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Prospects of high redshift constraints on dark energy models with the <i>E</i>p, i โ <i>E</i>iso correlation in long gamma ray bursts
ABSTRACT So far large and different data sets revealed the accelerated expansion rate of the Universe, which is usually explained in terms of dark energy. The nature of dark energy is not yet known, and several models have been introduced: a non-zero cosmological constant, a potential energy of some scalar โฆ