Confirmed width-Eiso and width-Liso relations in GRB: comparison with the Amati and Yonetoku relations
arXiv:2007.15443 · doi:10.3847/1538-4357/abaa45
Abstract
In this paper, we select a sample including 141 BEST time-integrated F spectra and 145 BEST peak flux P spectra observed by the Konus-Wind with known redshift to recheck the connection between the spectral width and as well as . We define six types of absolute spectral widths. It is found that all of the rest-frame absolute spectral widths are strongly positive correlated with as well as for the long burst for both the F and P spectra. All of the short bursts are the outliers for width- relation and most of the short bursts are consistent with the long bursts for the width- relation for both F and P spectra. Moreover, all of the location energy, and , corresponding to various spectral widths are also positive correlated with as well as . We compare all of the relations with the Amati and Yonetoku relations and find the width- and width- relations when the widths are at about 90\% maximum of the spectra almost overlap with Amati relation and Yonetoku relation, respectively. The correlations of , and , when the location energies are at 99\% maximum of the spectra are very close to the Amati and Yonetoku relations, respectively. Therefore, we confirm the existence of tight width- and width- relations for long bursts. We further show that the spectral shape is indeed related to and . The Amati and Yonetoku relations are not necessarily the best relationships to relate the energy to the and . They may be the special cases of the width- and width- relations or the energy- and energy- relations.
arXiv comment25 pages,25 figures,8 tables, accepted for publication in The Astrophysical Journal. arXiv admin note: text overlap with arXiv:1908.04663 by other authors
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