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31 May 2024: 6. Black Holes. Black holes are among the most enigmatic objects in the universe. They are described. by deceptively simple solutions to the Einstein equations, yet hold a host of insights. and surprises, from the meaning of causal structure, to

26 Jun 2024: integral as. n 4. (2)3 eµ. Z 1. 0. dp p2ep2/2m =. mkBT. 22. 3/2eµ (2.24). Let’s try to interpret this. Read naively, it seems to tell ... anti-aligned to give 3 dierent spin 1 states. With these two amendments, our expression for the number density (2

26 Jun 2024: 0 for all S(r) and R(r) (4.24). This is clearly satisfied if R and S are finite at the origin.

26 Jun 2024: Tr T ART BR. =1. 2I(R)AB. (4.24). The Dynkin index is related to the quadratic Casimir C(R), which we previously defined.

31 May 2024: should identify. g00(x) (1. 2Φ(x). c2. )(1.24). where Φ(x) is the Newtonian gravitational field. ... 1.24) but with a linear gravitational potential Φ of the kind that we would invoke for.

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.

18 Jun 2024: 𝑒𝑗 𝑒𝑗1. 𝑈 =. Back to the shift! ෍. 24. 0 1. ... Slide 24: Back to the shift! Slide 25: Back to the shift!

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: where. Kµ = µtr. A@A. 2i. 3AAA. (2.24). This means that, as in the Maxwell case, the theta term does not change the. ... derivative (2.24), the temporal component was K0 = 42W. For now, the key property of W(A) that we will need is.

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: p. Figure 24:. to be conserved if we deform the theory, provided that both. ... not Grassmann-valued) four-component spinors n satisfying. i /Dn = nn (3.24).

12 Jun 2024: 1.3.3 An Application: Work and Potential Energy 24. 1.3.4 A Subtlety 25. ... 24 –. We learn that a conservative force, one that can be written as (1.18), has a conserved.

26 Jun 2024: V (r) =g2s. 4rT AcaT? Adb. (3.24). – 99 –. We’ve still got those colour indices to deal with. ... the result (3.24).) Consider the operator. SA = T A(R1) 1 1 T A(R2).

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.

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.

31 May 2024: They solvedtheir lubrication equations (24)–(32), again by an expansion in a small Deborah numberWe 1, going to the first correction. ... p/. (1. c). p 1. De. H = 21/22. 23/24. Figure 1.

31 May 2024: S T)µ1.µp1.r1.q1.s. = Sµ1.µp1.qT1.r. 1.s (2.24). Given an (r, s) tensor T , we can also construct a tensor of lower rank (r

26 Jun 2024: 1.24). This is our starting point: representations of the Poincaré group are labelled by the.

26 Jun 2024: proportional to. eVScl! 0 as V! 1. (2.24). It’s obvious what’s going on here.