cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ 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¸ÑÐ·Ð¾ÐµÐ², ÐÐ¸ÑÐ¸Ð±ÐµÐº
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°Ð½Ð°Ð»Ð¸Ð·
Ð¾Ð±ÑÐµÐ¼ Ð¿ÑÐ¾Ð´Ð°Ð¶
Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°

description: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ñ Ð¿Ð¾Ð½ÑÑÐ¸Ðµ, Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð¸ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ, Ð¸Ð·ÑÑÐµÐ½ Ð¿ÑÐ¾ÑÐµÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ, Ð¾Ð¿Ð¸ÑÐ°Ð½Ñ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð° Ð´Ð¸Ð½Ð°Ð¼Ð¸ÐºÐ° Ð¸ ÑÑÑÑÐºÑÑÑÐ° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð° Ð²ÑÐ¿ÑÑÐºÐ° Ð¸ Ð¿ÑÐ¾Ð´Ð°Ð¶ ÑÐ¾Ð²Ð°ÑÐ¾Ð² ÐÐÐ Â«ÐÐ Â«ÐÐ°ÑÐ½Ð¸ÑÐ°Â», Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¿ÑÑÐ¸ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÐÐÐ Â«ÐÐ Â«ÐÐ°ÑÐ½Ð¸ÑÐ°Â».
Le stelle oversize di Hubble
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Mai prima d'ora era stata scoperta una concentrazione di astri così massicci tutti in un sol colpo: c'è riuscito un team di astronomi guidato da Paul Crowther dell’Università di Sheffield nel Regno Unito, scandagliando l'ammasso R136 con il telescopio spaziale di Nasa ed ESA
Measurement of the Atmospheric Neutrino Induced Muon Flux with the MACRO
  detector
Creators: name: Bernardini, Paolo
Publisher: name: INFN Open Access Repository
Year: 1998

description: The flux of neutrino-induced muons has been measured with the MACRO detector.
Different event topologies have been detected, due to neutrino interactions in
the apparatus and in the rock below it. The upward-throughgoing muon sample is
the larger one and is generated by neutrinos with an average energy of ~ 100
GeV. The observed upward-throughgoing muons are 26% fewer than expected and the
zenith angle distribution does not fit with the expected one. Assuming neutrino
oscillations, both measurements suggest maximum mixing and Dm2 of a few times
10-3 eV2. The other event categories due to interactions of low-energy
neutrinos (average energy ~ 4 GeV) have been recently studied and the results
of these new analyses are presented for the first time at this workshop. These
data show a regular deficit of observed events in each angular bin, as expected
assuming neutrino oscillations with maximum mixing, in agreement with the
analysis of the upward-throughgoing muona sample.
A study of British Columbia's tree farm licence tenure and a discussion of its applicability in Kenya
Creators: name: Spears, John Stephen
Publisher: name: University of British Columbia
Year: 2011

description: In Kenya, as in British Columbia, a high percentage of the forest land is owned by the Crown. Since Government controls most of the raw material for the forest industry, its timber disposal policies will have a considerable influence on the pattern of industrial development. The most suitable policy will be that which allows the maximum degree of industrial efficiency to be achieved and at the same time, adequately protects the public interest in the forest resource. The main methods of timber disposal open to the Kenya Government are: (i) To dispose of all Crown timber by public auction. (ii) To grant leases of Crown timber to private enterprise concerns, Government retaining the responsibility for forest management. (iii) To grant leases to private enterprise concerns and, in addition, to delegate to these same concerns the responsibility for forest management. Such a lease would be equivalent to British Columbia's Tree Farm Licence. (iv) To dispose of Crown timber by outright alienation. (v) To establish State manufacturing plants. It is not essential that the Government commit itself to any particular one of the above alternatives in practice, a combination of two or more may be desirable. This thesis is primarily concerned with the Tree Farm Licence method of timber disposal. The main objectives are: to study the progress of the Tree Farm Licence, to assess its advantages and disadvantages and to discuss its applicability in Kenya. The main conclusions drawn are that the Tree Farm Licence has brought several important benefits to British Columbia and in particular, has encouraged the establishment of the large integrated forest industries which play an important part in supporting the Provincial economy. The introduction of a similar licence into Kenya would be desirable, but for political reasons probably impracticable at present.
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð° Ð½Ð° ÑÑÐ°ÑÐ¸ÑÐµÑÐºÑÑ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð¸ ÑÑÐµÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÑ ÑÐ¸ÑÐ°Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¿Ð»Ð°Ð²Ð° ÐÐ¢-7Ð
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ÐµÐ¾Ð½Ð¾Ð², ÐÐ°Ð½Ð¸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: 2018
Subjects: Ð¢Ð¸ÑÐ°Ð½Ð¾Ð²ÑÐµ ÑÐ¿Ð»Ð°Ð²Ñ
ÐÐ¾Ð´Ð¾ÑÐ¾Ð´

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¿ÑÐ¸ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÑÐ¸ÑÐ°Ð½Ð¾Ð²ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² Ð² ÑÑÑÐ±Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ Ð¿Ð°ÑÐ¾Ð³ÐµÐ½ÐµÑÐ¸ÑÑÑÑÐµÐ³Ð¾ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÐ¾Ð´ÑÐ¾Ð±Ð½Ð¾ Ð¸Ð·ÑÑÐµÐ½Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð° Ð½Ð° Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÑÐ¸ÑÐ°Ð½Ð¾Ð²ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ»Ð°ÑÑÐ¾Ð². Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð´Ð¸ÐºÐ¸ Ð´Ð»Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ Ð¸ÑÐ¿ÑÑÐ°Ð½Ð¸Ð¹ ÑÑÑÐ±ÑÐ°ÑÑÑ Ð¾Ð±ÑÐ°Ð·ÑÐ¾Ð² Ð¸Ð· ÑÐ¸ÑÐ°Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¿Ð»Ð°Ð²Ð° ÐÐ¢-7Ð. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ñ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÐºÐ¾Ð½ÑÐµÐ½ÑÑÐ°ÑÐ¸Ð¹ Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð° Ð½Ð° ÑÑÐ°ÑÐ¸ÑÐµÑÐºÑÑ Ð¿ÑÐ¾ÑÐ½Ð¾ÑÑÑ Ð¸ ÑÑÐµÑÐ¸Ð½Ð¾ÑÑÐ¾Ð¹ÐºÐ¾ÑÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² ÑÑÑÐ±Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð· ÑÐ¸ÑÐ°Ð½Ð¾Ð²Ð¾Ð³Ð¾ ÑÐ¿Ð»Ð°Ð²Ð° ÐÐ¢-7Ð Ð² Ð´Ð¸Ð°Ð¿Ð°Ð·Ð¾Ð½Ðµ ÑÐµÐ¼Ð¿ÐµÑÐ°ÑÑÑ Ð¾Ñ +20Â°Ð¡ Ð´Ð¾ +350Â°Ð¡.
Proteine in microgravità
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

