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Radiation pressure
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1	Nonlinear Analysis: Modelling and Control, 2010, Vol. 15, No. 3, 287–298 Effects of pressure work on natural convection flow around a sphere with radiation heat loss T. Akhter1 , M.A. Alim2 1 Add to Reading List Source URL: www.lana.lt Language: English - Date: 2010-09-17 07:32:18
2	UNIVERSITY OF CALIFORNIA, IRVINE Add to Reading List Source URL: special.lib.uci.edu Language: English - Date: 2015-03-10 17:48:08 Radiometry Education Science Radiometer Measurement Radiation pressure Measuring instrument Plume Thesis University of California Irvine Io Versine
3	Pickering Nuclear Generating Station - RegDocReporting For 2016 up toReport Number Event Title Quarter: 2016Q1 P Add to Reading List Source URL: www.opg.com Language: English - Date: 2016-07-27 15:35:11 Physics Piping Plumbing Chemistry Construction Valve Water industry Relief valve Boiler Pressure Ionizing radiation
4	PHYSICAL REVIEW B 72, 054506 共2005兲 Pressure dependence of phonon interactions in liquid 4He Damian H. S. Smith, Ruslan V. Vovk, Charles D. H. Williams, and Adrian F. G. Wyatt School of Physics, University of Exeter Add to Reading List Source URL: newton.ex.ac.uk Language: English - Date: 2007-02-09 07:53:22 Scattering Condensed matter physics Heat transfer Bosons Phonon Quasiparticles Light scattering Thermodynamic temperature Thermodynamics of nanostructures Sound amplification by stimulated emission of radiation
5	EPJ Web of Conferences 106, DOI: epjconf C Owned by the authors, published by EDP Sciences, 2016 Radiation Damage Assessment in the Reactor Pressure Add to Reading List Source URL: www.epj-conferences.org Language: English Nuclear technology Reactor pressure vessel Neutron flux Neutron Nuclear reactor Nuclear fuel cycle Light-water reactor Nuclear fuel
6	SUMMARY IV: FUNDAMENTAL PRINCIPLES • Stars are self-gravitating bodies in dynamical equilibrium → balance of gravity and internal pressure forces (hydrostatic equilibrium); • stars lose energy by radiation from the Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-18 06:59:04
7	SUMMARY IV: FUNDAMENTAL PRINCIPLES • Stars are self-gravitating bodies in dynamical equilibrium → balance of gravity and internal pressure forces (hydrostatic equilibrium); • stars lose energy by radiation from the Add to Reading List Source URL: www-astro.physics.ox.ac.uk Language: English - Date: 2004-11-18 06:59:23
8	BARC NEWSLETTER FIRST PRINCIPLES STUDIES ON HIGH PRESSURE EQUATION OF STATE AND PHASE STABILITY OF SOLIDS P. Modak and Ashok K. Verma High Pressure and Synchrotron Radiation Physics Division Add to Reading List Source URL: www.barc.gov.in Language: English - Date: 2013-12-06 05:47:15
9	BARC NEWSLETTER FIRST PRINCIPLES STUDIES ON HIGH PRESSURE EQUATION OF STATE AND PHASE STABILITY OF SOLIDS P. Modak and Ashok K. Verma High Pressure and Synchrotron Radiation Physics Division Add to Reading List Source URL: www.barc.gov.in Language: English - Date: 2013-12-06 05:47:10
10	Accessing the radiation pressure ion acceleration regime using ultrathin targets Nicholas Dover Add to Reading List Source URL: hedpschool.lle.rochester.edu Language: English - Date: 2009-08-11 16:16:52