AAWSAP DIRD, High-Frequency Gravitational Wave Communications, April 2010
DOW-UAP-D140 · page 13 of 57
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UNCLASSIFIED//&OR Oii&ICI0L Ll&li QPIL¥ Position of focused GW generated IR monomode waveguide formed by active material High power IR source Figure 3. Circular Resonator Geometry Using Infrared Excitation Analogous to Figure 2, we see in Figure 4 the radiation pattern for a pair of orbiting masses. GW I .1 GW ' Figure 4. Radiation Pattern Calculated by Landau and Lifshitz (1975) Next consider a number N of such orbit planes stacked one on top of another with the gravitational-wave (GW) radiation growing flux (Wm-2) proportional to N2 as the GW moves up the axis of the N orbit planes as in Figure 5. UNCLASSIFIED//FOP OiiiilCl.t.k l!ISI!!! l>flti 8