑÐ¸Ð¹, Ð¿ÐµÑÐµÑÐµÐ½Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð´Ð»Ñ ÑÐ°Ð¼Ð¾Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ Ðº Ð·Ð°Ð½ÑÑÐ¸ÑÐ¼, Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÐ°Ð±Ð¾Ñ, Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐºÐ°Ð·Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¸ Ð·Ð°ÑÐ¸ÑÐµ ÐºÑÑÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐµÐ´ÑÑÐ²Ð° Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð² Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÐµÐ½Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÑÐ½ÐºÑÐ¸Ð¹ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ¸Ð·Ð¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸ÑÑÐµÐ¼ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ°. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÐ°ÐºÑÐ»ÑÑÐµÑÐ° Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½ÑÐºÐ¾Ð¹ ÑÐ¸Ð·Ð¸ÐºÐ¸ Ð¸ Ð±Ð¸Ð¾Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ¸Ð¸.
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ñ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
TECHNICAL DIAGNOSTICS OF ELECTRICAL EQUIPMENT BASED ON FUZZY LOGIC
Creators: name: Hasanov, A.I.
Publisher: name: Вестник науки
Year: 2023
Subjects: FUZZY LOGIC
REACTIVE POWER
SVC
VOLTAGE STABILITY

description: Voltage stability is one of the important factors in power system. The generation of harmonics, which can lead to voltage surges, voltage surges, and system instability. To compensate for all these problems of the transmission system, svc is used. A Static VAR Compensator (SVC) was used as an additional control to improve the transient stability and power droop of the system. The problem of svc with fuzzy logic controller is more adapted to the prevailing load requirement to maintain the stability of heavy load or lightening system. Static VAR compensator is chosen as a low cost solution to replace conventional capacitor bank, thus durable and flexible allowing the modal voltage to be adjusted.
Fixing the BMS frame of numerical relativity waveforms with BMS charges
Creators: name: Mitman, Keefe
name: Stein, Leo C.
name: Boyle, Michael
name: Deppe, Nils
name: Hébert, François
name: Kidder, Lawrence E.
name: Moxon, Jordan
name: Scheel, Mark A.
name: Teukolsky, Saul A.
name: Throwe, William
name: Vu, Nils L.
Publisher: name: arXiv
Year: 2022
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: The Bondi-van der Burg-Metzner-Sachs (BMS) group, which uniquely describes the symmetries of asymptotic infinity and therefore of the gravitational waves that propagate there, has become increasingly important for accurate modeling of waveforms. In particular, waveform models, such as post-Newtonian (PN) expressions, numerical relativity (NR), and black hole perturbation theory, produce results that are in different BMS frames. Consequently, to build a model for the waveforms produced during the merging of compact objects, which ideally would be a hybridization of PN, NR, and black hole perturbation theory, one needs a fast and robust method for fixing the BMS freedoms. In this work, we present the first means of fixing the entire BMS freedom of NR waveforms to match the frame of either PN waveforms or black hole perturbation theory. We achieve this by finding the BMS transformations that change certain charges in a prescribed way -- e.g., finding the center-of-mass transformation that maps the center-of-mass charge to a mean of zero. We find that this new method is 20 times faster, and more correct when mapping to the superrest frame, than previous methods that relied on optimization algorithms. Furthermore, in the course of developing this charge-based frame fixing method, we compute the PN expression for the Moreschi supermomentum to 3PN order without spins and 2PN order with spins. This Moreschi supermomentum is effectively equivalent to the energy flux or the null memory contribution at future null infinity $\mathscr{I}^{+}$. From this PN calculation, we also compute oscillatory ($m\not=0$ modes) and spin-dependent memory terms that have not been identified previously or have been missing from strain expressions in the post-Newtonian literature.
description: 16+4 pages with 2 appendices, 4 figures, 1 table
L’universo in evoluzione
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2009