A quota 400 chilometri, là dove vola la Stazione Spaziale Internazionale, i cristalli di proteine crescono più belli e meglio. A dirlo è uno studio giapponese appena pubblicato, che dei cristalli ha monitorato la lentissima crescita e il tasso di dissoluzione grazie alla tecnica dell’interferometria laser
Existence and Uniqueness of Strong Solutions for a Compressible Multiphase Navier-Stokes Miscible Fluid-Flow Problem in Dimension n = 1
Creators: name: Michoski, C.
name: Vasseur, A.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Mathematical Physics (math-ph)
subject: Analysis of PDEs (math.AP)
subject: FOS: Physical sciences
subject: FOS: Mathematics
subject: 76T30, 76N10, 92C45

description: We prove the global existence and uniqueness of strong solutions for a compressible multifluid described by the barotropic Navier-Stokes equations in dim = 1. The result holds when the diffusion coefficient depends on the pressure. It relies on a global control in time of the L2 norm of the space derivative of the density, via a new kind of entropy.
description: 37 pages, 0 figures
Atmospheric and Astrophysics Neutrinos with MACRO
Creators: name: T. Montaruli
name: For The MACRO Collaboration
Publisher: name: INFN Open Access Repository
Year: 1998

description: MACRO can detect three topologies of neutrino induced events, corresponding
to different parent neutrino energies. The most numerous sample is made of
upward throughgoing muons induced by atmospheric neutrinos of average energy
100 GeV. We have observed less events than expected events and the observed
zenith distribution does not fit the expected one in the no-oscillation
hypothesis, giving a maximum probability of 0.1 percent. Considering the
neutrino (numu-nutau) oscillation hypothesis the best probability (17 percent)
is obtained for maximum mixing and difference of square masses of a few times
10-3 eV2. The other detected samples are due to internally produced events and
upward-going stopping muons, corresponding to an average neutrino energy of
around 4 GeV. The results concerning these lower energy sample show a deficit
and a shape of the angular distributions in agreement with that predicted by
the oscillation model suggested by the higher energy sample. No evidence of a
neutrino signal due to dark matter particles in the direction of the core of
the Earth and of the Sun has been found among the background due to atmospheric
neutrinos and limits have been set. The neutralino hypothesis is investigated
and limits on its mass are given.
DEIMS-SDR Site Data Model Snapshot
Creators: name: Wohner, Christoph
Publisher: name: Zenodo
Year: 2022
Subjects: DEIMS-SDR
data model
UML

description: This XMI file represents a snapshot of the site data model in UML as it is implemented in DEIMS-SDR (deims.org). It represents the status as of February 2022. For the latest version of the site data model of DEIMS-SDR, please refer to https://deims.org/models/?id=site
Palermo scopre le sue carte d’archivio
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Presentato al pubblico l’inventario completo dell'archivio storico dell'Osservatorio Astronomico di Palermo. Le carte conservate riguardano il periodo compreso tra la direzione di Giuseppe Piazzi, il sacerdote che scoprì Cerere, fino agli anni ’70 dello scorso secolo, passando per il “Gattopardo”, ovvero il Principe di Lampedusa, valente astronomo dilettante dell'Ottocento. Per raffigurarlo al meglio, nel 1962 Luchino Visconti chiese in prestito all'Osservatorio strumentazione e carte originali
title: ÐÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð² Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° Ð½Ð° ÑÑÐ°Ð´Ð¸Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ°
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Ð¾Ð¿Ð¾Ð²Ð°, ÐÐºÐ°ÑÐµÑ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: 2018
Subjects: Ð¾ÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ°
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾-ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
ÑÐ½Ð¸ÐºÐ°Ð»ÑÐ½Ð¾Ðµ Ð·Ð´Ð°Ð½Ð¸Ðµ

description: ÐÐ»Ñ ÐºÐ°ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð±ÑÐµÐºÑÐ° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÐ¸ÑÐºÐ¸, ÑÑÐ¾Ð±Ñ Ð¸Ð¼ÐµÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ ÑÐ¿ÑÐ°Ð²Ð»ÑÑÑ Ð¸Ð¼Ð¸. Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÐ¼ÐµÐ½ÑÑÐ°ÐµÑ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÑ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð³Ð»Ð¾Ð±Ð°Ð»ÑÐ½ÑÑ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¼Ð¾Ð³ÑÑ Ð¿ÑÐ¸Ð²ÐµÑÑÐ¸ Ðº Ð¿ÑÐµÐºÑÐ°ÑÐµÐ½Ð¸Ñ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°. ÐÑÐµÐ½ÐºÐ° ÑÐ¸ÑÐºÐ¾Ð² â Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾Ðµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð´Ð»Ñ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð»ÑÐ±Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ° ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð°, Ð° Ð¼ÐµÑÐ¾Ð´ ÑÐºÑÐ¿ÐµÑÑÐ½ÑÑ Ð¾ÑÐµÐ½Ð¾Ðº Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°ÑÑ Ð¸Ð½ÑÑÐ¸ÑÐ¸Ñ, Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐ¹ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½ÑÐ¹ Ð¾Ð¿ÑÑ ÑÑÐ°ÑÑÐ½Ð¸ÐºÐ¾Ð² Ð¾Ð¿ÑÐ¾ÑÐ°. ÐÐ°Ð½Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð¼ ÑÐ½Ð¸ÐºÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð·Ð´Ð°Ð½Ð¸Ñ Ñ Ð·Ð°Ð³Ð»ÑÐ±Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÑÐ½Ð´Ð°Ð¼ÐµÐ½ÑÐ° Ð½Ð° 16 Ð¼. ÐÐµÑÐ¾Ð´ ÑÐºÑÐ¿ÐµÑÑÐ½ÑÑ Ð¾ÑÐµÐ½Ð¾Ðº Ð¸ÑÐ¿Ð¾Ð»ÑÐ·ÑÐµÑÑÑ Ð² ÑÐ²ÑÐ·Ð¸ Ñ ÑÐµÐ¼, ÑÑÐ¾ Ð°Ð½Ð°Ð»Ð¾Ð³Ð¾Ð² ÑÐ°ÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÐºÑÐ°Ð¹Ð½Ðµ Ð¼Ð°Ð»Ð¾, Ð¸ Ð¼ÐµÑÐ¾Ð´Ñ ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ðµ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ ÑÐµÐ°Ð»ÑÐ½Ð¾ Ð¾ÑÐµÐ½Ð¸ÑÑ ÑÐ¸ÑÐºÐ¸.
Einstein a casa tua
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2016

