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1. link.aps.org › doi › 10Phys. Rev. D 48, 5594 (1993) - Evolution of cosmic string...

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   15. Dez. 1993 · Evolution of cosmic string configurations Daren Austin, E. J. Copeland, and T. W. B. Kibble Phys. Rev. D 48, 5594 – Published 15 December 1993

2. www.sciencedirect.com › science › articleSelf-intersection of cosmic strings - ScienceDirect

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   7. Okt. 1982 · Next. Volume 116B, number 2.3 PHYSICS LETTERS 7 October 1982 SELF-INTERSECTION OF COSMIC STRINGS T.W.B. KIBBLE and Neff TUROK Blackett Laboratory, Imperial College, London SW7 2BZ, England Received 16 June 1982 We discuss some aspects of the theory of Zel'dovich and Vilenkin attributing the density perturbations needed to initiate the formation ...

3. link.aps.org › doi › 10Phys. Rev. 150, 1060 (1966) - Mutual Refraction of Electrons and...

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   Mutual Refraction of Electrons and Photons T. W. B. Kibble Phys. Rev. 150, 1060 – Published 28 October 1966

4. link.aps.org › doi › 10Interaction of Intense Laser Beams with Electrons

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   Lowell S. Brown and T. W. B. Kibble Phys. Rev. 133, A705 – Published 3 February 1964. More. × . Article; References; Citing Articles (539) PDF Export Citation. Abstract Authors References. Abstract . The interaction of an intense coherent photon beam w ...

5. arxiv.org › abs › 1302[1302.3648] Causality and non-equilibrium second-order phase ...

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   14. Feb. 2013 · Causality and non-equilibrium second-order phase transitions in inhomogeneous systems. A. del Campo, T. W. B. Kibble, W. H. Zurek. When a second-order phase transition is crossed at fine rate, the evolution of the system stops being adiabatic as a result of the critical slowing down in the neighborhood of the critical point.

6. www.sciencedirect.com › science › articleSome implications of a cosmological phase transition

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   1. Dez. 1980 · (11) T. W.B. Kibble, Some implications of a cosmological phase transition 191 As pointed out by Zelovich Kobzarev and Okun [23], the existence of such walls can easily be ruled out. They are so massive even for i~ 100 GeV that just one such wall stretched across the universe would be over 108 times more massive than all other known matter. Its gravitational effect would introduce an impossibly ...

7. link.aps.org › doi › 10Global Conservation Laws and Massless Particles

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   Global Conservation Laws and Massless Particles G. S. Guralnik, C. R. Hagen, and T. W. B. Kibble Phys. Rev. Lett. 13, 585 – Published 16 November 1964 An article within the collection: Letters from the Past - A PRL Retrospective