cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
The relative effectiveness of interval circuit training compared with three other methods of fitness training in a school physical education programme
Creators: name: Banister, Eric W.
Publisher: name: University of British Columbia
Year: 2012

description: Much controversy exists regarding the most efficient means of applying methods of progressive resistance work in training routines. The contrasting principles of isometric and isotonic exercise have added further confusion to the area, This study combines different forms of endurance and dynamic strength training in an easily administered form which can be used in a school physical education programme. It compares this method, called here. Interval Circuit Training, with three other types of training to determine which of these methods could be used best in a school. Four groups of fourteen to sixteen year old boys were matched initially on the basis of their scores on three indices; The Harvard Step Test Index, Larson's Strength Index, McCloys Classification Index. The first two of these indices namely endurance and strength were combined to give a Total Fitness Factor. The initial scores of the boys on each of these same tests also gave measures of what have been called The Endurance Factor and The Dynamic Strength Factor respectively. The boys took park in four different training programmes. One group did Interval Circuit Training emphasising endurance and strength training, one group conventional Circuit Training combined with endurance running, another group conventional Circuit Training followed by games activity and the final group had a total Activity programme. They took part in the different training methods once every eight days for a period of two months by which time eight training sessions had been completed. During the rest of their weekly programme all the groups followed a similar programme of athletics and gymnastics and there was no specific weight training or endurance running performed by any of the groups during this time. After two months the groups were re-tested and the respective fitness indices calculated. The differences of mean gains occurring between the groups from test to re-test were compared. The Interval Circuit Training Group showed gains in total fitness over the Circuit Training Activity group and the Games Activity group at the level of significance chosen (0.1). Also no significant gains were made by any of the other groups over each other in any of the factors tested at the 10 per cent level of confidence. Gains in the scores were made from test to re-test by all the groups on all the factors. The largest gains were made by the Interval Circuit Training group and these gains were particularly evident in the strength factor.
Additional file 6 of UGRP1-modulated MARCO+ alveolar macrophages contribute to age-related lung fibrosis
Creators: name: Chen, Yongyan
name: Hao, Xiaolei
name: Li, Ming
name: Tian, Zhigang
name: Cheng, Min
Publisher: name: figshare
Year: 2023
Subjects: subject: Biochemistry
subject: Medicine
subject: Cell Biology
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Physiology
subject: Immunology
subject: FOS: Clinical medicine
subject: Biological Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Infectious Diseases
subject: FOS: Health sciences

description: Additional file 6: Figure 5. Treatment of UGRP1 protein aggravated the BLM-induced pulmonaryfibrosis of the young mice.
title: ÐÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½Ð¾Ðµ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ðµ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ»ÐºÐ°
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: Ð¿ÑÐ¾ÐµÐºÑ Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ½ÐºÑÐ°
Ð´ÑÐµÐ½Ð°Ð¶Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ
ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð´ÑÐµÐ½Ð°Ð¶Ð°
Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½Ð°Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²ÐºÐ°
Ð»Ð¸Ð²Ð½ÐµÐ²Ð°Ñ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ñ

description: Ð Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½ Ð¿ÑÐ¾ÐµÐºÑ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð³Ð¾ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¼Ð°Ð»Ð¾Ð³Ð¾ Ð½Ð°ÑÐµÐ»ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿ÑÐ½ÐºÑÐ°, ÑÐ°ÑÐ¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð² ÐÐµÐ½Ð¸Ð½Ð³ÑÐ°Ð´ÑÐºÐ¾Ð¹ Ð¾Ð±Ð»Ð°ÑÑÐ¸. ÐÑÐ¾ÐµÐºÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð² ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²Ð¸Ð¸ Ñ Ð·Ð°Ð´Ð°Ð½Ð¸ÐµÐ¼ Ð½Ð° Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð´ÐµÐ¹ÑÑÐ²ÑÑÑÐ¸Ð¼Ð¸ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½ÑÐ¼Ð¸ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°Ð¼Ð¸. Ð Ð¿ÑÐ¾ÐµÐºÑÐµ Ð±ÑÐ»Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ: Ð²ÐµÑÑÐ¸ÐºÐ°Ð»ÑÐ½Ð°Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²ÐºÐ° ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ»ÐºÐ°; Ð¿ÑÐ¾ÐµÐºÑ Ð»Ð¸Ð²Ð½ÐµÐ²Ð¾Ð¹ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð´Ð»Ñ Ð¾ÑÐ²Ð¾Ð´Ð° Ð²Ð¾Ð´ Ñ ÑÐ»Ð¸Ñ, Ð¶Ð¸Ð»ÑÑ ÑÑÐ°ÑÑÐºÐ¾Ð² Ð¸ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½ÑÑ Ð·Ð¾Ð½; ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð² Ð»Ð¸Ð²Ð½ÐµÐ²Ð¾Ð¹ ÐºÐ°Ð½Ð°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸; Ð¿ÑÐ¾ÐµÐºÑ Ð´ÑÐµÐ½Ð°Ð¶Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ñ Ð´ÑÐµÐ½Ð°Ð¶ÐµÐ¹; Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÑÐ°Ð½Ð¸ÑÐ°ÑÐ½Ð¾Ð¹ Ð¾ÑÐ¸ÑÑÐºÐµ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸.
AREAS OF INCREASING NEED FOR INFORMATION TECHNOLOGIES  IN RECENT YEARS
Creators: name: Mansurov Umidjon, Abdullayev Ilhom Khojayorovich Uzbekistan-Finland Pedagogical Institute
Publisher: name: Zenodo
Year: 2024

description: . In the modern world, information technology plays a leading role in changing the professional environment. Information technology, which has penetrated every field, is changing the way of work, communication methods, and process management. This article covers a major trend in the use of information technology in the workplace and its impact on the professional landscape.