Si chiama Einstein@home ed è un progetto di citizen science che dà a chiunque la possibilità di partecipare alla caccia alle onde gravitazionali. Ne parla a Media INAF Maria Alessandra Papa, Research Group Leader del progetto presso il Max Planck Institute for Gravitational Physics
Reversal of Thermal Rectification in Quantum Systems
Creators: name: Zhang, Lifa
name: Yan, Yonghong
name: Wu, Chang-Qin
name: Wang, Jian-Sheng
name: Li, Baowen
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We study thermal transport in anisotropic Heisenberg spin chains using the quantum master equation. It is found that thermal rectification changes sign when the external homogeneous magnetic field is varied. This reversal also occurs when the magnetic field becomes inhomogeneous. Moreover, we can tune the reversal of rectification by temperatures of the heat baths, the anisotropy and size of the spin chains.
description: 4 pages, 7 figures
title: ÐÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¸Ðº Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â»
titleType: Subtitle
Creators: name: ÐÑÐ´ÐºÐ¸Ð½, ÐÐ°Ð»ÐµÐ½ÑÐ¸Ð½
name: ÐÐ°ÑÐ¾Ð¼Ð¾Ð², ÐÐµÐ²
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: ÐÐ²Ð°Ð½ÑÐ¾Ð²Ð°Ñ ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÐºÐ°

description: ÐÐ°ÑÑÑÑ ÑÐ¸Ð·Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ, Ð¸Ð·Ð»Ð°Ð³Ð°ÑÑÑÑ Ð¼ÐµÑÐ¾Ð´Ñ Ð¸ Ð¾Ð¿Ð¸ÑÑÐ²Ð°ÑÑÑÑ ÑÐ²Ð»ÐµÐ½Ð¸Ñ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð»ÐµÐ¶Ð°Ñ Ð² Ð¾ÑÐ½Ð¾Ð²Ðµ ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÐºÐ¸. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð¿ÑÐ¸Ð±Ð¾ÑÐ°Ð¼ ÐºÐ²Ð°Ð½ÑÐ¾Ð²Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð¸ÐºÐ¸ Ð¸ ÐµÐµ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐ¼ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸ÑÐ¼ . Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð¿ÑÐ¸Ð½ÑÐ¸Ð¿Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÑÑÑÐ¾Ð¹ÑÑÐ², Ð´Ð°ÐµÑÑÑ Ð¸Ñ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ, Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ¾Ð² ÑÐ°ÑÑÐ¾ÑÑ (ÑÐµÐ·Ð¸ÐµÐ²ÑÑ, ÑÑÐ±Ð¸Ð´Ð¸ÐµÐ²ÑÑ, Ð²Ð¾Ð´Ð¾ÑÐ¾Ð´Ð½ÑÑ), ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ Ð¼Ð°Ð³Ð½Ð¸ÑÐ¾Ð¼ÐµÑÑÐ¾Ð², Ð¿Ð°ÑÐ°Ð¼Ð°Ð³Ð½Ð¸ÑÐ½ÑÑ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»ÐµÐ¹ , ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð»Ð°Ð·ÐµÑÐ¾Ð². ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¼Ð°Ð³Ð½Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ·Ð¾Ð½Ð°Ð½ÑÐ° Ð² ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ñ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÑ ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð³Ð½Ð°Ð»Ð¾Ð² Ð¸ Ð¯ÐÐ -ÑÐ¾Ð¼Ð¾Ð³ÑÐ°ÑÐ¸Ð¸. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð»Ð°Ð·ÐµÑÐ¾Ð² Ð² ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ ÑÑÑÐ°Ð½Ð¾Ð²ÐºÐ°Ñ, Ð»Ð°Ð·ÐµÑÐ½ÑÑ Ð³Ð¸ÑÐ¾ÑÐºÐ¾Ð¿Ð°Ñ Ð¸ Ð´Ð°Ð»ÑÐ½Ð¾Ð¼ÐµÑÐ°Ñ, Ð² ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð°Ñ Ð·Ð°Ð¿Ð¸ÑÐ¸ Ð¸ ÑÑÐ°Ð½ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¸, Ð² Ð¼ÐµÐ´Ð¸ÑÐ¸Ð½Ðµ, Ð² ÑÐ¸ÑÑÐµÐ¼Ð°Ñ ÐºÐ¾Ð½ÑÑÐ¾Ð»Ñ Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ñ Ð¸ Ð»Ð°Ð·ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐµÐ»ÐµÐ²Ð¸Ð´ÐµÐ½Ð¸Ñ. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ Ð°ÑÐ¿Ð¸ÑÐ°Ð½ÑÐ¾Ð², Ð¸Ð·ÑÑÐ°ÑÑÐ¸Ñ ÐºÐ²Ð°Ð½ÑÐ¾Ð²ÑÑ ÑÐ°Ð´Ð¸Ð¾ÑÐ¸Ð·Ð¸ÐºÑ, Ð¾Ð¿ÑÐ¾ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÑ ÑÐµÑÐ½Ð¸ÐºÑ Ð¸ Ð¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ.
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ÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
E se la materia oscura fosse pesante?
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Secondo uno studio teorico recente, la materia oscura potrebbe essere composta da particelle più massicce di quanto si sia assunto fino a ora: non WIMP, dunque, ma PIDM. L’ipotesi, avanzata da ricercatori della University of Southern Denmark e del CERN, potrà essere testata con esperimenti per la rivelazione di onde gravitazionali
The Rise of the AGB in the Galactic Halo: Mg Isotopic Ratios and High Precision Elemental Abundances in M71 Giants
Creators: name: Melendez, Jorge
name: Cohen, Judy
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: High-resolution (R ~ 100 000), high signal-to-noise spectra of M71 giants have been obtained with HIRES at the KeckI Telescope in order to measure their Mg isotopic ratios, as well as elemental abundances of C, N, O, Na, Mg, Al, Si, Ca, Ti, Ni, Zr and La. We demonstrate that M71 has two populations, the first having weak CN, normal O, Na, Mg, and Al, and a low ratio of 26Mg/Mg (~4%) consistent with models of galactic chemical evolution with no contribution from AGB stars. The Galactic halo could have been formed from the dissolution of globular clusters prior to their intermediate mass stars reaching the AGB. The second population has enhanced Na and Al accompanied by lower O and by higher 26Mg/Mg (~8%), consistent with models which do incorporate ejecta from AGB stars via normal stellar winds. All the M71 giants have identical [Fe/H], [Si/Fe], [Ca/Fe], [Ti/Fe] and [Ni/Fe] to within sigma = 0.04 dex (10%). We therefore infer that the timescale for formation of the first generation of stars we see today in this globular cluster must be sufficiently short to avoid a contribution from AGB stars, i.e. less than ~0.3Gyr. Furthermore, the Mg isotopic ratios in the second M71 population, combined with their elemental abundances for the light elements, demonstrate that the difference must be the result of adding in the ejecta of intermediate mass AGB stars. Finally we suggest that the low amplitude of the abundance variations of the light elements within M71 is due to a combination of its low mass and its relatively high Fe-metallicity.
description: ApJ, in press
Che strane quelle macchie luminose su Cerere
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Le osservazioni hanno suggerito che la materia di cui sono composte le macchie sia volatile ed evapori grazie al calore della luce solare. Paolo Molaro, OA-Trieste, ci spiega perché sono così particolari
Additional file 2: of Functional characterization of Gh_A08G1120 (GH3.5) gene reveal their significant role in enhancing drought and salt stress tolerance in cotton
Creators: name: Kirungu, Joy
name: Magwanga, Richard
name: Lu, Pu
name: Cai, Xiaoyan
name: Zhou, Zhongli
name: Wang, Xingxing
name: Peng, Renhai
name: Wang, Kunbo
name: Liu, Fang
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics
subject: Chemical Sciences not elsewhere classified
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Table S2. physiochemical properties of the proteins encoded by the cotton GH3 genes. (DOCX 78 kb)
Anomalous Scaling Behavior in Polymer Thin Film Growth by Vapor Deposition
Creators: name: Son, Seung-Woo
name: Ha, Meesoon
name: Jeong, Hawoong
Publisher: name: arXiv
Year: 2008
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: As a first step to understand anomalous kinetic roughening with multifractality in recent experiments of the vapor deposition polymerization (VDP) growth, we study a simple toy model of the VDP growth in a (1+1)-dimensional lattice, along with monomer diffusion, polymer nucleation, limited active end bonding, and shadowing effects. Using extensive numerical simulations, we observe that the global roughness exponent is different from the local one. It is argued that such anomalies in VDP growth are attributed to the instability induced by the nonlocal shadowing effects on active ends of polymers. As varying the ratio of diffusion coefficient to the deposition rate by cosine flux, we also discuss the role of diffusion in kinetic roughening of the polymer thin film growth, which is quite different from that of the metal or semiconductor film growth. Finally, we suggest its (2+1)-dimensional version, which can be directly compared with experimental results.
description: 13 pages, 10 figures (17 eps files)
Il buco nero che sputa rosso
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

