https://doi.org/10.1140/epjc/s10052-019-6740-5
Regular Article - Theoretical Physics
Modified cosmology from extended entropy with varying exponent
1
Department of Physics, Nagoya University, Nagoya, 464-8602, Japan
2
Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, 464-8602, Japan
3
Institut de Ciencies de lEspai (IEEC-CSIC), Campus UAB, Carrer de Can Magrans, s/n 08193 Cerdanyola del Valles, Barcelona, Spain
4
Institució Catalana de Recerca i Estudis Avançats (ICREA), Passeig Lluís Companys, 23, 08010, Barcelona, Spain
5
Department of Physics, National Technical University of Athens, Zografou Campus GR 157 73, Athens, Greece
6
Department of Astronomy, School of Physical Sciences, University of Science and Technology of China, Hefei, 230026, China
7
Tomsk State Pedagogical University, 634061, Tomsk, Russia
8
Int. Lab. of Theor. Cosmology, TUSUR, 634050, Tomsk, Russia
* e-mail: Emmanuel_Saridakis@baylor.edu
Received:
3
December
2018
Accepted:
3
March
2019
Published online:
16
March
2019
We present a modified cosmological scenario that arises from the application of non-extensive thermodynamics with varying exponent. We extract the modified Friedmann equations, which contain new terms quantified by the non-extensive exponent, possessing standard 
CDM cosmology as a subcase. Concerning the universe evolution at late times we obtain an effective dark energy sector, and we show that we can acquire the usual thermal history, with the successive sequence of matter and dark-energy epochs, with the effective dark-energy equation-of-state parameter being in the quintessence or in the phantom regime. The interesting feature of the scenario is that the above behaviors can be obtained even if the explicit cosmological constant is set to zero, namely they arise purely from the extra terms. Additionally, we confront the model with Supernovae type Ia and Hubble parameter observational data, and we show that the agreement is very good. Concerning the early-time universe we obtain inflationary de Sitter solutions, which are driven by an effective cosmological constant that includes the new terms of non-extensive thermodynamics. This effective screening can provide a description of both inflation and late-time acceleration with the same parameter choices, which is a significant advantage.
© The Author(s), 2019
