Evaluation of the Single-component Thermal Dust Emission Model in Cosmic Microwave Background Experiments by Hao Liu, Jia-Rui Li, Yi-Fu Cai

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Stabilization of spherically symmetric static Boson stars by Coleman-Weinberg self-interaction potential by Firoozeh Eidizadeh, Hossein Ghaffarnejad

“…We choose the CW potential because of its important role in description of cosmic inflation.…”
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Thermodynamic Phase Transition of Anti De Sitter Schwarzschild Scalar-Tensor-Vector-Black Holes by Hossein Ghaffarnejad, Elham Ghasemi

“…Instead ofscalar-tensor gravitymodels which are applicable fordescription of cosmic inflation with unknown dark sector ofmatter/energy, at present tensethere are presented different alternativescalar-tensor-vector gravitieswhere meaningful dynamical vector fields can support cosmicinflation well without to use dark matter/energy concept. …”
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