Zobrazeno 1 - 10
of 1 998 524
pro vyhledávání: '"Low‐Frequency"'
Autor:
Ciu, Ningcheng1,2,3 (AUTHOR), Lei, Tao1,2,3 (AUTHOR) leit@sustech.edu.cn, Zhang, Wei1,2,3 (AUTHOR) zhangwei@sustech.edu.cn
Publikováno v:
Earth & Space Science. Nov2024, Vol. 11 Issue 11, p1-27. 27p.
Autor:
Ji, Airu1,2 (AUTHOR) jiairu@buaa.edu.cn, Sun, Jinji1,2 (AUTHOR) sunjinji@buaa.edu.cn
Publikováno v:
Materials (1996-1944). Nov2024, Vol. 17 Issue 22, p5584. 9p.
This paper demonstrates numerically and experimentally that it is possible to tailor flexural band gaps in the low-frequency regime by appropriate choice of cutout characteristics. The finite element method is used to obtain the numerical dispersion
Externí odkaz:
http://arxiv.org/abs/2412.10641
Amorphous solids exhibit an excess of low-frequency vibrational modes beyond the Debye prediction, contributing to their anomalous mechanical and thermal properties. Although a $\omega^4$ power-law scaling is often proposed for the distribution of th
Externí odkaz:
http://arxiv.org/abs/2412.06475
Low-frequency radio emission from the Large Magellanic Cloud~(LMC) is assumed to be dominated by nonthermal synchrotron radiation from energy loss of energetic $e^+/e^-$ in magnetic field. Two different kinds of sources of $e^+/e^-$, dark matter~(DM)
Externí odkaz:
http://arxiv.org/abs/2412.03163
Autor:
Escott, Emmy L., Morabito, Leah K., Scholtz, Jan, Hickox, Ryan C., Harrison, Chris M., Alexander, David M., Arnaudova, Marina I., Smith, Daniel J. B., Duncan, Kenneth J., Petley, James, Kondapally, Rohit, Rivera, Gabriela Calistro, Kolwa, Sthabile
Some Active Galactic Nuclei (AGN) host outflows which have the potential to alter the host galaxy's evolution (AGN feedback). These outflows have been linked to enhanced radio emission. Here we investigate the connection between low-frequency radio e
Externí odkaz:
http://arxiv.org/abs/2411.19326
Autor:
Thyzel, Tim
The resolution of low-frequency resistance noise measurements is increased by amplitude modulation, shifting the spectrum of the resistance fluctuations away from the 1/f noise contributed by measurement instruments. However, commercial lock-in ampli
Externí odkaz:
http://arxiv.org/abs/2412.00093
The broad-band radio spectral energy distribution (SED) of star-forming galaxies (SFGs) contains a wealth of complex physics. We aim to determine the physical emission and loss processes causing radio SED curvature and steepening to see which observe
Externí odkaz:
http://arxiv.org/abs/2412.03143
Autor:
Mangu, Aashrita, Westbrook, Benjamin, Beckman, Shawn, Corbett, Lance, Crowley, Kevin T., Dutcher, Daniel, Johnson, Bradley R., Lee, Adrian T., Kabra, Varun, Prasad, Bhoomija, Staggs, Suzanne T., Suzuki, Aritoki, Wang, Yuhan, Zheng, Kaiwen
Publikováno v:
J Low Temp Phys (2024)
The Simons Observatory (SO) is a cosmic microwave background (CMB) experiment located in the Atacama Desert in Chile that will make precise temperature and polarization measurements over six spectral bands ranging from 27 to 285 GHz. Three small aper
Externí odkaz:
http://arxiv.org/abs/2412.01204