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17 Jun 2019: tan(ka δ0). ka=. tan κa. κa,. where κ2 = k 2 γ 2. ... Part II, Paper 2 [TURN OVER. 22. 36B General Relativity. A vector field ka which satisfies.

17 Jun 2019: Sketch the ground state energy eigenfunction χ(x) and show that its energy isE =. 2k2. 2m , where k satisfies. tan ka = k2mV0. 2 k2.

17 Jun 2019: MATHEMATICAL TRIPOS Part II 2003. List of Courses. Geometry of SurfacesGraph TheoryNumber TheoryCoding and CryptographyAlgorithms and NetworksComputational Statistics and Statistical ModellingQuantum PhysicsStatistical Physics and

17 Jun 2019: MATHEMATICAL TRIPOS Part II 2004. List of Courses. Geometry of SurfacesGraph TheoryNumber TheoryCoding and CryptographyAlgorithms and NetworksComputational Statistics and Statistical ModellingQuantum PhysicsStatistical Physics and

17 Jun 2019: tanh (κa). κa=. tan (ka δ0). ka. where κ2 = γ2 k2.

17 Jun 2019: E =12(E0 E1 4A cos ka). 12. (E0 E1)2 16A2 cos2 ka.

17 Jun 2019: ka = i log(t. rr′. ). Part II, 2013 List of Questions [TURN OVER.

17 Jun 2019: By considering the s-wave solution to the Schrödinger equation,. show thattan(ka δ0). ... ka=. tanh(γ2 k2a). γ2 k2a. For low momenta, ka 1, compute the s-wave contribution to the total cross-section.Comment on the physical interpretation of your

30 Aug 2019: b) When ka 1, approximate the dispersion relation by. D(k, ω) D approx(k, ω) 2ω 2ka 2k2a2.

30 Aug 2019: MATHEMATICAL TRIPOS Part III. Wednesday, 8 June, 2011 9:00 am to 12:00 pm. PAPER 53. COSMOLOGY. Attempt no more than THREE questions. There are FOUR questions in total. The questions carry equal weight. STATIONERY REQUIREMENTS SPECIAL REQUIREMENTS.