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| Nature '''464''', 1018-1020 (15 April 2010) ''An image of an exoplanet separated by two diffraction beamwidths from a star'' | Nature '''464''', 1018-1020 (15 April 2010). ''An image of an exoplanet separated by two diffraction beamwidths from a star'' |
Interesting Papers Repository
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Phys. Rev. D 79, 122002 (2009) |
Prospects of higher-order Laguerre-Gauss modes in future gravitational wave detectors |
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Physics 3, 32 (2010) |
[http://physics.aps.org/viewpoint-for/10.1103/PhysRevLett.104.153901] |
Second-harmonic generation in microresonators through natural phase matching |
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Physics 3, 29 (2010) |
Precise simulations for future gravitational wave detectors |
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http://prl.aps.org/pdf/PRL/v104/i13/e133602 PRL 104, 133602 (2010) Backaction Amplification and Quantum Limits in Optomechanical Measurements P. Verlot, A. Tavernarakis, T. Briant, P.-F. Cohadon, and A. Heidmann
http://prl.aps.org/pdf/PRL/v104/i8/e083201 PRL 104, 083201 (2010) Direct Measurement of Intermediate-Range Casimir-Polder Potentials H. Bender, Ph.W. Courteille, C. Marzok, C. Zimmermann, and S. Slama
http://www.nature.com/nature/journal/v463/n7283/full/nature08685.html Nature 463, 924-925 An upper limit on the contribution of accreting white dwarfs to the type Ia supernova rate Marat Gilfanov1,2 & Ákos Bogdán1
http://prl.aps.org/pdf/PRL/v104/i7/e073601 PRL 104, 073601 (2010) Classical Signature of Ponderomotive Squeezing in a Suspended Mirror Resonator Francesco Marino,1 Francesco S. Cataliotti,2 Alessandro Farsi,1 Mario Siciliani de Cumis,3 and Francesco Marin1
http://prd.aps.org/pdf/PRD/v81/i4/e042001 PHYSICAL REVIEW D 81, 042001 (2010) Opto-acoustic interactions in gravitational wave detectors: Comparing flat-top beams with Gaussian beams S. Gras,* D. G. Blair, and L. Ju
http://prd.aps.org/pdf/PRD/v80/i12/e122005 PHYSICAL REVIEW D 80, 122005 (2009) Direct measurement of the anelasticity of a tungsten fiber Shan-Qing Yang, Liang-Cheng Tu, Cheng-Gang Shao, Qing Li, Qing-Lan Wang, Ze-Bing Zhou, and Jun Luo*
http://iopscience.iop.org/0264-9381/27/1/015003/pdf/0264-9381_27_1_015003.pdf Class. Quantum Grav. 27 (2010) 015003 A xylophone configuration for a third-generation gravitational wave detector S Hild1, S Chelkowski2, A Freise2, J Franc3, N Morgado3, R Flaminio3 and R DeSalvo4
Nature 464, 1018-1020 (15 April 2010). An image of an exoplanet separated by two diffraction beamwidths from a star
[http://www.economist.com/science-technology/displaystory.cfm?story_id=15905845]
[http://www.nature.com/nature/journal/v464/n7291/full/nature09007.html]