Dal Big Bang alla vita. A Bologna, fino al 2 dicembre, un affascinante percorso lungo 13 miliardi di anni. Con biologi, geologi, e gli astronomi dell'Osservatorio e dell'Università.
A computational model of affects
Creators: name: Turkia, Mika
Publisher: name: arXiv
Year: 2008
Subjects: subject: Artificial Intelligence (cs.AI)
subject: Multiagent Systems (cs.MA)
subject: FOS: Computer and information sciences
subject: I.2.11; J.4

description: This article provides a simple logical structure, in which affective concepts (i.e. concepts related to emotions and feelings) can be defined. The set of affects defined is similar to the set of emotions covered in the OCC model (Ortony A., Collins A., and Clore G. L.: The Cognitive Structure of Emotions. Cambridge University Press, 1988), but the model presented in this article is fully computationally defined.
description: A pre-print version; final version published in D. Dietrich et al. (Eds.): Simulating the Mind. Springer 2009, see http://www.springer.com/springerwiennewyork/computer+science/book/978-3-211-09450-1 . 7 pages, 2 figures
Localization via fractional moments for models on $\mathbb{Z}$ with single-site potentials of finite support
Creators: name: Elgart, Alexander
name: Tautenhahn, Martin
name: Veselić, Ivan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mathematical Physics (math-ph)
subject: Spectral Theory (math.SP)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 82B44, 60H25, 35J10

description: One of the fundamental results in the theory of localization for discrete Schrödinger operators with random potentials is the exponential decay of Green's function and the absence of continuous spectrum. In this paper we provide a new variant of these results for one-dimensional alloy-type potentials with finitely supported sign-changing single-site potentials using the fractional moment method.
description: LaTeX-file, 26 pages with 2 LaTeX figures
Additional file 7 of Association of self-efficacy, risk attitudes, and time preferences with health-related quality of life and functioning after total hip or knee replacement – Results of the MobilE-TRA 2 cohort
Creators: name: Fuchs, Sebastian
name: Schwettmann, Lars
name: Katzenberger, Benedict
name: Paulus, Alexander
name: Holzapfel, Boris Michael
name: Biebl, Johanna Theresia
name: Weigl, Martin
Publisher: name: figshare
Year: 2025
Subjects: subject: Medicine
subject: Biotechnology
subject: Sociology
subject: FOS: Sociology
subject: Science Policy

description: Supplementary Material 7
Additional file 1 of Clinico-pathologic relationships with Ki67 and its change with short-term aromatase inhibitor treatment in primary ER + breast cancer: further results from the POETIC trial (CRUK/07/015)
Creators: name: Bliss, Judith M.
name: Tovey, Holly
name: Evans, Abigail
name: Holcombe, Chris
name: Horgan, Kieran
name: Mallon, Elizabeth
name: Vidya, Raghavan
name: Skene, Anthony
name: Dodson, Andrew
name: Hills, Margaret
name: Detre, Simone
name: Zabaglo, Lila
name: Banerji, Jane
name: Kilburn, Lucy
name: Morden, James P.
name: Robertson, John F. R.
name: Smith, Ian
name: Dowsett, Mitch
Publisher: name: figshare
Year: 2023
Subjects: subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Physiology
subject: Pharmacology
subject: Biotechnology
subject: Biological Sciences not elsewhere classified
subject: Cancer
subject: Science Policy
subject: Hematology

description: Additional file 1: Fig. S1. Distribution of Ki67Baseline a. Distribution of Ki67 % positive cells b. Distribution of ln(Ki67+0.1) c. Distribution of Ki67Baseline by HER2 status
The Screened Field of a Test Particle
Creators: name: Dewar, R. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences

