Institution
University of Milano-Bicocca
Education•Milan, Italy•
About: University of Milano-Bicocca is a education organization based out in Milan, Italy. It is known for research contribution in the topics: Population & Blood pressure. The organization has 8972 authors who have published 22322 publications receiving 620484 citations. The organization is also known as: Università degli Studi di Milano-Bicocca & Universita degli Studi di Milano-Bicocca.
Topics: Population, Blood pressure, Large Hadron Collider, Branching fraction, Ambulatory blood pressure
Papers published on a yearly basis
Papers
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TL;DR: In this paper, the authors propose the use of social media data and sentiment analysis to study the affect-based responses to organizational actions by citizens, and critically discuss and compare the method used to measure organizational legitimacy.
Abstract: Conventional quantitative methods for the measurement of organizational legitimacy consider mainly three sources that make judgments about organizations visible: news media, accreditation bodies, and surveys Over the last decade, however, social media have enabled ordinary citizens to bypass the gatekeeping function of these institutional evaluators and autonomously make individual judgments public This inclusion of voices beyond functional and formally organized stakeholder groups potentially pluralizes the ongoing discussions about organizations The individual judgments in blogs, tweets, and Facebook posts give indication about the broader fit between an organization’s perceived behavior and heterogeneous social norms and therefore constitute an indicator of organizational legitimacy that can be accessed and measured We propose the use of social media data and sentiment analysis to study the affect-based responses to organizational actions by citizens We critically discuss and compare the method wi
143 citations
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TL;DR: In this paper, the authors explore the spin evolution of massive dual black holes orbiting inside a circumnuclear disc, relic of a gas-rich galaxy merger, and find that the black hole spins loose memory of their initial orientation, as accretion torques suffice to align the spins with the angular momentum of their orbit.
Abstract: Using high-resolution hydrodynamical simulations, we explore the spin evolution of massive dual black holes orbiting inside a circumnuclear disc, relic of a gas-rich galaxy merger. The black holes spiral inwards from initially eccentric co- or counter-rotating coplanar orbits relative to the disc’s rotation, and accrete gas that is carrying a net angular momentum. As the black hole mass grows, its spin changes in strength and direction due to its gravito-magnetic coupling with the small-scale accretion disc. We find that the black hole spins loose memory of their initial orientation, as accretion torques suffice to align the spins with the angular momentum of their orbit on a short time-scale (1–2 Myr). A residual off-set in the spin direction relative to the orbital angular momentum remains, at the level of 10 ◦ for the case of a cold disc, and 30 ◦ for a warmer disc. Alignment in a cooler disc is more effective due to the higher coherence of the accretion flow near each black hole that reflects the largescale coherence of the disc’s rotation. If the massive black holes coalesce preserving the spin directions set after formation of a Keplerian binary, the relic black hole resulting from their coalescence receives a relatively small gravitational recoil. The distribution of recoil velocities inferred from a simulated sample of massive black hole binaries has median 70 km s −1 ,
143 citations
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TL;DR: Starting treatment with a combination of two drugs is associated with a reduced risk of treatment discontinuation in patients initiating treatment with mono or combination therapy, as measured by persistence with antihypertensive drug therapy.
Abstract: ObjectivesTo measure persistence with antihypertensive drug therapy in patients initiating treatment with mono or combination therapy.MethodsData analysis was based on two cohorts of patients, that is, a cohort derived from the registration of drug prescriptions in all residents of the Lombardy regi
143 citations
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TL;DR: In this article, the production of charm and bottom quarks at forward rapidity in pp collisions at the LHC was discussed, and the QCD predictions for the run at [Formula: see text]
Abstract: We discuss production of charm and bottom quarks at forward rapidity in pp collisions at the LHC, updating the QCD predictions for the run at [Formula: see text] TeV. We show that, while the absolute rates suffer from large theoretical systematics, dominated by scale uncertainties, the increase relative to the rates precisely measured at 7 TeV can be predicted with an accuracy of a few percent, sufficient to highlight the sensitivity to the gluon distribution function.
143 citations
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TL;DR: In mildly to moderately hypertensive patients, carotid intima-media thickness and cardiovascular outcomes were related to the mean clinic or ambulatory SBP achieved by treatment but not to on-treatment visit-to-visit clinic or 24-hour BP variability, suggesting inconsistency of BP control between visits plays a less important prognostic role than long-term average BP levels.
Abstract: Background—In high-cardiovascular-risk treated hypertensive patients, the incidence of cardiovascular events has been reported to relate to visit-to-visit blood pressure (BP) variability. We invest...
143 citations
Authors
Showing all 9226 results
Name | H-index | Papers | Citations |
---|---|---|---|
Carlo Rovelli | 146 | 1502 | 103550 |
Giuseppe Mancia | 145 | 1369 | 139692 |
Marco Bersanelli | 142 | 526 | 105135 |
Teruki Kamon | 142 | 2034 | 115633 |
Marco Colonna | 139 | 512 | 71166 |
M. I. Martínez | 134 | 1251 | 79885 |
A. Mennella | 132 | 463 | 93236 |
Roberto Salerno | 132 | 1197 | 83409 |
Federico Ferri | 132 | 1376 | 89337 |
Marco Paganoni | 132 | 1438 | 88482 |
Arabella Martelli | 131 | 1318 | 84029 |
Sandra Malvezzi | 129 | 1326 | 84401 |
Andrea Massironi | 129 | 1115 | 78457 |
Marco Pieri | 129 | 1285 | 82914 |
Cristina Riccardi | 129 | 1627 | 91452 |