A closed-form hypergeometric and Taylor treatment of dark-energy and Cardassian distance integrals is fitted to SN and GRB data, but the key integral identity and the data treatment are flawed.
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The distance modulus in dark energy and Cardassian cosmologies via the hypergeometric function
A closed-form hypergeometric and Taylor treatment of dark-energy and Cardassian distance integrals is fitted to SN and GRB data, but the key integral identity and the data treatment are flawed.