description: The screened field (forward field and wake) of a test particle moving at constant velocity through an unmagnetized collisionless plasma is calculated analytically and numerically. This paper is based on unpublished material from my MSc thesis, supervised by the late Dr K. C. Hines.
description: 27 pp, 14 fig Publ "In Celeb Of KC Hines," www.worldscibooks.com/physics/7604.html. Based on Chs 2 & 3 of "Particle-field interactions in a plasma," RL Dewar, MSc Thesis, U Melbourne '67. v2: $\sin\psi$ and $\cos\psi$ interchanged after Eq. (4.1); v3: typos corrected pp 3, 4, 5, 19, in partic. repl. $q$ by $q/\epsilon_0$ & putting hat on k in arg. of \Phi in Eq.(2.5). See also arXiv 1107.5201
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐ²ÐµÑÐ¸Ð»ÑÐ½Ð¸ÐºÐ¾Ð² Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¶Ð¸Ð»Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ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¨ÑÐ»Ð°ÐµÐ²Ð°, ÐÐ»ÑÐ³Ð°
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Ð¸Ð»ÑÐµ Ð·Ð´Ð°Ð½Ð¸Ñ
ÐÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ½Ð¾Ðµ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸Ðµ
ÐÐ¸Ð¾Ð´Ñ ÑÐ²ÐµÑÐ¾Ð¸Ð·Ð»ÑÑÐ°ÑÑÐ¸Ðµ
Ð­Ð»ÐµÐºÑÑÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÐºÐ°
Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ Ð´Ð¸ÑÐºÐ¾Ð¼ÑÐ¾ÑÑÐ°

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐ²ÐµÑÐµÐ½Ð¸Ðµ Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸ÐµÐ¼ ÑÐ²ÐµÑÐ¾Ð´Ð¸Ð¾Ð´Ð½ÑÑ Ð¸ Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ½ÑÑ ÑÐ²ÐµÑÐ¸Ð»ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ ÑÑÐ°Ð¶Ð° Ð¶Ð¸Ð»Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¿Ð»Ð¾ÑÐ°Ð´ÑÑ 310,77 Ð¼2. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ ÑÐµÑÐµÐ½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð·Ð°Ð´Ð°ÑÐ¸: ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ Ñ ÑÑÐµÑÐ¾Ð¼ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÑ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ¾Ð², Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ°ÑÑÐµÑÐ½ÑÐµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð²ÑÐ±Ð¾Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¾Ð² Ð¸ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº ÑÐ²ÐµÑÐ¾Ð´Ð¸Ð¾Ð´Ð½ÑÑ Ð¸ Ð»ÑÐ¼Ð¸Ð½ÐµÑÑÐµÐ½ÑÐ½ÑÑ Ð»Ð°Ð¼Ð¿ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼ Nanocad Ð­Ð»ÐµÐºÑÑÐ¾ Ð¸ DIALux . Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑ Ð´Ð¸ÑÐºÐ¾Ð¼ÑÐ¾ÑÑÐ°.
title: ÐÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÐ·ÑÐºÐ° Ð´Ð»Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ¿Ð°Ð¼Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¯ÐºÐ¾Ð²Ð»ÐµÐ²Ð°, Ð®Ð»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: Ð²ÐµÐºÑÐ¾ÑÐ½Ð°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ ÑÐµÐºÑÑÐ°
ÑÐµÐ½ÑÐ¸Ð¼ÐµÐ½Ñ-Ð°Ð½Ð°Ð»Ð¸Ð·
ÑÐµÐ¼Ð°Ð½ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·
ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½ÑÐ¹ ÑÐ·ÑÐº
ÑÐ¿Ð°Ð¼
Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ Ð¿Ð¾ÑÑÑ

description: ÐÐ°ÑÑÐ¾ÑÑÐ°Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÑ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ¿Ð°Ð¼Ð°. ÐÑÐ»Ð¸ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ñ word2vec, Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² - Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµ Ð²ÐµÐºÑÐ¾ÑÐ¾Ð² Ñ ÑÑÐµÑÐ¾Ð¼ Ð²ÑÐ¾Ð´ÑÑÐ¸Ñ Ð² ÑÐ»Ð¾Ð²Ð¾ Ð¼Ð¾ÑÑÐµÐ¼. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ»ÑÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð° Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ ÑÐ¿Ð¾ÑÐ¾Ð± Ð´Ð»Ñ Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ñ ÑÐ¿Ð°Ð¼Ð° Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ word2vec, ÑÐ¿Ð¾ÑÐ¾Ð± Ð¿ÑÐ¾ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½ Ð½Ð° Ð¾Ð±ÑÑÐ½Ð¾Ð¼ word2vec Ð¸ Ð½Ð° word2vec Ñ Ð¼Ð¾ÑÑÐµÐ¼Ð½Ð¾Ð¹ Ð¼Ð¾Ð´Ð¸ÑÐ¸ÐºÐ°ÑÐ¸ÐµÐ¹. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÐµÐ°Ð»Ð¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð².
Astri e particelle. Le parole dell’Universo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2009

