2016
DOI: 10.3390/e18040126
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Reply to Jay Lawrence. Comments on Piero Quarati et al. Negentropy in Many-Body Quantum Systems. Entropy 2016, 18, 63

Abstract: The Comments are explicitly related to contents of two published papers: actual [1] and [2]. A third paper [3], where the measured screening potential liquid-solid difference is explained using the correlation entropy S − , should also be considered.The mechanism described in the published paper [1] that increases the kinetic energy of light nuclei undergoing nuclear fusion, usually low energy deuterons accelerated against a host environment with implanted deuterons, does not substitute the electronic screenin… Show more

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Cited by 4 publications
(4 citation statements)
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“…The background files are generated for each spectral channel by fitting the channel separately with a second order polynomial function before the burst (T 0 − 269.1 s to T 0 − 81.1 s) and after the burst (T 0 + 230.9 s to T 0 + 798.9 s). The gain-correction is applied to those spectral files by fitting the background lines at 1.47 MeV due to 138 La in the LaBr 3 (Ce) crystal for the HXM data (Quarati et al 2012) and 2.2 MeV due to activation of the BGO crystal for the SGM data. We examined the gain-corrected spectra using the is less than ∼ 1 • .5, we used the DRM for the fixed position.…”
Section: Spectrummentioning
confidence: 99%
“…The background files are generated for each spectral channel by fitting the channel separately with a second order polynomial function before the burst (T 0 − 269.1 s to T 0 − 81.1 s) and after the burst (T 0 + 230.9 s to T 0 + 798.9 s). The gain-correction is applied to those spectral files by fitting the background lines at 1.47 MeV due to 138 La in the LaBr 3 (Ce) crystal for the HXM data (Quarati et al 2012) and 2.2 MeV due to activation of the BGO crystal for the SGM data. We examined the gain-corrected spectra using the is less than ∼ 1 • .5, we used the DRM for the fixed position.…”
Section: Spectrummentioning
confidence: 99%
“…Here we assumed an energy resolution of ∆E/E = 5.0 × (E/662 keV) −0.5 [%] (FWHM) as the detector response. The energy resolutions of the ETCCs are assumed to be typical of high-resolution scintillators (e.g., GAGG [11] and LaBr 3 [12]) that are photo-absorber candidates for the satellite ETCCs. The open blue circles in Fig.…”
Section: Extragalactic Mev Gamma-ray Backgroundmentioning
confidence: 99%
“…LaBr3(Ce) scintillation detectors are very promising due to their high light yield (>65000 photons/MeV) that results in a better energy resolution compared to NaI(Tl) detector (<3% FWHM at 137 Cs), their decay time of 35 ns and their material density (5.29 g/cm 3 ) [1,2]. Due to their better scintillation properties, when compared with NaI(Tl) scintillators, they can substitute them in many applications.…”
Section: Introductionmentioning
confidence: 99%