Keywords: information, technology, cyber security, artificial intelligence
Atmospheric neutrino oscillations with the MACRO detector
Creators: name: M. Giorgini
name: For The MACRO Coll
Publisher: name: INFN Open Access Repository
Year: 2002

description: After a short overview of the MACRO detector, located at the Gran Sasso
Laboratory, I shall present and discuss the results on atmospheric muon
neutrino oscillations, concerning low ( ~ 4 GeV) and high ( ~ 50
GeV) energy data. Using the Multiple Coulomb Scattering of muons inside the
lower part of the detector, estimates of the neutrino energy were made event by
event for the high energy sample. The data on angular distributions, absolute
flux and L/E_nu distribution favor nu_mu  nu_tau oscillations with maximal
mixing and Delta m^2=2.5 x 10^-3 eV^2.
Meridiani Planum si prepara per Schiaparelli
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Scopriamo con Simone De Angelis, ricercatore presso l'INAF IAPS Roma, cosa ha di particolare questo sito: la conformazione planare del territorio assicurerà un safety landing all'EDM. In più è ben noto ai ricercatori
Nonlinear hopping transport in ring systems and open channels
Creators: name: Einax, Mario
name: Koerner, Martin
name: Maass, Philipp
name: Nitzan, Abraham
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We study the nonlinear hopping transport in one-dimensional rings and open channels. Analytical results are derived for the stationary current response to a constant bias without assuming any specific coupling to the external fields. It is shown that anomalous large effective jump lengths, as observed in recent experiments by taking the ratio of the third order nonlinear and the linear conductivity, can occur already in ordered systems. Rectification effects due to site energy disorder in ring systems are expected to become irrelevant for large system sizes. In open channels in contrast, rectification effects occur already for disorder in the jump barriers and do not vanish in the thermodynamic limit. Numerical solutions for a sinusoidal bias show that the ring system provides a good description for the transport behavior in the open channel for intermediate and high frequencies. For low frequencies temporal variations in the mean particle number have to be taken into account in the open channel, which cannot be captured in the more simple ring model.
description: 25 pages, 7 figures
I have a DREAMS
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2016

A bordo di ExoMars, protetto dalla robusta "armatura" del lander Schiaparelli, ecco lo strumento DREAMS: una suite di sensori per la misura dei parametri meteorologici e del campo elettrico atmosferico in prossimità della superficie di Marte. Lo osserviamo da vicino grazie all'infografica che MediaINAF ha realizzato in occasione del lancio della missione ESA
Neutrino Astronomy with ANTARES
Creators: name: Montaruli, Teresa
name: For The ANTARES Collaboration
Publisher: name: Acta Phys.Polon. B36 (2005) 509-518
Year: 2004

description: ANTARES is a project aiming at the operation of an underwater detector at a
depth of 2.5 km close to Toulon in the South of France. The detector is
expected to be completed at the beginning of 2007. The main purpose of the
experiment is the detection of high energy neutrinos produced in astrophysical
sources. Being weakly interacting, neutrinos could potentially be more powerful
messengers of the universe compared to photons, but their detection is
challenging. The technique employs phototubes to detect the arrival time and
the amplitude of photons emitted by neutrino charged secondaries due to the
Cherenkov effect. ANTARES will contribute significantly in the field of
neutrino astronomy, observing the Galactic Centre with unprecedented pointing
capabilities.
Un italiano alla guida di ExoMars nel team ESA
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2016

Quali le attese per ExoMars? Ma soprattutto: quali le insidie maggiori che dovrà affrontare il team di ingegneri e tecnici della missione? Media INAF lo ha chiesto a Giacinto Gianfiglio, membro dell’ExoMars Project Team dell’ESA con l’incarico di System and Orbiter Manager
Conto alla rovescia per DREAMS
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

A bordo della prima spedizione ExoMars, in partenza per Marte tra pochi giorni, c’è anche DREAMS, una stazione meteorologica pensata per studiare nel dettaglio le condizioni atmosferiche presenti sul suolo marziano. La PI dello strumento è Francesca Esposito dell’INAF - Osservatorio Astronomico di Capodimonte
title: “Nobody's ever asked me what it's like”: The role of family networks in the transitions of injured soldiers engaging with higher education.
Creators: name: Lambert-Heggs, Wendy
Publisher: name: University of Plymouth
Year: 2016
Subjects: subject: Networks of Intimacy
subject: Transitions to Higher Education
subject: Injured service personnel
subject: Military Service
subject: Other (e.g., MD, EdD, DBA, DClinPsy)

