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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Nagoya University1, University of Notre Dame2, Massey University3, University of Warsaw4, Royal Society5, University of St Andrews6, Centre national de la recherche scientifique7, Ohio State University8, Lawrence Livermore National Laboratory9, Institute for Advanced Study10, University of Auckland11, University of Canterbury12, Victoria University of Wellington13, Konan University14, College of Industrial Technology15, Institut d'Astrophysique de Paris16, University of Tasmania17, University of Chile18, National Institute for Space Research19, Liverpool John Moores University20, European Southern Observatory21, University of Stuttgart22, Ames Research Center23, University of the Free State24, University of Rijeka25, University of Vienna26, Niels Bohr Institute27, NASA Exoplanet Science Institute28, Space Telescope Science Institute29, Las Cumbres Observatory Global Telescope Network30, Heidelberg University31, University of Concepción32, Texas A&M University33, Chungbuk National University34, Korea Astronomy and Space Science Institute35, Auckland University of Technology36
TL;DR: The OGLE-2007-BLG-368Lb with a planet-star mass ratio of q = [9.5 ± 2.1] × 10^(-5] via gravitational microlensing was discovered in real-time thanks to the high cadence of the Microlensing Observations in Astrophysics survey and intensive followup observations.
Abstract: We present the discovery of a Neptune-mass planet OGLE-2007-BLG-368Lb with a planet-star mass ratio of q = [9.5 ± 2.1] × 10^(-5) via gravitational microlensing. The planetary deviation was detected in real-time thanks to the high cadence of the Microlensing Observations in Astrophysics survey, real-time light-curve monitoring and intensive follow-up observations. A Bayesian analysis returns the stellar mass and distance at M_l = 0.64^(+0.21)_(–0.26) M_☉ and D_l = 5.9^(+0.9)_(–1.4) kpc, respectively, so the mass and separation of the planet are M_p = 20^(+7)_(–8) M_⊕ and a = 3.3^(+1.4)_(–0.8) AU, respectively. This discovery adds another cold Neptune-mass planet to the planetary sample discovered by microlensing, which now comprises four cold Neptune/super-Earths, five gas giant planets, and another sub-Saturn mass planet whose nature is unclear. The discovery of these 10 cold exoplanets by the microlensing method implies that the mass ratio function of cold exoplanets scales as dN_(pl)/d log q ∝ q^(–0.7±0.2) with a 95% confidence level upper limit of n < –0.35 (where dN_(pl)/d log q ∝ q^n). As microlensing is most sensitive to planets beyond the snow-line, this implies that Neptune-mass planets are at least three times more common than Jupiters in this region at the 95% confidence level.
253 citations
TL;DR: The framework provides new tools to extract physics from strong field geometry and leads to a generalization of the zeroth and first laws of black hole mechanics and sheds new light on the "origin of the first law".
Abstract: The notion of isolated horizons is extended to allow for distortion and rotation. Space-times containing a black hole, itself in equilibrium but possibly surrounded by radiation, satisfy these conditions. The framework has three types of applications: (i) it provides new tools to extract physics from strong field geometry; (ii) it leads to a generalization of the zeroth and first laws of black hole mechanics and sheds new light on the “origin” of the first law; and (iii) it serves as a point of departure for black hole entropy calculations in nonperturbative quantum gravity.
252 citations
Fermilab1, Iowa State University2, University of Cincinnati3, University of Oxford4, Brookhaven National Laboratory5, University of Cambridge6, University of Texas at Austin7, Universidade Federal de Goiás8, Tufts University9, Indiana University10, University of Minnesota11, College of William & Mary12, University of Sussex13, State University of Campinas14, University of Manchester15, Harvard University16, College of the Holy Cross17, Argonne National Laboratory18, University of São Paulo19, University of Pittsburgh20, University of Warsaw21, California Institute of Technology22, University College London23, Stanford University24, Rutherford Appleton Laboratory25, University of South Carolina26, Illinois Institute of Technology27, Otterbein University28, National and Kapodistrian University of Athens29, Texas A&M University30, University of Houston31
TL;DR: A new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data using the three-flavor formalism and constrain δ(CP), the θ(23} octant degeneracy and the mass hierarchy is reported.
Abstract: We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the ν_μ disappearance and ν_e appearance data using the three-flavor formalism. We measure |Δm^2_(32)|=[2.28–2.46]×10^(−3) eV^2 (68% C.L.) and sin^2θ_(23)=0.35–0.65 (90% C.L.) in the normal hierarchy, and |Δm^2_(32)|=[2.32–2.53]×10^(−3) eV^2 (68% C.L.) and sin2θ23=0.34–0.67 (90% C.L.) in the inverted hierarchy. The data also constrain δ_(CP), the θ_(23) octant degeneracy and the mass hierarchy; we disfavor 36% (11%) of this three-parameter space at 68% (90%) C.L.
252 citations
TL;DR: In this paper, the advantages and limitations of heavy metals sorption on three different carbon materials: activated carbon, carbon nanotubes, and carbon-encapsulated magnetic nanoparticles.
252 citations
TL;DR: In this article, the authors discussed the phenomenon of shape coexistence within the self-consistent Hartree-Fock method and the nuclear shell model and traced the occurrence of the coexisting configurations with different intrinsic shapes back to the properties of the effective Hamiltonian.
Abstract: The phenomenon of shape coexistence is discussed within the self-consistent Hartree-Fock method and the nuclear shell model. The occurrence of the coexisting configurations with different intrinsic shapes is traced back to the properties of the effective Hamiltonian.
252 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 |