Institution
University of Warsaw
Education•Warsaw, Poland•
About: University of Warsaw is a education organization based out in Warsaw, Poland. It is known for research contribution in the topics: Population & Large Hadron Collider. The organization has 20832 authors who have published 56617 publications receiving 1185084 citations. The organization is also known as: Uniwersytet Warszawski & Warsaw University.
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University of Glasgow1, University of Salerno2, Max Planck Society3, University of Southampton4, University of Paris-Sud5, University of Nice Sophia Antipolis6, Washington State University7, Istituto Nazionale di Fisica Nucleare8, University of Warsaw9, University of Naples Federico II10, University of Birmingham11, Cardiff University12, University of Rome Tor Vergata13, Moscow State University14, California Institute of Technology15, VU University Amsterdam16, fondazione bruno kessler17, Leibniz University of Hanover18, University of Cambridge19, University of Tübingen20, University of Urbino21, University of Jena22, University of the Balearic Islands23, Northwestern University24, University of Minnesota25, University of Savoy26, Pennsylvania State University27, University of Pisa28, Roma Tre University29, Sapienza University of Rome30, University of Mississippi31
TL;DR: In this article, a special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates, including the most relevant fundamental noise contributions.
Abstract: Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a third-generation gravitational wave detector, has been proposed in order to fully open up the emerging field of gravitational wave astronomy. In this paper we describe sensitivity models for ET and investigate potential limits imposed by fundamental noise sources. A special focus is set on evaluating the frequency band below 10 Hz where a complex mixture of seismic, gravity gradient, suspension thermal and radiation pressure noise dominates. We develop the most accurate sensitivity model, referred to as ET-D, for a third-generation detector so far, including the most relevant fundamental noise contributions.
682 citations
TL;DR: A growing number of applications of carbon nanotubes (CNTs) in analytical chemistry are discussed in this paper, where the largest number of reported applications concern design of novel gas sensors, voltammetry, enzymatic biosensors, immunosensors and DNA probes.
Abstract: Discoveries of new materials have significant impact on development of new methods and instrumentation for chemical analysis. Based on 104 references, this article illustrates a growing number of applications of carbon nanotubes (CNTs) in analytical chemistry. The largest numbers of reported applications concern design of novel gas sensors, voltammetry, enzymatic biosensors, immunosensors and DNA probes. The sorptive properties of CNTs are also employed for analytical purposes in various ways.
681 citations
University of Tokyo1, Boston University2, Brookhaven National Laboratory3, University of California, Irvine4, California State University, Dominguez Hills5, George Mason University6, Gifu University7, University of Hawaii8, KEK9, Kobe University10, Kyoto University11, Los Alamos National Laboratory12, Louisiana State University13, University of Maryland, College Park14, Massachusetts Institute of Technology15, University of Minnesota16, State University of New York System17, Nagoya University18, Niigata University19, Osaka University20, Seoul National University21, Shizuoka University22, Tohoku University23, Tokai University24, Tokyo Institute of Technology25, University of Warsaw26, University of Washington27
TL;DR: In this paper, a number of different fits to solar neutrino mixing and mass square difference were performed using 1496 days of Super-Kamiokande-I's solar NE data.
680 citations
TL;DR: In this article, the authors compute the Galactic merger rates for NS-NS, BH-BH, and BH -BH mergers with the StarTrack code and show that the binding energy of the envelope plays a pivotal role in determining whether a binary merges within a Hubble time.
Abstract: The last decade of observational and theoretical developments in stellar and binary evolution provides an opportunity to incorporate major improvements to the predictions from population synthesis models. We compute the Galactic merger rates for NS-NS, BH-NS, and BH-BH mergers with the StarTrack code. The most important revisions include updated wind mass-loss rates (allowing for stellar-mass black holes up to 80 M {sub Sun }), a realistic treatment of the common envelope phase (a process that can affect merger rates by 2-3 orders of magnitude), and a qualitatively new neutron star/black hole mass distribution (consistent with the observed {sup m}ass gap{sup )}. Our findings include the following. (1) The binding energy of the envelope plays a pivotal role in determining whether a binary merges within a Hubble time. (2) Our description of natal kicks from supernovae plays an important role, especially for the formation of BH-BH systems. (3) The masses of BH-BH systems can be substantially increased in the case of low metallicities or weak winds. (4) Certain combinations of parameters underpredict the Galactic NS-NS merger rate and can be ruled out. (5) Models incorporating delayed supernovae do not agree with the observed NS/BH 'mass gap', in accordance with our previousmore » work. This is the first in a series of three papers. The second paper will study the merger rates of double compact objects as a function of redshift, star formation rate, and metallicity. In the third paper, we will present the detection rates for gravitational-wave observatories, using up-to-date signal waveforms and sensitivity curves.« less
678 citations
University of Tokyo1, Boston University2, Seoul National University3, Brookhaven National Laboratory4, University of California, Irvine5, California State University6, George Mason University7, Gifu University8, University of Hawaii at Manoa9, Kobe University10, Los Alamos National Laboratory11, Louisiana State University12, University of Maryland, College Park13, University of Chicago14, Miyagi University of Education15, Stony Brook University16, Niigata University17, Shizuoka University18, Osaka University19, Tohoku University20, Tokai University21, Tokyo Institute of Technology22, University of Warsaw23, University of Washington24
TL;DR: The first results of the solar neutrino flux measurement from Super-Kamiokande are presented in this article, where the results are obtained from data taken between 31 May 1996, and 23 June 1997.
Abstract: The first results of the solar neutrino flux measurement from Super-Kamiokande are presented. The results shown here are obtained from data taken between 31 May 1996, and 23 June 1997. Using our measurement of recoil electrons with energies above 6.5 MeV, we infer the total flux of ${}^{8}\mathrm{B}$ solar neutrinos to be $2.42\ifmmode\pm\else\textpm\fi{}0.06(\mathrm{stat}{)}_{\ensuremath{-}0.07}^{+0.10}(\mathrm{syst})\ifmmode\times\else\texttimes\fi{}{10}^{6}\mathrm{cm}{}^{\ensuremath{-}2}{\mathrm{s}}^{\ensuremath{-}1}$. This result is consistent with the Kamiokande measurement and is 36% of the flux predicted by the BP95 solar model. The flux is also measured in 1.5 month subsets and shown to be consistent with a constant rate.
677 citations
Authors
Showing all 21191 results
| Name | H-index | Papers | Citations |
|---|---|---|---|
| Alexander Malakhov | 139 | 1486 | 99556 |
| Emmanuelle Perez | 138 | 1550 | 99016 |
| Piotr Zalewski | 135 | 1388 | 89976 |
| Krzysztof Doroba | 133 | 1440 | 89029 |
| Hector F. DeLuca | 133 | 1303 | 69395 |
| Krzysztof M. Gorski | 132 | 380 | 105912 |
| Igor Golutvin | 131 | 1282 | 88559 |
| Jan Krolikowski | 131 | 1289 | 83994 |
| Michal Szleper | 130 | 1238 | 82036 |
| Anatoli Zarubin | 129 | 1204 | 86435 |
| Malgorzata Kazana | 129 | 1175 | 81106 |
| Artur Kalinowski | 129 | 1162 | 81906 |
| Predrag Milenovic | 129 | 1185 | 81144 |
| Marcin Konecki | 128 | 1178 | 79392 |
| Karol Bunkowski | 128 | 1192 | 79455 |