- Access by Xinjiang University
Electromagnetic response produced by interaction of high-frequency gravitational waves from braneworld with galactic-extragalactic magnetic fields
Phys. Rev. D 89, 104025 – Published 14 May, 2014
DOI: https://doi.org/10.1103/PhysRevD.89.104025
Abstract
Braneworld scenarios predict very strong high-frequency gravitational waves (HFGWs) in the GHz to THz band. The observation of such HFGWs would provide dynamical evidence for an extra dimension of space. In this paper, we for the first time analytically calculate the electromagnetic (EM) response to HFGWs via the interaction of the HFGWs from the braneworld with the galactic-extragalactic magnetic fields appearing in all galaxies and galaxy clusters, which would give rise to a significant spatial accumulation effect (caused by the synchro-propagation of the HFGWs and perturbed EM waves) and lead to possibly detectable EM signals. Our results show that the power of EM signals at the Earth can theoretically reach to with parameters in the typical range expected by contemporary studies and observations (from the lower values for the HFGW amplitude at and the galactic magnetic field , to the higher values of at and ), and the estimated upper bound of these signals may surpass the minimum level detectable by current technology.
Article Text
References (49)
- S. S. Seahra, C. Clarkson, and R. Maartens, Phys. Rev. Lett. 94, 121302 (2005).
- C. Clarkson and S. S. Seahra, Classical Quantum Gravity 24, F33 (2007).
- A. Chamblin, S. W. Hawking, and H. S. Reall, Phys. Rev. D 61, 065007 (2000).
- J. Garriga and M. Sasaki, Phys. Rev. D 62, 043523 (2000).
- S. S. Seahra, Phys. Rev. D 72, 066002 (2005).
- J. Garriga and T. Tanaka, Phys. Rev. Lett. 84, 2778 (2000).
- M. Cvetič, G. Shiu, and A. M. Uranga, Phys. Rev. Lett. 87, 201801 (2001).
- V. Frolov and D. Stojković, Phys. Rev. Lett. 89, 151302 (2002).
- J. A. R. Cembranos, A. Dobado, and A. L. Maroto, Phys. Rev. Lett. 90, 241301 (2003).
- C. Germani and C. F. Sopuerta, Phys. Rev. Lett. 88, 231101 (2002).
- G. W. Gibbons, H. Lü, and C. N. Pope, Phys. Rev. Lett. 94, 131602 (2005).
- A. M. Cruise, Classical Quantum Gravity 17, 2525 (2000).
- A. M. Cruise and R. M. J. Ingley, Classical Quantum Gravity 22, S479 (2005).
- R. Ballantini et al., arXiv:gr-qc/0502054.
- R. Ballantini, Ph. Bernard, E. Chiaveri, A. Chincarini, G. Gemme, R. Losito, R. Parodi, and E. Picasso, Classical Quantum Gravity 20, 3505 (2003).
- A. Nishizawa et al., Phys. Rev. D 77, 022002 (2008).
- F. Y. Li, M. X. Tang, and D. P. Shi, Phys. Rev. D 67, 104008 (2003).
- F. Y. Li, R. M. L. Baker, Jr., Z. Y. Fang, G. V. Stepheson, and Z. Y. Chen, Eur. Phys. J. C 56, 407 (2008).
- M. L. Tong, Y. Zhang, and F. Y. Li, Phys. Rev. D 78, 024041 (2008).
- F. Y. Li, N. Yang, Z. Y. Fang, R. M. L. Baker, G. V. Stephenson, and H. Wen, Phys. Rev. D 80, 064013 (2009).
- R. Clive Woods et al., J. Mod. Phys. 02, 498 (2011).
- J. Li, K. Lin, F. Y. Li, and Y. H. Zhong, Gen. Relativ. Gravit. 43, 2209 (2011).
- Y. F. Tan, F. T. Wang, Z. M. Chen, Y. N. Pan, and G. L. Kuang, Supercond. Sci. Technol. 22, 025010 (2009).
- L. M. Widrow, Rev. Mod. Phys. 74, 775 (2002).
- A. Nishizawa and K. Hayama, Phys. Rev. D 88, 064005 (2013).
- D. M. Eardley, D. L. Lee, A. P. Lightman, R. V. Wagoner, and C. M. Will, Phys. Rev. Lett. 30, 884 (1973).
- C. M. Will, Living Rev. Relativity 9, 3 (2006).
- D. Boccaletti, V. De Sabbata, P. Fortint, and C. Gualdi, Nuovo Cimento B 70, 129 (1970).
- A. M. Cruise, Classical Quantum Gravity 29, 095003 (2012).
- F. Y. Li and M. X. Tang, Acta Phys. Sin. (Overseas Edn) 6, 321 (1997).
- H. Wen, F. Y. Li, Z. Y. Fang, and A. Beckwith, arXiv:1403.7277v2.
- B. P. Abbott et al., Nature (London) 460, 990 (2009).
- A. Nishizawa, A. Taruya, K. Hayama, S. Kawamura, and M.-a. Sakagami, Phys. Rev. D 79, 082002 (2009).
- M. Tinto and M. E. d. S. Alves, Phys. Rev. D 82, 122003 (2010).
- K. Hayama and A. Nishizawa, Phys. Rev. D 87, 062003 (2013).
- A. Błaut, Phys. Rev. D 85, 043005 (2012).
- A. S. Goldhaber and M. M. Nieto, Rev. Mod. Phys. 82, 939 (2010).
- E. Berti, J. Gair, and A. Sesana, Phys. Rev. D 84, 101501 (2011).
- G. D. Moore and A. E. Nelson, J. High Energy Phys. 09 (2001) 023.
- L. S. Finn and P. J. Sutton, Phys. Rev. D 65, 044022 (2002).
- G. Dvali, A. Gruzinov, and M. Zaldarriaga, Phys. Rev. D 68, 024012 (2003).
- A. Gruzinov, New Astron. 10, 311 (2005).
- K. Lee, F. A. Jenet, R. H. Price, N. Wex, and M. Kramer, Astrophys. J. 722, 1589 (2010).
- D. Baskaran, A. G. Polnarev, M. S. Pshirkov, and K. A. Postnov, Phys. Rev. D 78, 044018 (2008).
- M. Gasperini and G. Veneziano, Phys. Rep. 373, 1 (2003).
- G. Veneziano, Sci. Am. 290, 54 (2004).
- M. Giovannini, Phys. Rev. D 60, 123511 (1999).
- M. Giovannini, Classical Quantum Gravity 26, 045004 (2009).
- A. Ashoorioon, B. Fung, R. B. Mann, M. Oltean, and M. M. Sheikh-Jabbari, J. Cosmol. Astropart. Phys. 03 (2014) 020.