Mostra realizzata dell'Istituto Nazionale di Fisica Nucleare, l'Istituto Nazionale di Astrofisica e l'Agenzia Spaziale Italiana, con la direzione scientifica di Roberto Battiston. Roma, Palaexpo, dal 27 ottobre 2009 al 14 febbraio 2010.
title: Ð¡Ð¾Ð³Ð»Ð°ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð½ÑÐµÑÐµÑÐ¾Ð² Ð¿ÑÐ±Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¸ ÑÐ°ÑÑÐ½ÑÑ Ð¿Ð°ÑÑÐ½ÐµÑÐ¾Ð² ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½Ñ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð¸Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð°
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ÑÐ²Ð¾Ð²Ð°, ÐÐ»ÐµÐºÑÐ°Ð½Ð´ÑÐ°
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: Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ðµ Ð¿Ð°ÑÑÐ½ÑÑÑÑÐ²Ð¾
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ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ
ÑÐ°ÑÑÐ½Ð¾Ðµ ÑÐ¸Ð½Ð°Ð½ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð³Ð¾ÑÐ¾Ð´ Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³. Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð° Ð¸ ÑÐ¸ÑÐ¼, ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð°ÑÑÐ½ÐµÑÑÐºÐ¸Ñ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ð¹ Ð¼ÐµÐ¶Ð´Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð¾Ð¼ Ð¸ ÑÐ¸ÑÐ¼Ð°Ð¼Ð¸, ÑÐ°ÐºÑÐ¾ÑÑ ÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð°. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÑÐ° Ð¸ ÑÐ¾Ð»Ð¸ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²Ð° Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¸ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð°. Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐµ Ð²ÑÐµÐ¼Ñ Ð² ÑÑÐ»Ð¾Ð²Ð¸ÑÑ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¸Ð½Ð½Ð¾Ð²Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¾Ð±Ð½Ð¾Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐ¸ Ð Ð¾ÑÑÐ¸Ð¸ Ð²ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ðµ Ð´ÐµÑÐ¸ÑÐ¸ÑÐ° Ð±ÑÐ´Ð¶ÐµÑÐ½ÑÑ ÑÐµÑÑÑÑÐ¾Ð² Ð²ÑÐµ Ð±Ð¾Ð»ÐµÐµ Ð°ÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼ ÑÑÐ°Ð½Ð¾Ð²Ð¸ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼Ð° Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ°ÑÑÐ½Ð¾Ð³Ð¾ Ð¿Ð°ÑÑÐ½ÐµÑÑÑÐ²Ð° Ð´Ð»Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¸Ð½ÑÑÐ°ÑÑÑÑÐºÑÑÑÐ½ÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð².
title: ÐÐµÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ Ð¿ÑÐ¸ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ¾ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ°Ð»ÑÐ½ÑÑ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐµÑÐ½Ð¸ÑÐºÐ¸Ð¹, ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
name: ÐÐ°ÑÐ²ÐµÐµÐ², ÐÐ³Ð¾ÑÑ
name: ÐÐµÑÐ½Ð¸ÑÐºÐ°Ñ, ÐÑÐ´Ð¼Ð¸Ð»Ð°
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: 2019
Subjects: ÐÑÐ»Ð¸Ð²ÐºÐ¸ ÑÑÐ°Ð»ÑÐ½ÑÐµ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ 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 Ð¾ÑÐ»Ð¸Ð²ÐºÐ¸ Ð´Ð»Ñ Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸Ð¹ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÐ½ÑÑ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº ÑÑÐ°Ð»ÑÐ½ÑÑ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº. Ð ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÑÐ¸Ñ ÑÐ°ÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸Ð¹.
Un timbro postale per la “Croce del Nord”
Creators: admin
Publisher: name: Media Inaf
Year: 2009

