Bumblebee models

Bumblebee models are effective field theories describing a vector field with a vacuum expectation value that spontaneously breaks Lorentz symmetry.[1][2][3][4] A bumblebee model is the simplest case of a theory with spontaneous Lorentz symmetry breaking.[5]

The development of bumblebee models was motivated primarily by the discovery that mechanisms in string theory (and subsequently other quantum theories of gravity) can lead to tensor-valued fields acquiring vacuum expectation values.[6] Bumblebee models are different from local U(1) gauge theories. Nevertheless, in some bumblebee models, massless modes that behave like photons can appear.

  1. ^ Kostelecký, V. Alan; Samuel, S. (1989). "Gravitational phenomenology in higher-dimensional theories and strings". Physical Review D. 40 (6): 1886–1903. Bibcode:1989PhRvD..40.1886K. doi:10.1103/PhysRevD.40.1886. hdl:2022/18652. PMID 10012017.
  2. ^ Kostelecký, V. Alan; Lehnert, Ralf (2001). "Stability, causality, and Lorentz and CPT violation". Physical Review D. 63 (6): 065008. arXiv:hep-th/0012060. Bibcode:2001PhRvD..63f5008K. doi:10.1103/PhysRevD.63.065008. S2CID 119074843.
  3. ^ Kostelecký, V. Alan (2004). "Gravity, Lorentz violation, and the standard model". Physical Review D. 69 (10): 105009. arXiv:hep-th/0312310. Bibcode:2004PhRvD..69j5009K. doi:10.1103/PhysRevD.69.105009. S2CID 55185765.
  4. ^ Bailey, Quentin; Kostelecký, V. Alan (2006). "Signals for Lorentz violation in post-Newtonian gravity". Physical Review D. 74 (4): 045001. arXiv:gr-qc/0603030. Bibcode:2006PhRvD..74d5001B. doi:10.1103/PhysRevD.74.045001. S2CID 26268407.
  5. ^ Bluhm, R. (2008). "Nambu-Goldstone modes in gravitational theories with spontaneous Lorentz breaking". International Journal of Modern Physics D. 16 (12b): 2357–2363. arXiv:hep-th/0607127. Bibcode:2007IJMPD..16.2357B. doi:10.1142/S021827180701122X. S2CID 12186967.
  6. ^ Kostelecký, V. Alan; Samuel, Stuart (1989). "Spontaneous breaking of Lorentz symmetry in string theory". Physical Review D. 39 (2): 683–685. Bibcode:1989PhRvD..39..683K. doi:10.1103/PhysRevD.39.683. hdl:2022/18649. PMID 9959689.

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