2,007 research outputs found

    Gratification obtained from television shows on Internet TV and conventional TV

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    Television shows once available only on conventional TV in homes at specific days and times are now available via Internet TV in nearly any location, 24 hours a day. However, while the shows may be the same on conventional TV and Internet TV, the motivations and benefits of viewing may be different for each delivery platform. This study employs uses and gratification theory (U&G) to compare audience rationales for watching television shows on conventional TV to watching TV shows on Internet TV. Research prior to the wide availability of Internet TV (Stafford et al., 2004) summarized reasons for watching television programs as 1) gratifications gained from the content of the program, 2) gratifications gained from the process of obtaining the program, and 3) gratifications gained from the social interactions that come from the consumption of television programming. Using those three gratifications, this study conducted an online survey among users of both conventional and Internet TV. The data indicated that on Internet TV, the process of watching shows to be the leading gratification. On conventional TV, the first motivation is the program content. The results of the survey offer suggestions for the management of Internet and conventional program services

    Towards Understanding Astrophysical Effects of Nuclear Symmetry Energy

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    Determining the Equation of State (EOS) of dense neutron-rich nuclear matter is a shared goal of both nuclear physics and astrophysics. Except possible phase transitions, the density dependence of nuclear symmetry \esym is the most uncertain part of the EOS of neutron-rich nucleonic matter especially at supra-saturation densities. Much progresses have been made in recent years in predicting the symmetry energy and understanding why it is still very uncertain using various microscopic nuclear many-body theories and phenomenological models. Simultaneously, significant progresses have also been made in probing the symmetry energy in both terrestrial nuclear laboratories and astrophysical observatories. In light of the GW170817 event as well as ongoing or planned nuclear experiments and astrophysical observations probing the EOS of dense neutron-rich matter, we review recent progresses and identify new challenges to the best knowledge we have on several selected topics critical for understanding astrophysical effects of the nuclear symmetry energy.Comment: 77 pages. Invited Review Article, EPJA (2019) in pres
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