Domenica 1 novembre dalle ore 15 alle 18 sarà presente presso il Centro Visite “Marcello Ceccarelli” un ufficio temporaneo delle Poste Italiane con un annullo (timbro) speciale realizzato in occasione dei 45 anni del radiotelescopio Croce del Nord. Con tale annullo sarà possibile timbrare le cartoline raffiguranti la Croce del Nord, affrancate con i francobolli… Leggi tutto »
The local B-polarization of the CMB: a very sensitive probe of cosmic defects
Creators: name: Garcia-Bellido, Juan
name: Durrer, Ruth
name: Fenu, Elisa
name: Figueroa, Daniel G.
name: Kunz, Martin
Publisher: name: arXiv
Year: 2010
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: General Relativity and Quantum Cosmology (gr-qc)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: We present a new and especially powerful signature of cosmic strings and other topological or non-topological defects in the polarization of the cosmic microwave background (CMB). We show that even if defects contribute 1% or less in the CMB temperature anisotropy spectrum, their signature in the local $\tilde{B}$-polarization correlation function at angular scales of tens of arc minutes is much larger than that due to gravitational waves from inflation, even if the latter contribute with a ratio as big as $r\simeq 0.1$ to the temperature anisotropies. We show that when going from non-local to local $\tilde{B}$-polarization, the ratio of the defect signal-to-noise with respect to the inflationary value increases by about an order of magnitude. Proposed B-polarization experiments, with a good sensitivity on arcminute scales, may either detect a contribution from topological defects produced after inflation or place stringent limits on them. Even Planck should be able to improve present constraints on defect models by at least an order of magnitude, to the level of $\ep <10^{-7}$. A future full-sky experiment like CMBpol, with polarization sensitivities of the order of $1μ$K-arcmin, will be able to constrain the defect parameter $\ep=Gv^2$ to a few $\times10^{-9}$, depending on the defect model.
description: Version Published in Physics Letters B
Unitary Integrals and Related Matrix Models
Creators: name: Morozov, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: Mathematical Physics (math-ph)
subject: FOS: Physical sciences

description: Concise review of the basic properties of unitary matrix integrals. They are studied with the help of the three matrix models: the ordinary unitary model, Brezin-Gross-Witten model and the Harish-Charndra-Itzykson-Zuber model. Especial attention is paid to the tricky sides of the story, from De Wit-t'Hooft anomaly in unitary integrals to the problem of correlators with Itzykson-Zuber measure. Of technical tools emphasized is the method of character expansions. The subject of unitary integrals remains highly under-investigated and a lot of new results are expected in this field when it attracts sufficient attention.
description: 27 pages
title: Ð¤ÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¼ÑÑÑ Ð¿Ð»ÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ° Ð»ÑÐ¶Ð½Ð¸ÐºÐ¾Ð²-Ð³Ð¾Ð½ÑÐ¸ÐºÐ¾Ð² Ð¿ÑÐ¸ Ð¿ÐµÑÐµÑ Ð¾Ð´Ðµ Ð½Ð° ÑÑÐ°Ð¿ Ð²ÑÑÑÐµÐ³Ð¾ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð°
title: Upper body muscles functionality in cross-country skiers when moving to the stage of higher sportsmanship
Creators: name: Ð ÐµÑÑÐºÐ°Ñ, ÐÐ»ÐµÐ½Ð°
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: Ð»ÑÐ¶Ð½Ð¸ÐºÐ¸-Ð³Ð¾Ð½ÑÐ¸ÐºÐ¸
ÑÑÐ°Ð¿ Ð²ÑÑÑÐµÐ³Ð¾ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð°
ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸
Ð¼ÑÑÑÑ Ð¿Ð»ÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ°
cross-country skiers
stage of highly qualified
functionality
upper body skeletal muscles

