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Institution

Collège de France

EducationParis, France
About: Collège de France is a education organization based out in Paris, France. It is known for research contribution in the topics: Population & Receptor. The organization has 6541 authors who have published 11983 publications receiving 648742 citations. The organization is also known as: College de France.


Papers
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Journal ArticleDOI
TL;DR: Stable nanoparticles dispersions of the porous hybrid MIL-101(Cr) allow dip-coating of high quality optical thin films with dual hierarchical porous structure and for the first time, mechanical and sorption properties of mesoporous MOFs based thin films are evaluated.

143 citations

Journal ArticleDOI
TL;DR: It is shown that optical-lattice-based experiments can be tailored to directly visualize the propagation of topological edge modes, and the scheme, applicable to an assortment of atomic topological phases, provides a method for imaging the dynamics of topology edge modes.
Abstract: Detecting topological order in cold-atom experiments is an ongoing challenge, the resolution of which offers novel perspectives on topological matter. In material systems, unambiguous signatures of topological order exist for topological insulators and quantum Hall devices. In quantum Hall systems, the quantized conductivity and the associated robust propagating edge modes—guaranteed by the existence of nontrivial topological invariants—have been observed through transport and spectroscopy measurements. Here, we show that optical-lattice-based experiments can be tailored to directly visualize the propagation of topological edge modes. Our method is rooted in the unique capability for initially shaping the atomic gas and imaging its time evolution after suddenly removing the shaping potentials. Our scheme, applicable to an assortment of atomic topological phases, provides a method for imaging the dynamics of topological edge modes, directly revealing their angular velocity and spin structure.

143 citations

Journal ArticleDOI
Felix Aharonian1, A. G. Akhperjanian1, Klaus-Michael Aye2, A. R. Bazer-Bachi3, M. Beilicke1, Wystan Benbow1, David Berge1, P. Berghaus4, Konrad Bernlöhr1, O. Bolz1, Catherine Boisson3, C. Borgmeier5, F. Breitling5, A. M. Brown2, J. Bussons Gordo6, P. M. Chadwick2, V. R. Chitnis3, L.-M. Chounet7, R. Cornils1, Luigi Costamante1, B. Degrange7, A. Djannati-Ataï1, L. O'c. Drury8, Tulun Ergin5, P. Espigat4, F. Feinstein1, P. Fleury7, G. Fontaine7, Stefan Funk1, Y. A. Gallant1, B. Giebels7, Stefan Gillessen1, P. Goret9, Julien Guy3, C. Hadjichristidis2, M. Hauser, G. Heinzelmann10, Gilles Henri11, G. Hermann1, Jim Hinton1, Werner Hofmann1, M. Holleran12, Dieter Horns1, O. C. de Jager12, I. Jung1, B. Khélifi1, Nu. Komin5, A. Konopelko1, I. J. Latham2, R. Le Gallou2, M. Lemoine7, A. Lemière4, N. Leroy7, Thomas Lohse5, A. Marcowith3, Conor Masterson1, T. J. L. McComb2, M. de Naurois1, S. J. Nolan2, A. Noutsos2, K. J. Orford1, J. L. Osborne1, M. Ouchrif3, M. Panter1, Guy Pelletier11, S. Pita4, Martin Pohl13, Gerd Pühlhofer1, Michael Punch4, B. C. Raubenheimer12, Martin Raue1, J. Raux3, S. M. Rayner2, I. Redondo3, I. Redondo7, A. Reimer13, Olaf Reimer13, J. Ripken10, M. Rivoal3, L. Rob14, L. Rolland3, Gavin Rowell1, V. Sahakian15, L. Saugé1, S. Schlenker5, Reinhard Schlickeiser13, C. Schuster13, Ullrich Schwanke5, M. Siewert13, Helene Sol3, R. Steenkamp16, C. Stegmann5, J.-P. Tavernet3, C. G. Théoret4, M. Tluczykont7, M. Tluczykont3, D. J. van der Walt12, G. Vasileiadis1, P. Vincent3, B. Visser12, Heinrich J. Völk1, Stefan Wagner 
01 Feb 2005
TL;DR: The high frequency peaked BL Lac PKS 2155-304 at redshift z=0.117 has been detected with high significance (~45 sigma) at energies greater than 160 GeV, using the H.E.S. stereoscopic array of imaging air-Cherenkov telescopes in Namibia as discussed by the authors.
Abstract: The high-frequency peaked BL Lac PKS 2155-304 at redshift z=0.117 has been detected with high significance (~45 sigma) at energies greater than 160 GeV, using the H.E.S.S. stereoscopic array of imaging air-Cherenkov telescopes in Namibia. A strong signal is found in each of the data sets corresponding to the dark periods of July and October, 2002, and June-September, 2003. The observed flux of VHE gamma rays shows variability on time scales of months, days, and hours. The monthly-averaged integral flux above 300 GeV varies between 10% and 60% of the flux observed from the Crab Nebula. Energy spectra are measured for these individual periods of data taking and are characterized by a steep power law with a time-averaged photon index of 3.32 +/- 0.06. An improved chi-square per degree of freedom is found when either a power law with an exponential cutoff energy or a broken power law are fit to the time-averaged energy spectrum. However, the significance of the improvement is marginal (~2 sigma). The suggested presence of features in the energy spectrum may be intrinsic to the emission from the blazar, or an indication of absorption of TeV gamma rays by the extragalactic infrared background light.