description: An increasing number of injured service personnel returning from active combat duty will not be redeployed and many of them face discharge from military service. A number of these men and women have sustained life-threatening injuries which may, if the individual survives, result in reduced physical and mental health functioning. This research is focused on the transitions and processes that injured personnel go through when contemplating a new career through engagement with a higher education programme of study. An in-depth qualitative case study of networks of intimacy was used, an approach developed by Heath and Fuller (2007) to explore how, and in what ways, decisions are made within networks of family/significant others. In this case study it was with regard to transitions from a military to civilian culture, where traumatic life-changing events had impacted on the men and their families. As Johnson et al (2008:20) believe, in the case of educational decision-making, it is co-constructed within social networks and interviewing multiple networks facilitates our understanding 'beyond the individual'. The research found that, by supporting their injured ex-combatants (IECs) in complex and difficult transitions, the family network also had to address their own social identities, established attachments and kinship routines and adjust to new ways of thinking and feeling. However whilst the family network is seen as a vital component in the 'operational effectiveness' for transitional readjustment, the Armed Forces Covenant , which states that supporting IECs is ‘an obligation for life’ (Ministry of Defence 2011:8), does not acknowledge that this obligation falls overwhelmingly on the IECs’ families, particularly the wives who receive little support. In both the United Kingdom (UK) and United States (US) there is an absence of research that considers how family and social networks influence transitions into civilian life and especially decisions to undertake higher education programmes. The thesis explores how widening participation policies can be implemented more successfully to support IECs and their families, and how higher education institutions in the UK should improve staff training to raise awareness and understanding of the uniquely special needs that IECs have as a result of their injuries and military experiences.
Constraints for weakly interacting light bosons from existence of massive neutron stars
Creators: name: Krivoruchenko, M. I.
name: Simkovic, F.
name: Faessler, Amand
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Theories beyond the standard model include a number of new particles some of which might be light and weakly coupled to ordinary matter. Such particles affect equation of state of nuclear matter and can shift admissible masses of neutron stars to higher values. The internal structure of neutron stars is modified provided the ratio between coupling strength and mass squared of a weakly interacting light boson is above $g^2/μ^2 \sim 25 ~\mathrm{GeV}^{-2}$. We provide limits on the couplings with the strange sector, which cannot be achieved from laboratory experiments analysis. When the couplings to the first family of quarks is considered the limits imposed by the neutron stars are not more stringent than the existing laboratory ones. The observations on neutron stars give evidence that equation of state of the $β$-equilibrated nuclear matter is stiffer than expected from many-body theory of nuclei and nuclear matter. A weakly interacting light vector boson coupled predominantly to the second family of the quarks can produce the required stiffening.
description: 5 pages REVTeX, 2 pdf figures
LVD highlights
Creators: name: Selvi, Marco
name: For The LVD Collaboration
Publisher: name: INFN Open Access Repository
Year: 2006

description: The Large Volume Detector (LVD) in the INFN Gran Sasso National Laboratory,
Italy, is a $\nu$ observatory mainly designed to study low energy neutrinos
from the gravitational collapse of galactic objects. The experiment has been
monitoring the Galaxy since June 1992, under increasing larger configurations:
in January 2001 it has reached its final active mass M=1 kt. LVD is one of the
largest liquid scintillator apparatus in the world for the detection of stellar
collapses and, besides SNO, SuperKamiokande and Amanda, it is a charter member
of the SNEWS network, that has become fully operational since July 1st, 2005.
No gravitational core-collapse has been detected by LVD during 14 years of data
acquisition; this allows to put an upper limit of 0.18 events y$^{-1}$ in our
galaxy at the 90% C.L. The LVD tracking system allows the detection and the
recontruction of the cosmic muon tracks in a large fraction of the whole solid
angle, in particular also horizontal tracks can be reconstructed. The results
of the muon depth--intensity relation and of the flux of neutrino--induced
muons are presented. Moreover, during 2006, the CNGS beam will start its
operation: the performances of LVD as a beam monitor are described.
title: ÐÐµÑÐ¾Ð´ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð² Ð·Ð°Ð´Ð°ÑÐ°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÐ¾Ð½ÐºÐ¾ÑÑÐµÐ½Ð½ÑÑ ÑÑÐµÑÐ¶Ð½ÐµÐ¹
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¸Ð½Ð¾Ð², ÐÐ°Ð´Ð¸Ð¼
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¡ÑÐµÑÐ¶Ð½Ð¸ ÑÐ¾Ð½ÐºÐ¾ÑÑÐµÐ½Ð½ÑÐµ
ÐÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´
Ð¿Ð¾Ð»ÑÑÐ´Ð²Ð¸Ð³Ð¾Ð²Ð°Ñ ÑÐµÐ¾ÑÐ¸Ñ
Ð¿Ð¾ÑÐµÑÑ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸
ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð½Ð°Ð³ÑÑÐ·ÐºÐ°
Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð°ÑÑÐ¸ÑÐ° Ð¶ÐµÑÑÐºÐ¾ÑÑÐ¸