description: Ð ÑÑÐ°ÑÑÐµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð¾Ð² ÑÑÐ½ÐºÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼ÑÑÑ Ð¿Ð»ÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ° Ð»ÑÐ¶Ð½Ð¸ÐºÐ¾Ð²-Ð³Ð¾Ð½ÑÐ¸ÐºÐ¾Ð² Ð½Ð° ÑÑÐ°Ð¿Ðµ Ð²ÑÑÑÐµÐ³Ð¾ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð° Ð¸ ÑÑÐ°Ð¿Ðµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð°. Ð ÑÐ¾Ð´Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²Ð»ÐµÐ½Ð¾, ÑÑÐ¾ Ð½Ð° ÑÑÐ°Ð¿Ðµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÑÐµÑÑÑÐ²Ð° Ð±Ð¾Ð»ÑÑÐµ Ð¿Ð¾Ð»Ð¾Ð²Ð¸Ð½Ñ Ð»ÑÐ¶Ð½Ð¸ÐºÐ¾Ð² Ð¸ Ð»ÑÐ¶Ð½Ð¸Ñ Ð¸Ð¼ÐµÑÑ Ð½Ð¸Ð·ÐºÐ¸Ð¹ Ð¸ Ð½Ð¸Ð¶Ðµ ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ ÑÐºÐ¾ÑÐ¾ÑÑÐ½Ð¾-ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¼ÑÑÑ Ð¿Ð»ÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ° Ð¸ Ð±Ð¾Ð»ÑÑÐµ Ð¿Ð¾Ð»Ð¾Ð²Ð¸Ð½Ñ Ð»ÑÐ¶Ð½Ð¸ÐºÐ¾Ð² Ð¸Ð¼ÐµÑÑ Ð½Ð¸Ð·ÐºÐ¸Ð¹ Ð¸ Ð½Ð¸Ð¶Ðµ ÑÑÐµÐ´Ð½ÐµÐ³Ð¾ ÑÑÐ¾Ð²ÐµÐ½Ñ ÑÐ¸Ð»Ð¾Ð²Ð¾Ð¹ Ð²ÑÐ½Ð¾ÑÐ»Ð¸Ð²Ð¾ÑÑÐ¸ Ð¼ÑÑÑ Ð¿Ð»ÐµÑÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾ÑÑÐ°.
description: The article provides a comparative description of the fulfillment of the standards of upper body muscles functionality for cross-country skiers at the stage of higher sportsmanship and the stage of improving sportsmanship. In the course of the study, it was found that at the stage of improving sportsmanship, more than half of cross-country skiers have a low and lower average level of development of upper body muscles functionality.
A Capodimonte tra Luna e musica
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2009

Mercoledì 16 settembre 2009 alle ore 19.00 presso l'Auditorium dell'INAF-Osservatorio Astronomico di Capodimonte in via Moiariello 16, a Napoli, si terrà la manifestazione "A Capodimonte tra Luna e Musica - I Luoghi della Musica tra Libri e Astri"
Bitemporal Dynamics Sinai Divergence, An Energetic Analog to Boltzmann's Entropy?
Creators: name: Rossler, Otto E.
name: Movassagh, Ramis
Publisher: name: arXiv
Year: 2008
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: Sinai chaos is characterized by exponential divergence between neighboring trajectories of a point billiard. If the repulsive potential of the finite-diameter fixed particle in the middle of the table is made smooth, the Sinai divergence persists with finite measure. So it does if the smooth potential is made attractive. So it still does if the potential is in addition made time-dependent (periodic). Then a systematic decrease in energy of the moving particle can be predicted to occur in both time directions for a long time. If so, classical entropy acquires an analog in real space.
description: 2 pages
title: ÐÐºÑÑÐ°Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾-ÑÐ¼Ð¸ÑÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð¶Ð°Ð½Ð¾Ð²Ð°, ÐÐ¸Ð½Ð°
name: ÐÐ¾ÑÐ°Ð±Ð»ÐµÐ², ÐÐ°Ð´Ð¸Ð¼
name: ÐÑÐ´Ð¸Ð½Ð¾Ð², Ð®ÑÐ¸Ð¹
Publisher: name: ÐÐÐ
Year: 1985
Subjects: Ð¡Ð¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ

