TY - JOUR
T1 - Warm inflationary model in loop quantum cosmology
AU - Herrera, Ramón
PY - 2010
Y1 - 2010
N2 - A warm inflationary universe model in loop quantum cosmology is studied. In general we discuss the condition of inflation in this framework. By using a chaotic potential, V(φ) φ 2, we develop a model where the dissipation coefficient Γ=Γ0=constant. We use recent astronomical observations for constraining the parameters appearing in our model.
AB - A warm inflationary universe model in loop quantum cosmology is studied. In general we discuss the condition of inflation in this framework. By using a chaotic potential, V(φ) φ 2, we develop a model where the dissipation coefficient Γ=Γ0=constant. We use recent astronomical observations for constraining the parameters appearing in our model.
UR - http://www.scopus.com/inward/record.url?scp=77954653503&partnerID=8YFLogxK
U2 - 10.1103/PhysRevD.81.123511
DO - 10.1103/PhysRevD.81.123511
M3 - Article
AN - SCOPUS:77954653503
SN - 1550-7998
VL - 81
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 12
M1 - 123511
ER -