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  2. 5 Phase Transitions‣ Statistical Physics by David Tong

    www.damtp.cam.ac.uk/user/tong/statphys/statmechhtml/S5.html
    18 Oct 2021: 5 Phase Transitions. 5 Phase Transitions. A phase transition is an abrupt, discontinuous change in the properties of a system. We’ve already seen one example of a phase transition in our discussion of Bose-Einstein condensation. In that case, we
  3. Turing’s Diffusive Threshold in Random Reaction-Diffusion Systems

    www.damtp.cam.ac.uk/user/gold/pdfs/turing.pdf
    9 Jun 2021: activator” [24,25], the com-plicated instability conditions for N > 2 [26] do not lendthemselves to analytical progress.Here, we analyze the diffusive threshold for Turing. ... Natl. Acad. Sci. U.S.A.115, 6572 (2018). [24] A. J. Koch and H.
  4. 5. When Gravity is Weak The elegance of the ...

    www.damtp.cam.ac.uk/user/tong/gr/five.pdf
    25 Feb 2021: 1 1. 2He. i!t. (5.24). where, as we mentioned previously, we should take the real part of the right-hand-side. ... S1(0)2 S2(0)2 = R2. The solutions (5.24) tell us how these geodesics evolve.
  5. 8 Jul 2021: B. Microsphere motion. The dynamics of a microsphere forced by an optical trap whose position is laterally oscillated isa well-studied problem [24]. ... Phys. 1, 28 (2018).[24] K. C. Neuman and S. M. Block, Optical trapping, Rev.
  6. 27 May 2021: B. Microsphere motion. The dynamics of a microsphere forced by an optical trap whose position is laterally oscillated isa well-studied problem [24]. ... Phys. 1, 28 (2018).[24] K. C. Neuman and S. M. Block, Optical trapping, Rev.
  7. justaqm

    www.damtp.cam.ac.uk/user/tong/aqm/justsix.pdf
    7 Apr 2021: qg = 2n with n 2 Z (6.24). This is the famous Dirac quantisation condition. ... In this. case, it’s sucient to impose the Dirac quantisation condition (6.24) where q is the.
  8. 5. Discrete Symmetries In this section, we discuss the ...

    www.damtp.cam.ac.uk/user/tong/aqm/aqmfive.pdf
    25 Aug 2021: L1 = L (5.24). – 137 –. We can also see how it acts on states. ... 5.24). S1 = S (5.26). For a spin- 12 particle, we have S =2 with the vector of Pauli matrices.
  9. dynrel

    www.damtp.cam.ac.uk/user/tong/relativity/two.pdf
    12 Jun 2021: perpendicular to B. In the last line, we’ve used the equation (2.24). ... oscillating with frequency! = qB/m. However, because of the constraint (2.24), the.
  10. Hydrodynamic synchronization in strong confinement

    www.damtp.cam.ac.uk/user/lauga/papers/187.pdf
    8 Jul 2021: Since all the prefactors in Eq. (24), including r2and 〈y1, y2〉, are positive numbers, the phase difference (2)0 isthe linearly stable solution to Eq. ... 24) is not entirelyequivalent to the Adler’s equation. It is important to note thatboth r2 and.
  11. 3 The Strong Force In the middle of the ...

    www.damtp.cam.ac.uk/user/tong/pp/pp3.pdf
    23 Apr 2021: 3 The Strong Force. In the middle of the 20th century, the number of seemingly “fundamental” particles. exploded. The electron, proton and neutron had long been known. These were joined,. in 1947, by a new particle called the pion, whose role

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