description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð° ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð² Ð´Ð»Ñ ÑÐµÑÐµÐ½Ð¸Ñ Ð·Ð°Ð´Ð°Ñ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ ÑÐ¾Ð½ÐºÐ¾ÑÑÐµÐ½Ð½ÑÑ ÑÑÐµÑÐ¶Ð½ÐµÐ¹ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð¿Ð¾Ð»ÑÑÐ´Ð²Ð¸Ð³Ð¾Ð²Ð¾Ð¹ ÑÐµÐ¾ÑÐ¸Ð¸ Ð. Ð. Ð¡Ð»Ð¸Ð²ÐºÐµÑÐ°. Ð­ÑÐ° ÑÐµÐ¾ÑÐ¸Ñ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ ÐµÐ´Ð¸Ð½ÑÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼ ÑÐµÑÐ°ÑÑ Ð·Ð°Ð´Ð°ÑÐ¸ ÐºÐ°Ðº Ð´Ð»Ñ ÑÑÐµÑÐ¶Ð½ÐµÐ¹ Ð¾ÑÐºÑÑÑÐ¾Ð³Ð¾, ÑÐ°Ðº Ð¸ Ð·Ð°Ð¼ÐºÐ½ÑÑÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐ¸Ð»ÐµÐ¹. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ñ Ð³ÐµÐ¾Ð¼ÐµÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¼Ð°ÑÑÐ¸ÑÑ Ð¶ÐµÑÑÐºÐ¾ÑÑÐ¸ ÐºÐ¾Ð½ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ° Ñ Ð´Ð²ÑÐ¼Ñ Ð¶ÐµÑÑÐºÐ¸Ð¼Ð¸ ÑÐ·Ð»Ð°Ð¼Ð¸ (ÑÐµÑÑÑ ÑÑÐµÐ¿ÐµÐ½ÐµÐ¹ ÑÐ²Ð¾Ð±Ð¾Ð´Ñ Ð² ÐºÐ°Ð¶Ð´Ð¾Ð¼ ÑÐ·Ð»Ðµ) Ð¸ Ð´Ð»Ñ Ð¿ÑÑÐ¸ ÑÐ»ÑÑÐ°ÐµÐ², ÐºÐ¾Ð³Ð´Ð° Ð² Ð¾Ð´Ð½Ð¾Ð¼ Ð¸Ð· ÑÐ·Ð»Ð¾Ð² ÐºÐ¾Ð½ÐµÑÐ½Ð¾Ð³Ð¾ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ° ÑÐ°ÑÐ¿Ð¾Ð»Ð°Ð³Ð°ÑÑÑÑ ÑÐ°ÑÐ½Ð¸ÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð½ÑÑ Ð¼Ð°ÑÑÐ¸Ñ, Ð´Ð»Ñ ÑÐµÐ³Ð¾ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸ Ð±ÑÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ ÑÐ¾ÑÐ¼Ñ Ð¿Ð¾ÑÐµÑÐ¸ ÑÑÑÐ¾Ð¹ÑÐ¸Ð²Ð¾ÑÑÐ¸ Ð¸ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ñ ÐºÑÐ¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¸Ð», Ð¸Ñ Ð²ÑÐ·ÑÐ²Ð°ÑÑÐ¸Ðµ. ÐÐ°ÑÐµÐ¼ ÑÐ¾ Ð¶Ðµ ÑÐ°Ð¼Ð¾Ðµ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ð¾ Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ ÐºÐ¾Ð½ÐµÑÐ½ÑÑ ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ¾Ð². ÐÐ¾Ð»ÑÑÐµÐ½Ð° ÑÐ¾ÑÐ¾ÑÐ°Ñ ÑÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÑ Ð¼ÐµÐ¶Ð´Ñ ÑÐ¸ÑÐ»ÐµÐ½Ð½ÑÐ¼ Ð¸ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼Ð¸.
Radiatively Corrected Bound on the Light Higgs Mass in a Minimal Non
  Minimal Supersymmetric Standard Model
Creators: name: D. Comelli
Publisher: name: INFN Open Access Repository
Year: 1992

description: The neutral Higgs sector of the Minimal non Minimal Supersymmetric Standard
Model is considered. By effective potential and R.G.E. supported method; an
upper bound of the lightest Higgs is analysed. From the request of
perturbativity of the coupling in the superpotential, adding the leading stop
top contributions, the absolute bound of $\sim 130$ GeV for $90 GeV < m_t< 180
GeV$ and $M_{\tilde{t}} \simeq 1000 $ GeV is derived. The interesting
dependence on $m_t$ for $\tan{\beta} \to 1$ is discussed .
title: Ð¡Ð¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð½Ð° ÑÑÐ½ÐºÐµ ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÑÐ»ÑÐ³
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ÑÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
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¢ÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¸
ÑÑÐ½Ð¾Ðº
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ
ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ Ð°Ð½Ð°Ð»Ð¸Ð·

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð³Ð¾ Ð¸ Ð Ð¾ÑÑÐ¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÑÐ½ÐºÐ° ÑÐµÐ»ÐµÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¹. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÐµ ÑÑÑÐ°ÑÐµÐ³Ð¸Ð¸ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ ÐÐ¢Ð¡. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ ÐÐ¢Ð¡. ÐÑÑÐ²Ð»ÐµÐ½Ð¾ ÑÐµÐºÑÑÐµÐµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²ÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ð¹ Ð´Ð»Ñ Ð¿ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ ÐÐÐ ÐÐ¢Ð¡.
Il tempismo dei buchi neri in rotazione
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Un team internazionale di scienziati aveva previsto che OJ 287, uno dei buchi neri più massicci dell’Universo, avrebbe emesso un lampo di luce ottica verso la fine di novembre 2015. La campagna di osservazioni pianificate ha confermato le loro previsioni. I risultati sono molto promettenti per la ricerca di sorgenti di onde gravitazionali. Il commento di Guido Risaliti dell'Osservatorio Astrofisico di Arcetri dell'INAF
title: ÐÐ½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ´Ð°ÑÐ½ÑÐ¹ ÑÑÐµÐ½Ð´ Ð¡ÐÐ£1200
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ°ÑÐ¸Ð»ÑÐµÐ², ÐÐ»ÐµÐºÑÐµÐ¹
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Ð½ÐµÐ²Ð¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ
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Modification of the Equivalent Photon Approximation for Resolved Photon
  Processes
Creators: name: Drees, Manuel
name: Godbole, Rohini M.
Publisher: name: INFN Open Access Repository
Year: 1995

