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19 Jan 2011: Department of Applied Mathematics and Theoretical Physics. Electromagnetism 1B. Lecturer: Dr Natalia Berloff. Office: CMS G1.02. E-mail: N.G.Berloff@damtp.cam.ac.uk. Lecture: Mill Lane Lecture Room 3, Tu, Thu. 11. Class web page:

20 Jan 2011: Therefore, the Maxwell equation d F = 0implies that φ is harmonic on R3 and. ... We have also found one class of examples correspondingto non-ASD Maxwell field.

11 Dec 2011: MD, Tod. Math. Proc. Cam. Phil. Soc. (2010). 2 Can you find Euclidean supersymmeries (and how many) in a givencosmological Einstein–Maxwell instanton space–time?

10 Feb 2011: Special cases. I Maxwell UCM λ2 = 0. I Newtonian λ1 = λ2. ... I a retardation time λ2. Special cases. I Maxwell UCM λ2 = 0.

28 Apr 2011: general. In Sec. V we shall consider the cosmologi-cal C metrics in Einstein-Maxwell theory. ... The C metric solves the Einstein-Maxwell equationswith the electromagnetic field edy dt, or the pureEinstein equations in the limiting case e 0.

10 Apr 2011: In order to calculate the electric contributions we need the Maxwell stresses normal to the z axis. ... Insertion of the Debye-Hiickel potential of the flat membrane, eq 4, shows that the osmotic pressure is equal to the negative Maxwell stress.

6 Jun 2011: theory by Maxwell, Boltzmann and others showed that the laws of thermodynamics. ... such as energy. Similarly, Maxwell’s theory of electromagnetism describes the motion.

10 Apr 2011: One finds from a Maxwell construction applied to eq 4.2 near the critical point that three-body interactions do indeed introduce a new energy scale, with all critical amplitudes depending

10 Apr 2011: R E S E A R C H A R T I C L E. Fluid dynamics of self-propelled microorganisms,from individuals to concentrated populations. Luis H. Cisneros Æ Ricardo Cortez ÆChristopher Dombrowski Æ Raymond E. Goldstein ÆJohn O. Kessler. Received: 13 February

10 Apr 2011: Physica D 190 (2004) 266–289. Dynamic supercoiling bifurcations of growing elastic filaments. Charles W. Wolgemutha, Raymond E. Goldsteinb, Thomas R. Powersc,a Department of Cell Biology, University of Connecticut Health Center, Farmington, CT

10 Apr 2011: Since the SN interfaces are sharp compared to the lamspacing we work with the macroscopic Maxwell equationIn the normal regions“ 3 B5 0 and“•B5 0, which can besolved by introducing

11 Jun 2011: Without these effects wecannot correctly describe, for instance, the overall torque balance, which necessarilyinvolves mean meridional circulations (MMCs) as well as Maxwell stresses. ... Bφ = Bz. z. ur. B2zdz. (4.9). For any ur profile that decays

10 Oct 2011: PART I: Symmetries and particles. NOTES BY PROF. HUGH OSBORN. Books. Books developing group theory by physicists from the perspective of particle physics are. H. F. Jones, Groups, Representations and Physics, 2nd ed., IOP Publishing (1998).A fairly

14 Jul 2011: Fundamentals of Atmosphere–OceanDynamics. M. E. McIntyre. LATEX version edited by. Björn Haßler. and. Christophe Koudella. with the kind assistance of. Teresa Cronin. and. Sarah Shea–Simonds. Version of 2007–8. ii Part , 0.0. Author’s