Please wait a minute...
Acta Physica Sinica (Overseas Edition), 1997, Vol. 6(3): 161-171    DOI: 10.1088/1004-423X/6/3/001
GENERAL   Next  

HIGH FREQUENCY GRAVITATIONAL WAVE OF A COMPOSITE TOROIDAL ELECTROMAGNETIC RESONANT SYSTEM

TANG MENG-XI (唐孟希)a, LI FANG-YU (李芳昱)b, LUO JUN (罗俊)c
a Department of Physics, Zhongshan University, Guangzhou 510275, China;
b Department of Physics, Chongqing University, Chongqing 630044, China; 
c Center for Gravitational Experiment, Huazhong University of Science and Technology, Wuhan 430074, China
Abstract  Starting with the Einstein equation of weak gravitational field, a new scheme of generating high frequency gravitational wave by composite toroidal electromagnetic resonant system is discussed. The system is a composite toroidal electromagnetic resonant cavity consisting of a vacuum and a dielectric regions. In the focal region of the cavity under the condition of allowable ohmic losses in the cavity walls, the amplitude of the standing gravitational wave is almost two orders of magnitude higher than that in usual cavity with the same volume. A concrete numerical calculation shows that a composite toroidal electromagnetic resonant system with a volume 2×108cm3 could generate the standing gravitational wave with an amplitude h=10-33, wavelength $\lambda$= 40 cm in its focal region. This is comparable to the typical order of magnitude of several astrophysical sources, and it would be displayed by electromagnetic detection due to very high frequency.
Received:  08 April 1996      Accepted manuscript online: 
PACS:  04.30.-w (Gravitational waves)  
  04.20.Gz (Spacetime topology, causal structure, spinor structure)  
Fund: Project supported by the National Natural Science Founation of China.

Cite this article: 

TANG MENG-XI (唐孟希), LI FANG-YU (李芳昱), LUO JUN (罗俊) HIGH FREQUENCY GRAVITATIONAL WAVE OF A COMPOSITE TOROIDAL ELECTROMAGNETIC RESONANT SYSTEM 1997 Acta Physica Sinica (Overseas Edition) 6 161

[1] Simulation of the gravitational wave frequency distribution of neutron star-black hole mergers
Jianwei Zhang(张见微), Chengmin Zhang(张承民), Di Li(李菂), Xianghan Cui(崔翔翰), Wuming Yang(杨伍明), Dehua Wang(王德华), Yiyan Yang(杨佚沿), Shaolan Bi(毕少兰), and Xianfei Zhang(张先飞). Chin. Phys. B, 2021, 30(12): 120401.
[2] Gravitational collapse with standard and dark energy in the teleparallel equivalent of general relativity
Gamal G. L. Nashed . Chin. Phys. B, 2012, 21(6): 060401.
[3] Gravitational waves from the axial perturbations of hyperon stars
Wen De-Hua(文德华), Yan Jing(燕晶), and Liu Xue-Mei(刘雪梅) . Chin. Phys. B, 2012, 21(6): 060402.
[4] Impact of neutron star crust on gravitational waves from the axial  w-modes
Wen De-Hua(文德华), Fu Hong-Yang(付宏洋), and Chen Wei(陈伟). Chin. Phys. B, 2011, 20(6): 060402.
[5] Determining the long living quasi-normal modes of relativistic stars
Lü Jun-Li(吕君丽) and Suen Wai-Mo(孙纬武) . Chin. Phys. B, 2011, 20(4): 040401.
[6] Gravitational radiation fields in teleparallel equivalent of general relativity and their energies
Gamal G.L. Nashed. Chin. Phys. B, 2010, 19(11): 110402.
[7] A POSSIBLE EXPERIMENTAL TEST ON THE GRAVITATION THEORY OF COMPLEX FIELD
Tang Zhi-ming (唐智明). Chin. Phys. B, 2000, 9(12): 881-884.
[8] POSITIVE DEFINITE PROBLEM OF ENERGY DENSITY AND RADIATIVE ENERGY FLUX FOR PULSE CYLINDRICAL GRAVITATIONAL WAVE
LI FANG-YU (李芳昱), TANG MENG-XI (唐孟希). Chin. Phys. B, 1997, 6(5): 321-333.
No Suggested Reading articles found!