description: We propose a modification of the equivalent photon approximation (EPA) for
processes which involve the parton content of the photon, to take into account
the suppression of the photonic parton fluxes due to the virtuality of the
photon. We present simple, physically motivated ans\"atze to model this
suppression and show that even though the parton content of the electron no
longer factorizes into an electron flux function and a photon structure
function, it is still possible to express it as a single integral. We also show
that for the TRISTAN experiments its effect can be numerically of the same size
as that of the NLO corrections. Further, we discuss a possible measurement at
HERA, which can provide an experimental handle on the effect we model through
our ans\"atze.
Unitarity of spin-2 theories with linearized Weyl symmetry in $D=2+1$
Creators: name: Dalmazi, D.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: Here we prove unitarity of the recently found fourth-order self-dual model of spin-2 by investigating the analytic structure of its propagator. The model describes massive particles of helicity +2 (or -2) in $D=2+1$ and corresponds to the quadratic truncation of a higher derivative topologically massive gravity about a flat background. It is an intriguing example of a theory where a term in the propagator of the form $1/\lbrack\Box^2 (\Box - m^2)\rbrack $ does not lead to ghosts. The crucial role of the linearized Weyl symmetry in getting rid of the ghosts is pointed out. We use a peculiar pair of gauge conditions which fix the linearized reparametrizations and linearized Weyl symmetries separetely.
description: 9 pages, no figures
The Role of the Coherence Length in Exclusive Electroproduction of
  Vector Mesons off Nuclei
Creators: name: J. Huefner
name: B. Kopeliovich
name: J. Nemchik
Publisher: name: INFN Open Access Repository
Year: 1995

description: The variation of the coherence length $l_c=2\nu/(Q^2+m_V^2)$ in virtual
photoproduction of vector mesons off nuclei as a function of the photon energy
$\nu$ or virtuality $Q^2$ results in dramatic changes in the values of the
nuclear transparency. Color transparency effects can be easily mixed up with
the effects of the coherence length in incoherent photoproduction on nuclei.
Invariant Einstein metrics on generalized flag manifolds with two isotropy summands
Creators: name: Arvanitoyeorgos, Andreas
name: Chrysikos, Ioannis
Publisher: name: arXiv
Year: 2009
Subjects: subject: Differential Geometry (math.DG)
subject: Representation Theory (math.RT)
subject: FOS: Mathematics
subject: 53C25, 53C30, 22E46

description: Let $M=G/K$ be a generalized flag manifold, that is the adjoint orbit of a compact semisimple Lie group $G$. We use the variational approach to find invariant Einstein metrics for all flag manifolds with two isotropy summands. We also determine the nature of these Einstein metrics as critical points of the scalar curvature functional under fixed volume.
Recognition of Stroke Warning Signs and Risk Factors Among Rural Population in Central Pennsylvania
Creators: name: Zeenat Qureshi Stroke Institutes
Publisher: name: Zenodo
Year: 2018

description: Background

Recognition of stroke warning signs and risk factors reduces prehospital delay and increases stroke survival. The goal of this study was to evaluate the public knowledge of stroke warning signs and risk factors in a rural area in Central Pennsylvania.

Materials and Methods

In this study, the 2016 Sullivan County Health Fair attendees in central Pennsylvania answered a structured close-ended multiple choice questionnaire about stroke warning signs and risk factors. Further questions were asked about their reaction to acute stroke, the source of their stroke knowledge, and if they had personally known a stroke victim.

Results

Out of 163 respondents, 85.3% selected ≥3 (out of 4) correct stroke warning signs and 71.8% of respondents selected ≥3 (out of 5) correct stroke risk factors. Regarding the wrong stroke warning signs, 34.4% mentioned neck pain followed by chest pain (33.1%). Identification of ≥1 (out of 3) wrong stroke warning signs were significantly lower among the respondents of postgraduate level education in comparison with other literacy groups. 95.7% of respondents chose “call 911 immediately” in response to an acute stroke. A relative with a history of stroke was the most cited source of information. Multivariate analysis found that a high level of education increases odds of recognition of ≥3 correct stroke risk factors (0.21; 95% confidence interval, 0.09–0.61). Knowing anyone with stroke was associated with an awareness of the life-threatening nature of stroke (r = 0.21, P < 0.01).
A New Quark Model Approach to Hyperon Semi-Leptonic Decays
Creators: name: Ratcliffe, Philip G.
Publisher: name: INFN Open Access Repository
Year: 1997

description: A new analysis of hyperon semi-leptonic decay data is presented, based on
simple and general arguments for an SU(3)-breaking structure of the couplings
involved. The results obtained are compatible with those of earlier
investigations and highlight the uncertainties inherent in extraction of the
V_us Cabibbo-Kobayashi-Maskawa matrix element from such data, and the need for
complete analyses. For F and D, the results can be summarised by the ratio:
F/D=0.57+/-0.01; while as far as the value of V_us is concerned, the only
conclusion to be drawn is that, insofar as SU(3) breaking is still not totally
under control, the value obtained is compatible but not competitive with that
obtained from kaon semi-leptonic decays.
High star formation activity in the central region of a distant cluster at z=1.46
Creators: name: Hayashi, Masao
name: Kodama, Tadayuki
name: Koyama, Yusei
name: Tanaka, Ichi
name: Shimasaku, Kazuhiro
name: Okamura, Sadanori
Publisher: name: arXiv
Year: 2009
Subjects: subject: Cosmology and Nongalactic Astrophysics (astro-ph.CO)
subject: FOS: Physical sciences

