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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.

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.

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

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

23 May 2024: 24. Residual DMD (ResDMD).

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.

18 Mar 2024: Then, using our previous result (1.24), we have. Tr (1)FeβH =X. ... 24 –. Note that we’re not assuming that all critical points of h correspond to true E = 0.

20 May 2024: Slide 23: Example: Verified spectra and modes. Slide 24: Example: Verified dictionary.

1 Apr 2024: ψ(x,y) = ψn,k(x mE/eB2,y) (1.24). and the energies are now given by. ... holomorphic and anti-holomorphic derivatives. =1. 2. (. x+ i. y. )and ̄ =. 1. 2. (. x i. y. ). – 24 –. which obey z = ̄z̄ = 1 and z̄ = ̄z = 0.

10 Jun 2024: Received 10 October 2023; revised 27 December 2023; accepted 24 February 2024). ... F(Z, ζ ) = 13ζ. Z0. H(Z̃) dZ̃. (3.25). We note that solutions (3.24) satisfy the matching conditions between theinner and outer regions.