143 citations

Journal ArticleDOI
TL;DR: In this article, the authors present new BeppoSAX observations of the TeV-emitting blazar Mrk 501 performed in 1999 June and a homogeneous reanalysis of all the Beppo SAX observations during the period from 1997 April to 1999 June.
Abstract: We present new BeppoSAX observations of the TeV-emitting blazar Mrk 501 performed in 1999 June and a homogeneous reanalysis of all the BeppoSAX observations during the period from 1997 April to 1999 June. Recently published TeV spectra by the Cerenko Array at Themis, which are quasi-simultaneous with the 1997 BeppoSAX pointings, are used to constrain further the physical parameters of the jet in 1997 April with detailed models of the X-ray and TeV components. During the 1997-1999 period, the peak frequency of the synchrotron emission moved from about 100 keV in 1997 April to 0.5 keV in 1999 June. The shift in the peak frequency appears to be correlated with the long-term luminosity decrease. We interpret the results in the framework of a homogeneous synchrotron self-Compton model, discussing the evolution of the physical parameters of the emitting region under simple assumptions for the variability model. We also compute the expected variations of the TeV flux under the same assumptions.

143 citations

Journal ArticleDOI
TL;DR: In this paper, the authors studied the dynamics of the Teichmuller flow in the moduli space of Abelian differentials and showed that the (Masur-Veech) invariant probability measure is exponentially mixing for the class of Holder observables.
Abstract: We study the dynamics of the Teichmuller flow in the moduli space of Abelian differentials (and more generally, its restriction to any connected component of a stratum). We show that the (Masur-Veech) absolutely continuous invariant probability measure is exponentially mixing for the class of Holder observables. A geometric consequence is that the SL(2, R) action in the moduli space has a spectral gap.

142 citations


Authors

Showing all 6597 results

NameH-indexPapersCitations
Pierre Chambon211884161565
Irving L. Weissman2011141172504
David R. Williams1782034138789
Kari Alitalo174817114231
Pierre Bourdieu153592194586
Stanislas Dehaene14945686539
Howard L. Weiner144104791424
Alain Fischer14377081680
Yves Agid14166974441
Michel Foucault140499191296
Jean-Pierre Changeux13867276462
Jean-Marie Tarascon136853137673
K. Ganga13227299004
Jacques Delabrouille13135494923
G. Patanchon12824187233
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Performance
Metrics
No. of papers from the Institution in previous years
YearPapers
20238
202293
2021418
2020429
2019385
2018391