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George Efstathiou's Home Page
https://people.ast.cam.ac.uk/~gpe/17 Oct 2013: Professor Efstathiou has received several prizes for his research including the 1990 Maxwell Medal and Prize of the Institute of Physics, the 1990 Vainu Bappu Prize of the Astronomical Society of -
Other WWW pages
https://people.ast.cam.ac.uk/~optics/www/otherwww.htm16 Jun 2015: [Local pages. Telescope projects. Observatories/Departments. There is a comprehensive list of observatories maintained by the RGO. ESO On-Line Information System. Instrumentation Groups. Detectors. Software Applications/Packages. FITS. URL http://www -
Educational and Outreach talks and activities for Carolin Crawford ...
https://people.ast.cam.ac.uk/~csc/newcv/2014talks.html24 Jul 2019: Nov. 90. Dark energy and the ever-expanding Universe. Maxwell Society lecture, King's London. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_10.pdf22 Oct 2017: Reaction Rate for Fusion. We have the velocity in terms of the particle energies already and the distribution of particle energies is given by the Maxwell-Boltzmann distribution:. ... Substitute expression for cross-section into equation for the -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_03.pdf9 Oct 2017: Atoms, mass m, in thermal equilibrium in stellar atmosphere. • Random motion obeying Maxwell-Boltzmann distribution, most probable speed vmp =(2kT/m)1/2. • ... Velocity, v, from the Maxwell-Boltzmann distribution, vmp = (2kT/m)1/2 , and. • -
probs1.dvi
https://people.ast.cam.ac.uk/~gpe/paprobs1.pdf21 Feb 2011: p e H γ. Assume that the particle densities are given by the non-relativistic Maxwell-Boltzmann formula. -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture07.pdf23 Oct 2023: We obtain this by recalling that thedistribution of particle velocities as a function of T is given by the Maxwell-Boltzmann distribution:. ... With the Maxwell-Boltzmann distribution in energy terms:. nE dE =2n. π1/21. -
Mark Wyatt
https://people.ast.cam.ac.uk/~wyatt/15 Apr 2024: The optical constants for these grains are added together assuming various ratios for the components using Maxwell-Garnett effective medium theory. -
Domain walls, cosmic strings and monopoles, dark matter ...
https://people.ast.cam.ac.uk/~gpe/Astroparticle_11.pdf27 Feb 2012: No evidence seen so far - still agree with Maxwell! But monopoles arise naturally in GUTs and other theories based on large gauge groups! -
L93 The Astrophysical Journal, 570:L93–L96, 2002 May 10 �� ...
https://people.ast.cam.ac.uk/~wyatt/jhkg02.pdf19 Apr 2006: Our 850 mm map, obtained with the Submillimeter Common-UserBolometric Array on the James Clerk Maxwell Telescope, shows three peaks of emission at the 2.5 mJy levelin the vicinity of -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture12.pdf17 Nov 2020: the lowest momentum state, in accord with the 1-D Maxwell-Boltzmanndistribution:. P(px) dpx =(. 1. 2π mkT. )1/2exp. p2x2mkT. dpx (12.9)shown on the right side ... The normal Maxwell-Boltzmann distribution of protonenergies serves to define -
SUBMILLIMETER OBSERVATIONS OF AN ASYMMETRIC DUST DISK AROUND…
https://people.ast.cam.ac.uk/~wyatt/hgdw03.pdf19 Apr 2006: 1999) wasused on the James Clerk Maxwell Telescope (JCMT) toobtain deep simultaneous images of Fomalhaut at wave-lengths of 450 and 850 lm. -
M. Pettini: Introduction to Cosmology — Lecture 9 RECOMBINATION ...
https://people.ast.cam.ac.uk/~pettini/Intro%20Cosmology/Lecture09.pdf6 Nov 2018: In statistical equilibrium at temperature T,the number density nx of particles with mass mx is given by the Maxwell-Boltzmann equation:. -
mnr7957.tex
https://people.ast.cam.ac.uk/~wyatt/gwhd04.pdf19 Apr 2006: 1999) at the James Clerk Maxwell Telescope wasused to observe τ Ceti in 2001 September and November, for a totalintegration time of 13.3 h. -
Debris discs around nearby solar analogues
https://people.ast.cam.ac.uk/~wyatt/gwb09.pdf8 Jul 2009: 2 S U RV E Y D ATA. The SCUBA camera on the 15 m James Clerk Maxwell Telescope(JCMT) was used to survey G-dwarf (luminosity class V or -
arX iv:a stro -ph/ 0311 593 v1 26 N ...
https://people.ast.cam.ac.uk/~wyatt/sdw04.pdf19 Apr 2006: 2 OBSERVATIONS. Sub-mm observations were made using the SCUBA bolome-ter array on the James Clerk Maxwell Telescope. ... Details of Maxwell-Garneteffective medium theory, and the methods used to calculateabsorption efficiencies are discussed in Bohren & -
M. Pettini: Structure and Evolution of Stars — Lecture ...
https://people.ast.cam.ac.uk/~pettini/Stellar%20Structure%20Evolution/Lecture05.pdf13 Oct 2014: 3.4);. 4. The kinetic temperature, defined by the Maxwell-Botzmann distribu-tion:. nv dv = n. -
842 Publications of the Astronomical Society of the Pacific, ...
https://people.ast.cam.ac.uk/~wyatt/mghw07.pdf18 Sep 2007: ABSTRACT. We present the scientific motivation and observing plan for an upcoming detection survey fordebris disks using the James Clerk Maxwell Telescope. ... SCUBA-2 (Holland et al. 2006) is a new submillimeter cam-era arriving at the James Clerk -
Mon. Not. R. Astron. Soc. 000, 1–8 (2016) Printed ...
https://people.ast.cam.ac.uk/~wyatt/ghmm16.pdf21 Jul 2016: The James Clerk Maxwell Telescope is operated by the EastAsian Observatory on behalf of The National Astronomical Ob-servatory of Japan, Academia Sinica Institute of Astronomy andAstrophysics, the Korea Astronomy and -
arX iv:2 110. 0431 9v1 [as tro- ph.E P] ...
https://people.ast.cam.ac.uk/~wyatt/wyat21.pdf12 Oct 2021: Fitzgerald, Maxwell A. Millar-Blanchaer, GaspardDuchêne, Jennifer Patience, Justin Hom, Marshall D.
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