description: Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ¸Ð·Ð¸ÐºÐ¾-ÑÐ¸Ð¼Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¿ÑÐ¸Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ²ÐµÑÐ´ÑÑ ÑÐµÐ» Ð¼ÐµÑÐ¾Ð´Ð°Ð¼Ð¸ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾-ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾-ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸ Ñ ÑÐ³Ð»Ð¾Ð²ÑÐ¼ ÑÐ°Ð·ÑÐµÑÐµÐ½Ð¸ÐµÐ¼ Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð¸Ð·Ð²Ð»ÐµÑÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾Ð± ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¼ ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸ Ð¿ÑÐ¸Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ½Ð¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐ²ÐµÑÐ´ÑÑ ÑÐµÐ» ÑÑÐ¸Ð¼ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼. ÐÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¼ÐµÑÐ¾Ð´Ñ Ð½Ð¸Ð·ÐºÐ¾ÑÐ½ÐµÑÐ³ÐµÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð²ÑÐ¾ÑÐ¸ÑÐ½Ð¾-ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸; ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¾ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸ ÑÐ¿Ð¸Ð½-Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð²; ÐºÑÐ°ÑÐºÐ¾ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¸ Ð´ÐµÑÐµÐºÑÐ¾ÑÑ Ð¿Ð¾Ð»ÑÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð½ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð², Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²Ð¸Ð´Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸ Ð¾ Ð¿Ð¾Ð²ÐµÑÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ°Ñ ÑÐ¼Ð¸ÑÑÐ¸Ð¸ Ð¸ ÑÐ°ÑÑÐµÑÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¾Ð², Ð¿Ð¾Ð»ÑÑÐ°ÐµÐ¼ÑÐµ Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÑÐ¾Ð¹ ÑÐ¿ÐµÐºÑÑÐ¾ÑÐºÐ¾Ð¿Ð¸Ð¸. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ 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¸Ð·Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°Â», Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ ÑÑÑÐ´ÐµÐ½ÑÐ°Ð¼, Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ°Ð¼ Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ°Ð¼ Ð±Ð»Ð¸Ð·ÐºÐ¸Ñ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹.
The effect of magnetic field on the inner Galactic rotation curve
Creators: name: Chan, Man Ho
name: Del Popolo, Antonino
Publisher: name: arXiv
Year: 2022
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: In the past few decades, some studies pointed out that magnetic field might affect the rotation curves in galaxies. However, the impact is relatively small compared with the effects of dark matter and the baryonic components. In this letter, we revisit the impact of magnetic field on the rotation curve of our Galaxy. We show that the inner Galactic rotation curve could be affected significantly by the magnetic field. The addition of the inner bulge component, which has been proposed previously to account for the inner rotation curve data, is not necessary. The magnetic field contribution can fully account for the excess of the inner rotation velocity between 5 pc to 50 pc from the Galactic Centre. Our analysis can also constrain the azimuthal component of the central regular magnetic field strength to $B_0 \sim 50-60$ $μ$G, which is consistent with the observed range.
description: Accepted in MNRAS Letters
Scoping review protocol
Creators: name: Prüsse, Julie Hougaard
name: Bunkenborg, Gitte
name: Bove, Dorthe Gaby
name: Hansen, Stine Thestrup
Publisher: name: OSF Registries
Year: 2023
Subjects: subject: Health Information Technology
subject: Medicine and Health Sciences
subject: Other Nursing
subject: Nursing
subject: FOS: Health sciences

description: Protocol for scoping review on Point-of-care Documentation in somatic inpatient hospital settings