A giugno scorso il buco nero chiamato V404 Cygni ha attraversato un periodo di intensa attività. Puntando sulla sorgente lo strumento ULTRACAM montato sul William Herschel Telescope a La Palma, un team internazionale di scienziati ha scoperto che V404 Cygni ha emesso dei lampi di colore rosso, della durata di poche frazioni di secondo. Il commento di Piergiorgio Casella dell’INAF-OAR
Additional file 1: of Use of barbed sutures in robotic bariatric bypass surgery: a single-center case series
Creators: name: Beckmann, Jan
name: Kersebaum, Jan-Niclas
name: SchĂśnfels, Witigo
name: Becker, Thomas
name: Schafmayer, Clemens
name: Egberts, Jan
Publisher: name: figshare
Year: 2019
Subjects: subject: Space Science
subject: Medicine
subject: Physiology
subject: FOS: Biological sciences
subject: Biotechnology
subject: Developmental Biology
subject: Marine Biology
subject: Science Policy
subject: Infectious Diseases
subject: FOS: Health sciences

description: Peri- and postoperative results after using barbed sutures in robotic bariatric bypass surgery. Operative time, robotic time, length of hospital stay, and ideal body weight was calculated as that equivalent to a BMI of 25â kg/m2. Follow-up rate 98%, number of reoperations and complications within the first 30â days according to Clavien-Dindo classification [21]. (DOCX 16 kb)
title: ÐÑÐ»Ð»ÐµÑÐµÐ½Ñ Ð½Ð¾Ð²ÑÑ Ð¿Ð¾ÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ð¹ Ð·Ð° Ð¸ÑÐ»Ñ Ð¸ Ð°Ð²Ð³ÑÑÑ 2021 Ð³Ð¾Ð´Ð°
Creators: 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. ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½ÑÐ¹ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑ
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: 2021
Subjects: Ð±Ð¸Ð±Ð»Ð¸Ð¾Ð³ÑÐ°ÑÐ¸Ñ