description: We present an unbiased deep [OII] emission survey of a cluster XMMXCS J2215.9-1738 at z=1.46, the most distant cluster to date with a detection of extended X-ray emission. With wide-field optical and near-infrared cameras (Suprime-Cam and MOIRCS, respectively) on Subaru telescope, we performed deep imaging with a narrow-band filter NB912 (lambda_c=9139A, Delta_lambda=134A) as well as broad-band filters (B, z', J and Ks). From the photometric catalogues, we have identified 44 [OII] emitters in the cluster central region of 6'x6' down to a dust-free star formation rate of 2.6 Msun/yr (3 sigma). Interestingly, it is found that there are many [OII] emitters even in the central high density region. In fact, the fraction of [OII] emitters to the cluster members as well as their star formation rates and equivalent widths stay almost constant with decreasing cluster-centric distance up to the cluster core. Unlike clusters at lower redshifts (z<1) where star formation activity is mostly quenched in their central regions, this higher redshift 2215 cluster shows its high star formation activity even at its centre, suggesting that we are beginning to enter the formation epoch of some galaxies in the cluster core eventually. Moreover, we find a deficit of galaxies on the red sequence at magnitudes fainter than ~M*+0.5 on the colour-magnitude diagram. This break magnitude is brighter than that of lower redshift clusters, and it is likely that we are seeing the formation phase of more massive red galaxies in the cluster core at z~1. These results may indicate inside-out and down-sizing propagation of star formation activity in the course of cluster evolution.
description: 12 pages, 9 figures, 1 table, accepted for publication in MNRAS
Additional file 2 of Genome-centric metagenomics reveals the host-driven dynamics and ecological role of CPR bacteria in an activated sludge system
Creators: name: Wang, Yulin
name: Zhang, Yulin
name: Hu, Yu
name: Liu, Lei
name: Liu, Shuang-Jiang
name: Zhang, Tong
Publisher: name: figshare
Year: 2023
Subjects: subject: Microbiology
subject: FOS: Biological sciences
subject: Genetics

description: Additional file 2: Figure S1. Completeness estimation using different gene marker sets. Figure S2. Ridge plot shows the temporal dynamics of abundant saccharimonadial bacteria with relative abundance >0.5% in at least one activated sludge sample. The numbers in the ridge plot are the maximum relative abundance of CPR bacteria. The lowest taxonomic assignments of different CPR bacteria are shown in brackets. Figure S3. Ridge plot shows the temporal dynamics of abundant CPR bacteria from the same module and associated bacteria inferred by the microbial network. The lowest taxonomic assignments of different CPR bacteria are shown in brackets. Figure S4. Representation of CPR proteome content reporting how the pangenome varies as genomes are added in random order to the analysis. This analysis is conducted with pangenome of protein families with 5 or more members among CPR bacteria (a) and all protein families (b). Figure S5. COG categories of ORFs predicted by the putative lateral transferred DNA fragments. Figure S6. Relative abundance of CPR bacteria in activated sludge and effluent metagenomes generated from corresponding samples.
Entanglement Metrology Using a Joint Readout of Superconducting Qubits
Creators: name: Chow, J. M.
name: DiCarlo, L.
name: Gambetta, J. M.
name: Nunnenkamp, A.
name: Bishop, Lev S.
name: Frunzio, L.
name: Devoret, M. H.
name: Girvin, S. M.
name: Schoelkopf, R. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: Accurate and precise detection of multi-qubit entanglement is key for the experimental development of quantum computation. Traditionally, non-classical correlations between entangled qubits are measured by counting coincidences between single-shot readouts of individual qubits. We report entanglement metrology using a single detection channel with direct access to ensemble-averaged correlations between two superconducting qubits. Following validation and calibration of this joint readout, we demonstrate full quantum tomography on both separable and highly-entangled two-qubit states produced on demand. Using a subset of the measurements required for full tomography, we perform entanglement metrology with ~95% accuracy and ~98% precision despite ~10% fidelity of single measurements. For the highly entangled states, measured Clauser-Horne-Shimony-Holt operators reach a maximum value of 2.61+/-0.04 and entanglement witnesses give a lower bound of ~88% on concurrence. In its present form, this detector will be able to resolve future improvements in the production of two-qubit entanglement and is immediately extendable to 3 or 4 qubits.
description: 7 pages, 4 figures, and 4 pages of supporting material
Salto di qualità nella rete VLBI geodetica
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2016

