TY - JOUR
T1 - A holographic cut-off inspired in the apparent horizon
AU - Cruz, Miguel
AU - Lepe, Samuel
N1 - Funding Information:
M. C. acknowledges the hospitality of the Instituto de Física of Pontificia Universidad Católica de Valparaíso, Chile, where part of this work was done. M.C. work is supported by S.N.I. (CONACyT-México) and PRODEP (UV-PTC-851).
Funding Information:
Acknowledgements M. C. acknowledges the hospitality of the Insti-tuto de Física of Pontificia Universidad Católica de Valparaíso, Chile, where part of this work was done. M.C. work is supported by S.N.I. (CONACyT-México) and PRODEP (UV-PTC-851).
Publisher Copyright:
© 2018, The Author(s).
PY - 2018/12/1
Y1 - 2018/12/1
N2 - In this work we consider a general function for the c2 term that appears in the conventional expression for the holographic dark energy in a FLRW curved spacetime. The cut-off prospective is inspired in the apparent horizon length. By exploring the slowly varying condition for the c2 term, we obtain a range of validity for this holographic proposal. Under these considerations can be found that this holographic cut-off is adequate to describe the late cosmic evolution. Additionally, by considering some values constrained with the use of observational data for some cosmological parameters in the context of dark energy models, such as the deceleration parameter or the parameter state, can be shown that this holographic model remains close to the Λ CDM model.
AB - In this work we consider a general function for the c2 term that appears in the conventional expression for the holographic dark energy in a FLRW curved spacetime. The cut-off prospective is inspired in the apparent horizon length. By exploring the slowly varying condition for the c2 term, we obtain a range of validity for this holographic proposal. Under these considerations can be found that this holographic cut-off is adequate to describe the late cosmic evolution. Additionally, by considering some values constrained with the use of observational data for some cosmological parameters in the context of dark energy models, such as the deceleration parameter or the parameter state, can be shown that this holographic model remains close to the Λ CDM model.
UR - http://www.scopus.com/inward/record.url?scp=85057711928&partnerID=8YFLogxK
U2 - 10.1140/epjc/s10052-018-6484-7
DO - 10.1140/epjc/s10052-018-6484-7
M3 - Article
AN - SCOPUS:85057711928
VL - 78
JO - European Physical Journal C
JF - European Physical Journal C
SN - 1434-6044
IS - 12
M1 - 994
ER -