description: Ð Ð½Ð°ÑÑÐ¾ÑÑÐ¸Ð¹ Â«ÐÑÐ»Ð»ÐµÑÐµÐ½ÑÂ» Ð²ÐºÐ»ÑÑÐµÐ½Ñ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÑÑÑÑ, Ð¿Ð¾ÑÑÑÐ¿Ð¸Ð²ÑÐ¸Ðµ Ð²Ð¾ Ð²ÑÐµ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾-Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÑÐ½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ° Ð¡ÐÐ±ÐÐ£ Ð² Ð¸ÑÐ»Ðµ Ð¸ Ð°Ð²Ð³ÑÑÑÐµ 2021 Ð³Ð¾Ð´Ð°. Â«ÐÑÐ»Ð»ÐµÑÐµÐ½ÑÂ» ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð·Ð°Ð¿Ð¸ÑÐµÐ¹ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÐºÐ°ÑÐ°Ð»Ð¾Ð³Ð°. ÐÐ°Ð¿Ð¸ÑÐ¸ ÑÐ´ÐµÐ»Ð°Ð½Ñ Ð² ÑÐ¾ÑÐ¼Ð°ÑÐµ RUSMARC Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Â«Ð ÑÑÐ»Ð°Ð½-ÐÐµÐ¾Â». ÐÐ°ÑÐµÑÐ¸Ð°Ð» ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½ Ð² ÑÐ¸ÑÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¼ Ð¿Ð¾ÑÑÐ´ÐºÐµ Ð¿Ð¾ Ð¾ÑÑÐ°ÑÐ»ÑÐ¼ Ð·Ð½Ð°Ð½Ð¸Ñ, Ð²Ð½ÑÑÑÐ¸ ÑÐ°Ð·Ð´ÐµÐ»Ð¾Ð² â Ð² Ð°Ð»ÑÐ°Ð²Ð¸ÑÐµ Ð°Ð²ÑÐ¾ÑÐ¾Ð² Ð¸ Ð·Ð°Ð³Ð»Ð°Ð²Ð¸Ð¹. ÐÐ°Ð¿Ð¸ÑÐ¸ Ð²ÐºÐ»ÑÑÐ°ÑÑ Ð¿Ð¾Ð»Ð½Ð¾Ðµ Ð±Ð¸Ð±Ð»Ð¸Ð¾Ð³ÑÐ°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹, Ð¸Ð½Ð²ÐµÐ½ÑÐ°ÑÐ½ÑÐ¹ Ð½Ð¾Ð¼ÐµÑ Ð¸ Ð½Ð°Ð·Ð²Ð°Ð½Ð¸Ðµ Ð¾ÑÐ´ÐµÐ»Ð° Ð² ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð½Ð¾Ð¼ Ð²Ð¸Ð´Ðµ (ÑÐ¸ÑÑ Ð¾ÑÐ´ÐµÐ»Ð°). Ð¡Ð¿Ð¸ÑÐ¾Ðº ÑÐ¾ÐºÑÐ°ÑÐµÐ½Ð¸Ð¹ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð² Â«ÐÑÐ»Ð»ÐµÑÐµÐ½ÐµÂ». Ð Ð½Ð°ÑÑÐ¾ÑÑÐµÐ¼ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¸ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ñ ÐºÐ½Ð¸Ð³Ð¸, Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ Ð¸ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½ÑÐµ ÑÐµÑÑÑÑÑ â Ð¿Ð¾Ð»Ð½Ð¾ÑÐµÐºÑÑÐ¾Ð²ÑÐµ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÑ, Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½ÑÐµ Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¼ ÐºÐ°ÑÐ°Ð»Ð¾Ð³Ðµ Ð² ÑÐ¾ÑÐ¼Ð°ÑÐ°Ñ pdf Ð¸ html, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÐµÑÐµÑÐµÐ½Ñ Ð¿ÑÐ¸Ð¾Ð±ÑÐµÑÐµÐ½Ð½ÑÑ Ð­ÐÐ¡ Ð¸ Ð´Ð¾ÑÑÑÐ¿Ð½ÑÑ Ð±Ð°Ð· Ð´Ð°Ð½Ð½ÑÑ. ÐÐ»Ñ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÑÑÐ° ÑÐºÐ°Ð·Ð°Ð½ URL-Ð°Ð´ÑÐµÑ. Ð Â«ÐÑÐ»Ð»ÐµÑÐµÐ½ÐµÂ» Ð¾ÑÐ´ÐµÐ»ÑÐ½Ð¾ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ñ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ, Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÐµ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¾Ð¹ Ð² ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¿Ð¾Ð¶ÐµÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ð¹. Ð ÐºÐ¾Ð½ÑÐµ Ð±ÑÐ»Ð»ÐµÑÐµÐ½Ñ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½ ÑÐ¿Ð¸ÑÐ¾Ðº Ð¿ÐµÑÐ¸Ð¾Ð´Ð¸ÑÐµÑÐºÐ¸Ñ Ð¸Ð·Ð´Ð°Ð½Ð¸Ð¹, Ð²ÑÐ¿Ð¸ÑÐ°Ð½Ð½ÑÑ Ð±Ð¸Ð±Ð»Ð¸Ð¾ÑÐµÐºÐ¾Ð¹ Ð½Ð° 2021 Ð³Ð¾Ð´. ÐÐ½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐ¹ Â«ÐÑÐ»Ð»ÐµÑÐµÐ½Ñ Ð½Ð¾Ð²ÑÑ Ð¿Ð¾ÑÑÑÐ¿Ð»ÐµÐ½Ð¸Ð¹Â» Ð²ÑÐ¿ÑÑÐºÐ°ÐµÑÑÑ Ð² ÑÐ»ÐµÐºÑÑÐ¾Ð½Ð½Ð¾Ð¼ Ð²Ð¸Ð´Ðµ. Ð­Ð»ÐµÐºÑÑÐ¾Ð½Ð½Ð°Ñ Ð²ÐµÑÑÐ¸Ñ Ð¾ÑÑÐ°Ð¶ÐµÐ½Ð° Ð½Ð° ÑÐµÑÐ²ÐµÑÐµ Ð¡ÐÐ±ÐÐ£ Ð¿Ð¾ Ð°Ð´ÑÐµÑÑ: http://library.spbstu.ru/ru/.
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÐºÐ°Ð´ÑÐ¾Ð² Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ-Ð­Ð½ÐµÑÐ³Ð¾Â»)
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ÑÐµÐ¼Ð¸Ð½Ð°, ÐÐºÐ°ÑÐµÑ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: 2018
Subjects: Ð¿ÐµÑÑÐ¾Ð½Ð°Ð» Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸
Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÐµ Ð¿ÑÐ¾ÐµÐºÑÑ
Ð¸Ð½Ð¶Ð¸Ð½Ð¸ÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÑÑÐ»ÑÐ³Ð¸
ÑÑÑÐ´Ð¾Ð²ÑÐµ ÑÐµÑÑÑÑÑ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐÐÐ Â«ÐÐ-Ð­Ð½ÐµÑÐ³Ð¾Â». Ð¦ÐµÐ»ÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð¼Ð¼ÐµÑÑÐµÑÐºÐ¾Ð¹ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. 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¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð°ÑÐ¿ÐµÐºÑÐ¾Ð² Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÑÐµÑ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ¾Ð² Ð¿ÑÐ¾ÐµÐºÑÐ° Ð¿Ð¾ Ð¾ÑÐºÑÑÑÐ¸Ñ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÐµÐ½ÑÑÐ¾Ð² Ð¸ Ð¾ÑÑÑÐµÑÑÐ²Ð»ÐµÐ½Ð¸Ðµ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð² ÑÑÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸.
Asymmetric Exclusion Processes with Disorder: Effect of Correlations
Creators: name: Foulaadvand, M. Ebrahim
name: Kolomeisky, Anatoly
name: Teymouri, Hamid
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: Multi-particle dynamics in one-dimensional asymmetric exclusion processes with disorder is investigated theoretically by computational and analytical methods. It is argued that the general phase diagram consists of three non-equilibrium phases that are determined by the dynamic behavior at the entrance, at the exit and at the slowest defect bond in the bulk of the system. Specifically, we consider dynamics of asymmetric exclusion process with two identical defect bonds as a function of distance between them. Two approximate theoretical methods, that treat the system as a sequence of segments with exact description of dynamics inside the segments and neglect correlations between them, are presented. In addition, a numerical iterative procedure for calculating dynamic properties of asymmetric exclusion systems is developed. Our theoretical predictions are compared with extensive Monte Carlo computer simulations. It is shown that correlations play an important role in the particle dynamics. When two defect bonds are far away from each other the strongest correlations are found at these bonds. However, bringing defect bonds closer leads to the shift of correlations to the region between them.
description: 11 pages, 15 eps figures, RevtexIV
The area generating function for simple-2-column polyominoes with hexagonal cells
Creators: name: Feretic, S.
name: Trinajstic, N.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Combinatorics (math.CO)
subject: FOS: Mathematics
subject: 05B50