Condotte con successo le prime prove di osservazioni simultanee con tre antenne radio di nuova generazione della NASA per osservazioni interferometriche a lunghissima base, che andranno a sostituire nel tempo quelle oggi operative. Il commento di Monia Negusini (INAF)
Marte nel caos dopo Siding Spring
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Nell'ottobre 2014 la cometa C/2013 A1 è passata a soli 140 mila chilometri da Marte. Per diverse ore la sua chioma ha travolto l'atmosfera marziana arrivando davvero vicino alla superficie: una marea invisibile di particelle cariche si sono temporaneamente fuse con il campo magnetico del pianeta. Il caos su Marte
Climbing the Jaynes-Cummings Ladder and Observing its Sqrt(n) Nonlinearity in a Cavity QED System
Creators: name: Fink, J. M.
name: Goeppl, M.
name: Baur, M.
name: Bianchetti, R.
name: Leek, P. J.
name: Blais, A.
name: Wallraff, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: Superconductivity (cond-mat.supr-con)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: The already very active field of cavity quantum electrodynamics (QED), traditionally studied in atomic systems, has recently gained additional momentum by the advent of experiments with semiconducting and superconducting systems. In these solid state implementations, novel quantum optics experiments are enabled by the possibility to engineer many of the characteristic parameters at will. In cavity QED, the observation of the vacuum Rabi mode splitting is a hallmark experiment aimed at probing the nature of matter-light interaction on the level of a single quantum. However, this effect can, at least in principle, be explained classically as the normal mode splitting of two coupled linear oscillators. It has been suggested that an observation of the scaling of the resonant atom-photon coupling strength in the Jaynes-Cummings energy ladder with the square root of photon number n is sufficient to prove that the system is quantum mechanical in nature. Here we report a direct spectroscopic observation of this characteristic quantum nonlinearity. Measuring the photonic degree of freedom of the coupled system, our measurements provide unambiguous, long sought for spectroscopic evidence for the quantum nature of the resonant atom-field interaction in cavity QED. We explore atom-photon superposition states involving up to two photons, using a spectroscopic pump and probe technique. The experiments have been performed in a circuit QED setup, in which ultra strong coupling is realized by the large dipole coupling strength and the long coherence time of a superconducting qubit embedded in a high quality on-chip microwave cavity.
description: ArXiv version of manuscript published in Nature in July 2008, 5 pages, 5 figures, hi-res version at http://www.finkjohannes.com/SqrtNArxivPreprint.pdf
Il Telescopio Solare Europeo è strategico
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2016

Il Telescopio Solare Europeo (EST) è stato selezionato dallo European Strategy Forum for Research Infrastructures tra le 21 infrastrutture scientifiche considerate strategiche per l’Europa. Il progetto è stato promosso dalla comunità astrofisica solare europea. Per l’Italia, partecipano l’INAF e le Università di Calabria, Catania e Roma Tor Vergata
Cristalli di ghiaccio per la cometa 67P
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2016

Il ghiaccio all’interno della cometa 67P/Churyumov-Gerasimenko si presenta essenzialmente in forma cristallina. Questo ghiaccio si sarebbe dunque prodotto nella nebulosa da cui si è formato il Sistema solare, di cui quindi condivide l’età. La scoperta è stata ottenuta da un team internazionale, tra gli autori Jonathan Lunine della Cornell University, a cui abbiamo chiesto un commento
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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¡Ð¾Ð²ÐµÑÐ¾Ð²Ð°, ÐÐ½Ð½Ð°
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ÑÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¸Ðµ ÑÑÐ°Ð½Ð´Ð°ÑÑÑ
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La forza invisibile che accende le galassie nane
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2016

Batuffoli di sola materia oscura attorno alle galassie nane possono innescare fenomeni di intensa formazione stellare. Questa interazione, secondo una simulazione al computer realizzata da un gruppo di ricerca olandese e statunitense, è alla base anche della formazione delle misteriose galassie nane sferoidali isolate
title: Ð­Ð»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ ÐÐ­Ð¡ Ñ ÑÐµÐ°ÐºÑÐ¾ÑÐ°Ð¼Ð¸ ÐÐÐ­Ð -1200 Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 2*1200 Ð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°ÑÐ°Ð½Ð¾Ð²Ð°, 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: 2017
Subjects: ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÐ°Ð½ÑÐ¸Ð¸
Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
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description: Ð ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÑÐ°ÑÑÐ¸ Ð°ÑÐ¾Ð¼Ð½Ð¾Ð¹ ÑÐ»ÐµÐºÑÑÐ¾ÑÑÐ°Ð½ÑÐ¸Ð¸. ÐÑÐ±ÑÐ°Ð½Ð° Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ½Ð°Ñ ÑÑÐµÐ¼Ð° Ð¸ Ð¾ÑÐ½Ð¾Ð²Ð½Ð¾Ðµ ÑÐ»ÐµÐºÑÑÐ¾Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. Ð Ð°ÑÑÑÐ¸ÑÐ°Ð½Ñ ÑÐ¾ÐºÐ¸ ÐºÐ¾ÑÐ¾ÑÐºÐ¾Ð³Ð¾ Ð·Ð°Ð¼ÑÐºÐ°Ð½Ð¸Ñ. ÐÑÐ±ÑÐ°Ð½Ñ ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð°Ð¿Ð¿Ð°ÑÐ°ÑÑ Ð¸ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð½Ð¸ÐºÐ¸. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð³Ð»Ð°Ð²Ð½Ð°Ñ ÑÑÐµÐ¼Ð° ÑÐ»ÐµÐºÑÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾ÐµÐ´Ð¸Ð½ÐµÐ½Ð¸Ð¹ Ð¸ ÑÑÐµÐ¼Ð° ÑÐ¾Ð±ÑÑÐ²ÐµÐ½Ð½ÑÑ Ð½ÑÐ¶Ð´.
Efficient methods for the numerical integration of ordinary differential equations
Creators: name: Creemer, Albert Lee
Publisher: name: University of British Columbia
Year: 2011

description: The purpose of this thesis is to study the factors involved in determining a most efficient method for the numerical integration of the differential equation x' = f(t,x) . By "a most efficient method" we mean a method requiring a minimum of computation to obtain a solution within prescribed error bounds. We outline two computational procedures and derive estimates for the propagated error of a general multi-step method when based on either procedure. These estimates, lead us to conclude that a stable single-iterate procedure, involving one evaluation of f at each step, will determine a solution most efficiently. In particular, this procedure based on Adams formulas is recommended. Experimental results support our conclusion in all stable cases. However, these results also indicate that the role of stability in the choice of a most efficient procedure is in need of further investigation.
Sos, Marte rischia la contaminazione?
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2016

