Prospects of higher-order Laguerre Gauss modes in future gravitational wave detectors

PRD/v74/e082003. [8] M. Bondarescu, O. Kogan, and Y. Chen, Physical Review D (Particles, Fields, Gravitation, and Cosmology)78, 082002 (2008), URL http://link.aps.org/doi/10. 1103/PhysRevD.78.082002. [9] B. Mours, E. Tournefier, and J.-Y. Vinet, Classical and Quantum Gravity 23, 5777 (2006). [10] H. He, M. E. J. Friese, N. R. Heckenberg, andH. Rubinsztein-Dunlop, Phys. Rev. Lett. 75, 826 (1995). [11] K. Bongs, S. Burger, S. Dettmer, D. Hellweg, J. Arlt, W. Ertmer, and K. Sengstock, Phys. Rev. A 63, 031602 (2001).[12] J. Arlt, K. Dholakia, L. Allen, and M. J. Padgett, Journal of Modern Optics 45, 1231 (1998). [13] M. A. Clifford, J. Arlt, J. Courtial, and K. Dholakia, Optics Communications 156, 300 (1998). [14] S. A. Kennedy, M. J. Szabo, H. Teslow, J. Z. Porterfield,and E. R. Abraham, Phys. Rev. A 66, 043801 (2002). [15] J. Courtial and M. J. Padgett, Optics Communications159, 13 (1999).[16] A. T. O’Neil and J. Courtial, Optics Communications181, 35 (2000). [17] S.-C. Chu and K. Otsuka, Optics Communications 281,