description: Column-convex polygons were first counted by area several decades ago, and the result was found to be a simple, rational, generating function. In this chapter we generalize that result. Let a p-column polyomino be a polyomino whose columns can have 1, 2,..., p connected components. Then column-convex polygons are equivalent to 1-convex polyominoes. The area generating function of even the simplest generalization, namely to 2-column polyominoes, is unlikely to be solvable. We therefore define a class of polyominoes which interpolates between column-convex polygons and 2-column polyominoes. We derive the area generating function of that class, using an extension of an existing algorithm. The growth constant of the new class is greater than the growth constant of column-convex polygons. A rather tight lower bound on the growth constant complements a compelling numerical analysis.
description: 16 pages, 2 figures
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ ÑÐµÐ»ÑÑÐ¾Ð²Ð¾Ð¹ ÐºÐ¾Ð»ÐµÐ¸ Ð¿Ð¾ Ð²Ð¸Ð´ÐµÐ¾Ð¸Ð·Ð¾Ð±ÑÐ°Ð¶ÐµÐ½Ð¸Ñ
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¸Ð¼Ð¾ÑÐµÐ½ÐºÐ¾, ÐÐ»ÐµÐºÑÐ°Ð½Ð´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: ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð·ÑÐµÐ½Ð¸Ðµ
Ð°Ð²ÑÐ¾Ð¿Ð¸Ð»Ð¾Ñ
Ð¾Ð±Ð½Ð°ÑÑÐ¶ÐµÐ½Ð¸Ðµ Ð¿ÑÐµÐ¿ÑÑÑÑÐ²Ð¸Ð¹
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Ð¿ÑÐµÐ¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¥ÐÐ¤Ð

description: Ð¦ÐµÐ»ÑÑ Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ° ÑÐ²Ð»ÑÐµÑÑÑ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ°
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Evolution of Nuclear Many-Body Forces with the Similarity Renormalization Group
Creators: name: Jurgenson, E. D.
name: Navratil, P.
name: Furnstahl, R. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: The first practical method to evolve many-body nuclear forces to softened form using the Similarity Renormalization Group (SRG) in a harmonic oscillator basis is demonstrated. When applied to He4 calculations, the two- and three-body oscillator matrix elements yield rapid convergence of the ground-state energy with a small net contribution of the induced four-body force.
description: 4 pages, 5 figures, PRL published version
The solution classical and quantum feedback optimal control problem without the Bellman Equation
Creators: name: Foukzon, Jaykov
Publisher: name: arXiv
Year: 2008
Subjects: subject: Data Analysis, Statistics and Probability (physics.data-an)
subject: FOS: Physical sciences

description: A new approach, which is proposed in this paper allows one to construct the Bellman function V(t,x) and optimal control u(t) directly,i.e.,without any reference to the Bellman equation, by way of using strong large deviations principle for the solutions Colombeau-Ito's SDE.
description: 295 pages
title: Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ° ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ ÑÐ±Ð¾ÑÐºÐ¸ Ð¸ ÑÐ²Ð°ÑÐºÐ¸ Ð²Ð°Ð»Ð° ÑÐ¾ÑÐ¾ÑÐ° ÑÑÑÐ±Ð¸Ð½Ñ Ð´Ð»Ñ ÐÐ­Ð¡ Ð±Ð¾Ð»ÑÑÐ¾Ð¹ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð ÑÐ±ÑÐ¾Ð², ÐÐ°Ð²ÐµÐ»
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Ð¾ÑÐ¾Ñ
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description: ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. Ð¡ÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, ÑÑÐµÐ±ÑÑÑÐ¸Ðµ ÑÐµÑÐµÐ½Ð¸Ñ Ð² Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¼ Ð¿ÑÐ¾ÐµÐºÑÐµ. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½Ð¾Ðµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½Ð° ÑÐµÐ¼Ñ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð½Ð°Ñ ÑÐ²Ð°ÑÐºÐ° Ð² Ð·Ð°ÑÐ¸ÑÐ½ÑÑ Ð³Ð°Ð·Ð°Ñ Ð¸ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ²Ð°ÑÐºÐ° Ð¿Ð¾Ð´ ÑÐ»Ð¾ÐµÐ¼ ÑÐ»ÑÑÐ° Ð² Ð¼Ð°ÑÐ¸Ð½Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸Ð¸. ÐÑÐ±ÑÐ°Ð½ Ð¸ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð½ÑÐ¹ ÑÐ¿Ð¾ÑÐ¾Ð± ÑÐ²Ð°ÑÐºÐ¸. ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÑÐµÐ¼Ð° ÑÐ±Ð¾ÑÐºÐ¸ Ð¸ ÑÐ²Ð°ÑÐºÐ¸ ÑÐ¾ÑÐ¾ÑÐ°. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐ°ÑÑÐµÑÐ½Ð¾Ðµ Ð¸ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ°Ð»ÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²ÑÐ±Ð¾ÑÐ° ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÑ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð¸ ÑÐµÐ¶Ð¸Ð¼Ð¾Ð² Ð´Ð»Ñ Ð°Ð²ÑÐ¾Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ²Ð°ÑÐºÐ¸. ÐÑÐ±ÑÐ°Ð½ ÑÐ²Ð°ÑÐ¾ÑÐ½ÑÐ¹ ÑÑÐµÐ½Ð´ Ð´Ð»Ñ ÑÐ²Ð°ÑÐºÐ¸, ÑÐ²Ð°ÑÐ¾ÑÐ½Ð¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. ÐÐ¾Ð´ÑÐ²ÐµÑÐ¶Ð´ÐµÐ½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ ÑÐµÐ»ÐµÑÐ¾Ð¾Ð±ÑÐ°Ð·Ð½Ð¾ÑÑÑ Ð´Ð°Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¿Ð¾ÑÐ¾Ð±Ð° ÑÐ²Ð°ÑÐºÐ¸.
The HotQCD Equation of State
Creators: name: Soltz, R. A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Lattice (hep-lat)
subject: FOS: Physical sciences