Parola all'esperto, John Robert Brucato (astrofisico ed esobiologo dell’INAF–Osservatorio Astrofisico di Arcetri): il modulo di atterraggio (EDM), nonostante abbia subito tutte le procedure di sterilizzazione, non verrà a contatto con le regioni speciali e quindi le aree più sensibili nel pianeta (dove ci sono acqua ed eventuali batteri) non dovrebbero entrare in contatto con microbi terrestri
Высшее образование сегодня,Выпуск 8 2018
Creators: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Publisher: name: Автономная некоммерческая организация высшего образования «Российский новый университет»
Year: 2018

description: Высшее образование сегодня,Выпуск 8 2018
Instrument and data analysis challenges for imaging spectropolarimetry
Creators: name: Denker, C.
Publisher: name: arXiv
Year: 2010
Subjects: subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: The next generation of solar telescopes will enable us to resolve the fundamental scales of the solar atmosphere, i.e., the pressure scale height and the photon mean free path. High-resolution observations of small-scale structures with sizes down to 50 km require complex post-focus instruments, which employ adaptive optics (AO) and benefit from advanced image restoration techniques. The GREGOR Fabry-Perot Interferometer (GFPI) will serve as an example of such an instrument to illustrate the challenges that are to be expected in instrumentation and data analysis with the next generation of solar telescopes.
description: 4 pages, 1 figure, accepted for publication in Astronomische Nachrichten/AN, special issue of the 1st EAST-ATST Workshop: "Science with large solar telescopes" in Freiburg, Germany, October 14-16, 2009
Additional file 2 of Co-enrichment of CD8-positive T cells and macrophages is associated with clinical benefit of tislelizumab in solid tumors
Creators: name: Ye, Dingwei
name: Desai, Jayesh
name: Shi, Jingwen
name: Liu, Si-Yang Maggie
name: Shen, Wei
name: Liu, Tengfei
name: Shi, Yang
name: Wang, Dan
name: Liang, Liang
name: Yang, Silu
name: Ma, Xiaopeng
name: Jin, Wei
name: Zhang, Pei
name: Huang, Ruiqi
name: Shen, Zhirong
name: Zhang, Yun
name: Wu, Yi-Long
Publisher: name: figshare
Year: 2023
Subjects: subject: Immunology
subject: FOS: Clinical medicine

description: Additional file 2. Ethics committees and study approval numbers.
FracTCAM: Fracturable LUTRAM-Based TCAM Emulation on Xilinx FPGAs
Creators: name: Khattak, Shadan
name: Zahir, Ali
name: Ullah, Anees
name: Reviriego, Pedro
name: Muslim, Fahad bin
name: Ahmad, Waleed
Publisher: name: figshare
Year: 2023
Subjects: Electronics, sensors and digital hardware not elsewhere classified

description: In this brief, we present FracTCAM, an efficient methodology for ternary content addressable memory (TCAM) emulation on Xilinx field-programmable gate arrays (FPGAs) by leveraging primitive architectural resources. The proposed methodology exploits the fracturable nature of lookup table random access memories (LUTRAMs) and built-in slice flip-flops for deeper pipelining. Multiple slices can be combined together to build deeper and wider TCAMs using ANDing operations. This results in TCAM implementations that achieve lower resources utilization, lower delay, and power consumption. A comparison with the existing schemes shows that FracTCAM consistently achieves the best performance per area (PA) and performance per area per watt (PAW).
Internal relaxation time in immersed particulate materials
Creators: name: Rognon, P.
name: Einav, I.
name: Gay, C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Fluid Dynamics (physics.flu-dyn)
subject: FOS: Physical sciences

description: We study the dynamics of the solid to liquid transition for a model material made of elastic particles immersed in a viscous fluid. The interaction between particle surfaces includes their viscous lubrication, a sharp repulsion when they get closer than a tuned steric length and their elastic deflection induced by those two forces. We use Soft Dynamics to simulate the dynamics of this material when it experiences a step increase in the shear stress and a constant normal stress. We observe a long creep phase before a substantial flow eventually establishes. We find that the typical creep time relies on an internal relaxation process, namely the separation of two particles driven by the applied stress and resisted by the viscous friction. This mechanism should be relevant for granular pastes, living cells, emulsions and wet foams.
L’astrochimica sbarca a Firenze
Creators: Francesca Brunetti e Linda Podio
Publisher: name: Media Inaf
Year: 2016

Capire l’evoluzione chimica del gas e della polvere interstellare richiede una forte sinergia tra astrofisici e chimici. Il 10 e 11 marzo a Firenze, nella splendida cornice di Palazzo Strozzi, il Primo Workshop Italiano di Astrochimica: dalle osservazioni ai modelli teorici, dagli esperimenti di laboratorio ai risultati più recenti della ricerca, per discutere le domande aperte e intraprendere nuove collaborazioni