R Murray, M Spanner, S Patchkovskii… - Physical Review Letters, 2011 - APS Ryan Murray,1,2 Michael Spanner,3 Serguei Patchkovskii,4,* and Misha Yu. Ivanov2 1University of Waterloo, Waterloo ON, N2L 3G1, Canada 2Department of Physics, Imperial College London, South Kensington Campus, SW7 2AZ London, United Kingdom 3National ... Cited by 1 - Related articles - All 4 versions
MP Lavery, DJ Roberston, GD Love… - International …, 2011 - opticsinfobase.org Light is a ubiquitous carrier of information. At both classical and quantum levels, information can be encoded in terms of the optical intensity, frequency, polarization or direction. The polarization sets the spin angular momentum of the photon, that can take one of two orthogonal states ... Related articles
J Deisenhofer, Z Wang… - Bulletin of the American Physical …, 2011 - APS We report on the magnetic and phononic excitation spectrum of SrCrO~determined by THz and infrared (IR) spectroscopy, specific heat, and electron spin resonance measurements. We identify the singlet-triplet excitations in the dimerized ground state and observe an extended ... All 4 versions
[PDF] from arxiv.orgM Kunitomo, M Ikoma, B Sato, Y Katsuta… - Arxiv preprint arXiv: …, 2011 - arxiv.org Abstract. Around low- and intermediate-mass (1.5-3 M⊙) red giants, no planets have been found inside 0.6 AU. Such a paucity is not seen in the case of 1M⊙ main sequence stars. In this study, we examine the possibility that short-period planets were engulfed by their host ... Cited by 1 - Related articles - All 5 versions
[PDF] from arxiv.orgBE Schaefer, AU Landolt, M Linnolt… - Arxiv preprint arXiv: …, 2011 - arxiv.org ... Discovery, the Pre-eruption Rise, the Pre-eruption Orbital Period, and the Reason for the Long Delay ... We present 19 timings of pho- tometric minima from 1986 to February 2011, where the orbital period is fast increasing with P/ ˙ P = +313, 000 years. ...
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