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31 May 2024: 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.

31 May 2024: ṙ2 Ve(r) = E2 (4.24). but this time with the eective potential. ... This tells us that the particle follows a null geodesic. The equation (4.24) gets replaced.

26 Jun 2024: in (1.24) because E = (0,0,E) lies parallel to the side of the torus, not perpendicular. ... Instead, both (1.23) and (1.24) are best thought of as integrating the 2-form Fµν over.

26 Jun 2024: Instead, both (1.23) and (1.24) are best thought of as integrating the 2-form Fµ over. ... Armed with (1.23) and (1.24), we see that, at least for this specific example,.

26 Jun 2024: 4.24). with @ = @t @x. The equations of motion tell us @ = @ = 0. ... moving fermion. The chiral symmetry of the action (4.24) means that the left- and right-handed.

26 Jun 2024: group, means that the theory admits fluxes (8.24) and gauge transformations (8.25). ... a derivative of the Chern-Simons term (2.24). (It also arose in the same context when.

26 Jun 2024: 1. ar v̇ = Ḣ. 1. arv̇. Take the gradient of (3.24) to get. ... 1.24). In such a situation, it would make little sense to talk about perturbations with.

31 May 2024: 1.4.1 The Metric on the Higgs Branch 23. 1.4.2 Constructing the Solutions 24. ... in 5 1 dimensions is a sigma-model on a hyperKähler target space [24] which, for.

26 Jun 2024: 4i. 1 log. i. 2UV. iv2. (7.24). where, to reach the second line, we’ve Taylor expanded in /2UV. , ... 2. This is the same kind of integral that we met in (7.24) when solving the 2d CPN1.

10 Jun 2024: Slide 24: Spectral measures goes to diagonalisation. Slide 25: Spectral measures goes to dynamics.