2014
DOI: 10.1007/s11433-014-5560-8
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Some statistical correlation analyses for Fermi/LAT Blazars

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Cited by 7 publications
(5 citation statements)
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“…Under the same conditions, we have also studied the acoustomechanical and mechanical entanglement considering multiple flexural modes. Large acoustomechanical entanglement can be achieved for single or multimode case, confirming previous results that indicated that vacuum forces enable steady-state acoustomechanical entanglement [17]. On the other hand, we demonstrated that the mechanical entanglement is very fragile and strongly depends on ϑ (N ) .…”
Section: Discussionsupporting
confidence: 90%
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“…Under the same conditions, we have also studied the acoustomechanical and mechanical entanglement considering multiple flexural modes. Large acoustomechanical entanglement can be achieved for single or multimode case, confirming previous results that indicated that vacuum forces enable steady-state acoustomechanical entanglement [17]. On the other hand, we demonstrated that the mechanical entanglement is very fragile and strongly depends on ϑ (N ) .…”
Section: Discussionsupporting
confidence: 90%
“…Ground-state cooling and large steady-state acoutomechanical entanglement, E N ≈ 5, is shown to be possible via Casimir-Polder interactions, in agreement with ref. [17].…”
Section: Acoustomechanical Entanglement In a Single Mode Membranementioning
confidence: 99%
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“…Through the log-parabolic model fitting, 12 fitting parameters can be obtained as β syn , β ic , log ν syn peak , log ν ic peak , log L syn peak , log L ic peak , and the spectral index α ν of each band: the radio (1.4 GHz), infrared (2.2 µm), optical (J band, 1250 nm), ultraviolet (250 nm), soft X-ray (1 keV) and γ-ray (20 GeV) bands (Fossati et al 1998;Nie et al 2014;Yang et al 2017). We can also calculate the physical parameters indirectly, including D, R, B and γ p .…”
Section: The Intrinsic Physical Parametersmentioning
confidence: 99%
“…We can also calculate the physical parameters indirectly, including D, R, B and γ p . In addition, we can calculate the γ-ray luminosity at E = 20 GeV by the following formula (Fan et al 2012(Fan et al , 2015Nie et al 2014;Yang et al 2017):…”
Section: The Intrinsic Physical Parametersmentioning
confidence: 99%