description: We present results from recent calculations of the QCD equation of state by the HotQCD Collaboration and review the implications for hydrodynamic modeling. The equation of state of QCD at zero baryon density was calculated on a lattice of dimensions $32^3 \times 8$ with $m_l = 0.1 m_s$ (corresponding to a pion mass of $\sim$220 MeV) using two improved staggered fermion actions, p4 and asqtad. C alculations were performed along lines of constant physics using more than 100M cpu-hours on BG/L supercomputers at LLNL, NYBlue, and SDSC. We present paramete rizations of the equation of state suitable for input into hydrodynamics models of heavy ion collisions.
description: 4 pages, 5 figures - to appear in the conference proceedings for Quark Matter 2009, March 30 - April 4, Knoxville, Tennessee
New DELPHI Results from Semileptonic b, c Decays
Creators: name: Margoni, Martino
Publisher: name: INFN Open Access Repository
Year: 1999

description: The inclusive direct and cascade semileptonic branching ratios of the b quark
were measured from a fit to the lepton momentum spectrum in the B-hadron rest
frame, exploiting the charge correlation between the lepton and the heavy
meson. The value of the Vcb element in the CKM quark mixing matrix was computed
from the differential decay width of the process B0--> D+-* l- nu, measured as
a function of the product W of the B and D* 4-velocities, using an inclusive
method of D* reconstruction. A measurement of the ratio Vub/Vcb has been
obtained by using the reconstructed secondary hadronic mass in semileptonic
decays of B hadrons. The charm semileptonic branching ratio was measured using
a double tag method based on the detection of exclusively reconstructed D
mesons accompanied by a lepton in the opposite hemisphere.
Meteoriti: una cascata di diamanti
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Si chiama lonsdaleite ed è una forma esagonale di diamante che si genera esclusivamente durante eventi estremi come la caduta di un meteorite a Terra. Lo dice uno studio appena pubblicato su Nature Communication che dei diamanti vuole fare veri e propri “marker” da impatto cosmico
Energy decay for solutions of the wave equation with general memory boundary conditions
Creators: name: Cornilleau, Pierre
name: Nicaise, Serge
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optimization and Control (math.OC)
subject: FOS: Mathematics

description: We consider the wave equation in a smooth domain subject to Dirichlet boundary conditions on one part of the boundary and dissipative boundary conditions of memory-delay type on the remainder part of the boundary, where a general borelian measure is involved. Under quite weak assumptions on this measure, using the multiplier method and a standard integral inequality we show the exponential stability of the system. Some examples of measures satisfying our hypotheses are given, recovering and extending some of the results from the literature.
description: 14 pages, submitted to Diff. Int. Equ
Come ti piego un’onda a mille GHz
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2016

Uno studio appena uscito su Nature Scientific Reports illustra un dispositivo dielettrico in grado di focalizzare onde con frequenze comprese fra i 100 e i 10 mila GHz. Francesco Cuttaia (INAF): «Aprono l’orizzonte a innumerevoli applicazioni in campo astrofisico e tecnologico»
Temporal and Interview Consistent Error Concealment Technique for Multiview Plus Depth Video
Creators: name: Khattak, Shadan
name: Hamzaoui, Raouf
name: Frossard, Pascal
name: Maugey, Thomas
Publisher: name: figshare
Year: 2023
Subjects: Video processing
Image and video coding

description: Multiview plus depth (MVD) is an emerging video format with many applications, including 3-D television and free viewpoint television. During the broadcast of a compressed MVD video, transmission errors may cause the loss of whole frames, resulting in significant degradation of video quality. Error concealment techniques have been widely used to deal with transmission errors in video communication. However, the existing solutions do not address the requirement that the reconstructed frames should be consistent with neighboring frames, i.e., corresponding pixels should have consistent color information. We propose a new consistency model for error concealment of MVD video that allows one to maintain a high level of consistency between frames of the same view (temporal consistency) and those of neighboring views (inter-view consistency). We then propose an algorithm that uses our model to implement concealment in a consistent way. Simulations with the reference software for the multiview video coding project of the joint video team of the ISO/IEC MPEG and ITU-T VCEG show that our method outperforms benchmark techniques, including a baseline approach based on the boundary matching algorithm, with respect to both reconstruction quality and view consistency.
Marte, stiamo arrivando!
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2016

Lancio e manovre da manuale per la missione ExoMars: la sonda europea ha iniziato al meglio il suo viaggio verso Marte. Nicolò D'Amico, presidente INAF: «C’è molto INAF in questa missione, e sono convinto che le nostre ricercatrici e i nostri ricercatori saranno protagonisti e potranno svelare alcuni dei segreti che il Pianeta rosso ancora conserva»
Future projects on atmospheric neutrinos
Creators: name: T. Tabarelli De Fatis
Publisher: name: INFN Open Access Repository
Year: 2002

description: New results from Super-Kamiokande, K2K and SNO not only have spurred on the
interest in neutrino oscillation physics, but also have started to shift the
interest from discovery to precision measurements. Future projects focusing on
atmospheric neutrinos are reviewed in this context. Important contributions
could be made in the precision determination of the oscillation parameters, in
the observation of matter effects and in the determination of the neutrino mass
hierarchy. Unfortunately, the probability that the projects discussed in this
review will be running in the next ten years is rather small. The only project
with a shorter time scale has not been funded.
Queueing process with excluded-volume effect
Creators: name: Arita, Chikashi
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: FOS: Physical sciences

