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1 - 10 of 15 search results for KA :PC53 |u:www.damtp.cam.ac.uk where 0 match all words and 15 match some words.

  1. Results that match 1 of 2 words

  2. 2 Hilbert Space The realm of Quantum Mechanics is ...

    www.damtp.cam.ac.uk/user/dbs26/PQM/chap2.pdf
    8 Oct 2021: kA| ik  M k| ik for some fixed M > 0.

  3. Preprint typeset in JHEP style - HYPER VERSION Lent ...

    www.damtp.cam.ac.uk/user/tong/aqm/justaqm.pdf
    25 Aug 2021: q. kA(eiqa/2 eiqa/2). Notice that only the combination (r t) appears.

  4. The bank of swimming organisms at the micron scale (BOSO-Micro)

    www.damtp.cam.ac.uk/user/lauga/papers/195.pdf
    8 Jul 2021: RESEARCH ARTICLE. The bank of swimming organisms at the. micron scale (BOSO-Micro). Marcos F. Velho Rodrigues1, Maciej LisickiID2, Eric Lauga1. 1 Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge, United.

  5. justaqm

    www.damtp.cam.ac.uk/user/tong/aqm/justone.pdf
    23 Apr 2021: q. kA(eiqa/2 eiqa/2). Notice that only the combination (r t) appears.

  6. Preprint typeset in JHEP style - HYPER VERSION Statistical ...

    www.damtp.cam.ac.uk/user/tong/statphys/sp.pdf
    17 Apr 2021: Preprint typeset in JHEP style - HYPER VERSION. Statistical PhysicsUniversity of Cambridge Part II Mathematical Tripos. David Tong. Department of Applied Mathematics and Theoretical Physics,. Centre for Mathematical Sciences,. Wilberforce Road,.

  7. Lecture Notes on Cosmological Soft Theorems Enrico Pajera aDepartment …

    www.damtp.cam.ac.uk/user/ep551/notes_cosmo_soft_theorems.pdf
    16 Apr 2021: na=1. La〈O(k1)O(k2). O(kn)〉 = 0 , (1.1). where La = L(τa,τa, ka,ka) is some linear, possibly differential operator made of func-. ... Then (4.26) becomes[. 3(n 1) na=1. ka. ka. ]〈R(k1)R(k2). R(kn)〉′! = 0 , (4.38).

  8. Field Theory in Cosmology: Example Sheet 1 1. For ...

    www.damtp.cam.ac.uk/user/ep551/example_sheet_1_FT_in_Cosmo.pdf
    15 Apr 2021: φ(k1). φ(kn)〉 δ3D. (na=1. ka. ). (19). 7. For the metric. ... φ(k1). φ(kn)〉 = (2π)3δ3D. (na=1. ka. )Bn(k1,. ,kn). (34). must scale as.

  9. Field Theory in Cosmology (Part III) Enrico Pajer Contents ...

    www.damtp.cam.ac.uk/user/ep551/field_theory_in_Cosmology.pdf
    15 Apr 2021: Field Theory in Cosmology (Part III). Enrico Pajer. Contents. 1 A quick review of background cosmology 51.1 Classical cosmological backgrounds. 51.2 Motivations for Inflation. 101.3 A prolonged phase of quasi-de Sitter expansion. 151.4 Single field

  10. solidstate

    www.damtp.cam.ac.uk/user/tong/aqm/solid4.pdf
    7 Apr 2021: m!2 = 2 eika eika. = 4sin2. ka. 2. We find the dispersion relation! = ... 2 =. mM. hm M. p(m M)2 4mM cos2(ka). i. The resulting dispersion relation is sketched in Figure 64 in the first Brillouin zone.

  11. justaqm

    www.damtp.cam.ac.uk/user/tong/aqm/justfive.pdf
    7 Apr 2021: m!2 = 2 eika eika. = 4sin2. ka. 2. We find the dispersion relation! = ... 2 =. mM. hm M. p(m M)2 4mM cos2(ka). i. The resulting dispersion relation is sketched in Figure 74 in the first Brillouin zone.

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