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3421“…Pulsar Timing Arrays (PTAs) have reported evidence for a stochastic gravitational wave (GW) background at nHz frequencies, possibly originating in the early Universe. …”
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3422por Cai, Jinchi, Li, Wei, Su, Zixuan, Xu, Jin, Yue, Linna, Yin, Hairong, Yin, Pengcheng, Zhao, Guoqing, Wang, Wenxiang, Wei, Yanyu, Syratchev, Igor, Burt, Graeme“…Nevertheless, Standing wave (SW) mode pattern is prerequisite condition in the beam-wave interaction analysis in well-established KlyC large signal simulations. …”
Publicado 2023
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Enlace del recurso
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3423por Huseynzade, Elina“…As the titles of the projects indicate, the first project focuses on the investigation of Mach shock waves, which are basically a type of pressure wave that propagates at the speed of sound within a compressible flow. …”
Publicado 2023
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3424por Alvey, James, Bhardwaj, Uddipta, Domcke, Valerie, Pieroni, Mauro, Weniger, Christoph“…The next generation of space- and ground-based facilities promise to reveal an entirely new picture of the gravitational wave sky: thousands of galactic and extragalactic binary signals, as well as stochastic gravitational wave backgrounds (SGWBs) of unresolved astrophysical and possibly cosmological signals. …”
Publicado 2023
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3425“…Several modified gravity theories predict a possible time variation of the propagation speed of gravitational waves (GW) which could be tested with multimessenger astronomy. …”
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3426
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3427
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3428
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3429
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3430
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3431
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3432
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3433
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3434
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3435por Amelino-Camelia, G., Ellis, John R., Mavromatos, N.E., Nanopoulos, Dimitri V., Sarkar, Subir“…In particular, the fine-scale time structure and hard spectra of GRB emissions are very sensitive to dispersion of electromagnetic waves in vacuo: $\delta v\sim E/E_{\QG}$, a possibility suggested in some approaches to quantum gravity. …”
Publicado 1997
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Enlace del recurso
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3436
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3437
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3438
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3439
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3440