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.0708. [9] A. De Simone. M. P. Hertzberg. and F. Wilczek. Phys.Lett. B678. 1 (2009). arXiv:0812.4946. [1
S. R. Coleman and E. J. Weinberg, Phys.Rev. D7. 1888 (1973). [50] D. I. Kaiser. Phys.Rev. D81.084044 (2010), arXiv:1003.1159. 151] L. M. Krauss and E Wilczek. Phys.Rev. D89. 047501 (2014). arXiv:1309.5343. [52] B. M. Kastening. Phys.Lett. 11283, 287 (1992). [53] M. Bando. T Kugo, N. Maekawa. and H. Naka
Prokopec and J. Weenink, (2014), arXiv:1403.3219. [261 D. Donau° a at, (2013). arXiv:1307.3536. [27] S. Weinberg, Phys.Rev. D7, 2887 (1973). [28] R. Jackiw, Phys. Rev. 139. 1686(1974). [29] L. Dolan and R. Jackiw, Phys.Rev. 139, 2904 (1974). (A10) 1301 J. Kang, Phys.Rev. DIO, 3455 (1974). [311 N. K.
Some examples of brandied Hamiltonians were explored both classically and in the context of quan- tum mechanics, as recently advocated by Shapere and Wilczek. These are in fact cases of switch- back potentials, albeit in momentum space, as previously analyzed by us for quasi-Hamiltonian chaotic dynamical
Physics 10 (1974) 363-384. [54] L. Iorio, "Constraints on Galileon-induced precessions from solar system orbital motions" JCAP 07 (2012) 001 [55] R. Jackiw and S.-Y. Pi, "Tutorial on Scale and Conformal Symmetries in Diverse Dimensions" 3. Phys. A44 (2011) 223001, arXiv:1101.4886 [math-ph], and referenc
S. R. Coleman and E. J. Weinberg, Phys.Rev. D7, 1888 (1973). 50] D. I. Kaiser. Phys.Rev. D81, 084044 (2010), arXiv:1003.1159. 51] L. M. Krauss and F Wilczek, Phys.Rev. D89. 047501 (2014), arXiv:1309.5343. 52] B. M. Kastening. Phys.Lett. B283. 287 (1992). 53] M. Bando. T. Kugo, N. Maekawa. and H. Nakano
okopec and J. Weenink, (2014), arXiv:1403.3219. [26] D. Buttaz2o er at, (2013), arXiv:1307.3536. [27] S. Weinberg, Phys.Rev. D7, 2887 (1973). [28] R. Jackiw. Phys. Rev. D9, 1686 (1974). [29] L. Dolan and R. Jackiw, Phys.Rev. D9. 2904 (1974). 30] J. Kang. Phys.Rev. D10, 3455 (1974). 31] N. K. Nielsen, N
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