description: We introduce an extension of the M/M/1 queueing process with a spatial structure and excluded- volume effect. The rule of particle hopping is the same as for the totally asymmetric simple exclusion process (TASEP). A stationary-state solution is constructed in a slightly arranged matrix product form of the open TASEP. We obtain the critical line that separates the parameter space depending on whether the model has the stationary state. We calculate the average length of the model and the number of particles and show the monotonicity of the probability of the length in the stationary state. We also consider a generalization of the model with backward hopping of particles allowed and an alternate joined system of the M/M/1 queueing process and the open TASEP.
description: 9 figures
title: Ð¢Ð¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÐºÐ¾ÑÑÑÐ¼Ð½ÑÑ ÐºÐ°Ð¼Ð²Ð¾Ð»ÑÐ½ÑÑ ÑÐµÑÑÑÑÐ½ÑÑ ÑÐºÐ°Ð½ÐµÐ¹ Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹
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ÑÑÑÐ°Ð½Ð¸, ÐÐ¾Ð»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: 2018
Subjects: ÑÐµÑÑÑÑÐ½ÑÐµ ÑÐºÐ°Ð½Ð¸
ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ Ñ Ð°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°
ÐºÐ¾ÑÑÑÐ¼Ð½ÑÐµ ÑÐºÐ°Ð½Ð¸
ÐºÐ°Ð¼Ð²Ð¾Ð»ÑÐ½ÑÐµ ÑÐºÐ°Ð½Ð¸

description: Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð±ÑÐµÐºÑÐ° Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð»Ñ Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ Ð²ÑÐ±ÑÐ°Ð½Ñ ÐºÐ¾ÑÑÑÐ¼Ð½ÑÐµ ÐºÐ°Ð¼Ð²Ð¾Ð»ÑÐ½ÑÐµ ÑÐµÑÑÑÑÐ½ÑÐµ ÑÐºÐ°Ð½Ð¸ Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ñ Ð¸ Ð·Ð°ÑÑÐ±ÐµÐ¶Ð½ÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´Ð¸ÑÐµÐ»ÐµÐ¹. Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ â ÑÐ¾Ð²Ð°ÑÐ¾Ð²ÐµÐ´Ð½Ð°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð¸ ÑÐºÑÐ¿ÐµÑÑÐ¸Ð·Ð° ÐºÐ°ÑÐµÑÑÐ²Ð° ÐºÐ¾ÑÑÑÐ¼Ð½ÑÑ ÐºÐ°Ð¼Ð²Ð¾Ð»ÑÐ½ÑÑ ÑÐµÑÑÑÑÐ½ÑÑ ÑÐºÐ°Ð½ÐµÐ¹ Ð²ÐµÐ´Ð¾Ð¼ÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ.
Ultime da ExoMars: è vivo e comunica
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Ricevuto dalla base dell'Agenzia Spaziale Italiana a Malindi l'attesissimo segnale radio dalla sonda in volo verso Marte. Pannelli solari aperti, batterie in carica, tutto procede come previsto
Neutrino Physics and Astrophysics with the MACRO Experiment at the Gran
  Sasso Lab
Creators: name: G. Giacomelli
name: For The MACRO Collaboration
Publisher: name: Braz.J.Phys. 33 (2003) 211-217
Year: 2003

description: The results of the MACRO experiment on atmospheric neutrino oscillations are
presented and discussed. The data concern different event topologies with
average neutrino energies of ~ 4 and ~ 50 GeV. The Multiple Coulomb Scattering
of muons in the MACRO absorbers was used to estimate the neutrino energy of
each event of the higher energy sample. The angular distributions, the absolute
fluxes and the L/E distribution favour nu_mu  nu_tau oscillations with
maximal mixing and Delta m^2=0.0025 eV^2. Results are presented on the searches
for astrophysical sources of high energy muon neutrinos, for bursts of electron
antineutrinos from stellar gravitational collapses and on indirect searches for
WIMPs from the Earth and from the Sun.
Ore 10:31, ExoMars è in volo
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Il possente lanciatore Proton-M è decollato dalla rampa di lancio del cosmodromo di Baikonur, e sta conducendo in questi minuti la prima delle due navicelle del Programma ExoMars verso il Pianeta Rosso. Media INAF ha dedicato a questa missione, a forte presenza italiana, una ricca serie di articoli, interviste, immagini e video
Metal - Insulator transition in Fe1.01-xCuxSe
Creators: name: Williams, A J
name: McQueen, T M
name: Ksenofontov, V
name: Felser, C
name: Cava, R J
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Iron Selenide, Fe1.01Se, the layered parent compound of the recently discovered superconducting arsenide family, has previously been shown to be non magnetic and superconducting with a critical temperature of 8 K. Here we show that copper can be substituted at the iron site in Fe1.01Se up to a solubility limit of 20-30 %, after which a first order transition to the three-dimensional CuFeSe2 structure type is observed. As little as 1.5 % percent copper is sufficient to suppress the superconductivity, and 4 % drives the system through a metal-insulator transition. A local magnetic moment is introduced, which maximizes near 12% doping, where a spin-glass transition near 15 K is observed.
Marte: l’invasione robot
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

Sono 5 le sonde in orbita attorno al Pianeta Rosso, 6 con ExoMars in arrivo. Ma fra rover, lander, strumenti e archibugi HiTech l'invasione pacifica di tecnologia umana sulle lande marziane racconta una storia lunga 50 anni: con Media INAF abbiamo realizzato un'infografica che raccoglie tutte le missioni ammartate e gli orbiter attualmente attivi
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐµÑÐ½Ð° Heineken N.V.)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐµÐ»Ð¸ÐºÑÐ½, ÐÐ°ÑÐ³Ð°ÑÐ¸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: 2017
Subjects: ÐÐ½ÑÐµÑÐ½ÐµÑ
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ ÐºÐ¾Ð½ÑÐµÑÐ½ Heineken N. V.
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ÐºÐ¾ÑÐ¿Ð¾ÑÐ°ÑÐ¸Ð²Ð½ÑÐµ ÑÐ°Ð¹ÑÑ

description: Ð Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð½Ð° ÑÐµÐ¼Ñ Â«ÐÐ½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ ÐºÐ°Ðº Ð¸Ð½ÑÑÑÑÐ¼ÐµÐ½ÑÐ° ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ PR-Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð½ÑÐµÑÐ½Ð° Heineken N.V.Â» Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°Ð½Ð°Ð»Ð¸Ð·Ð° Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¹ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð² ÑÑÐµÑÐµ PR. ÐÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ PR-ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼Ð¸ Ð² ÑÐµÑÐ¸ ÐÐ½ÑÐµÑÐ½ÐµÑ. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ñ ÑÑÐ¸Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ PR-ÑÐ¿ÐµÑÐ¸Ð°Ð»Ð¸ÑÑÐ°Ð¼Ð¸ ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Heineken N.V. Ð Ð·Ð°ÐºÐ»ÑÑÐµÐ½Ð¸Ð¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ñ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ ÑÐ»ÑÑÑÐµÐ½Ð¸Ñ ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÑ Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð² ÑÑÐµÑÐµ PR Ð´Ð»Ñ Ð²ÑÐ±ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ°Ð·Ð´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Heineken N.V.