بررسی رشد ساختارهای بزرگ مقیاسدرکیهان انرژی ثابت گرانش غالب و مطالع تحول زمان
First Statement of Responsibility
/نوراله نظری پویا
.PUBLICATION, DISTRIBUTION, ETC
Name of Publisher, Distributor, etc.
: فیزیک
Date of Publication, Distribution, etc.
، ۱۳۹۵
Name of Manufacturer
، افشاری
NOTES PERTAINING TO PUBLICATION, DISTRIBUTION, ETC.
Text of Note
چاپی
CONTENTS NOTE
Text of Note
فاقد چکیده فارسی
DISSERTATION (THESIS) NOTE
Dissertation or thesis details and type of degree
دکتری
Discipline of degree
فیزیک گرایش نجوم و اختر فیزیک
Date of degree
۱۳۹۵/۱۱/۱۹
Body granting the degree
دانشگاه تبریز
SUMMARY OR ABSTRACT
Text of Note
The accelerated expansion of the universe is a rather established fact in cosmology and many different models have been proposed as a viable explanation. Many of these models are based on the standard general relativistic framework of non-interacting fluids or more recently of coupled (interacting) dark energy models, where dark energy (the scalar field) is coupled to the dark matter component giving rise to a fifth-force. An interesting alternative is to couple the scalar field directly to the gravity sector via the Ricci scalar. These models are dubbed non-minimally coupled models and give rise to a time-dependent gravitational constant. In this work we study few models falling into this category and describe how observables depend on the strength of the coupling. We extend recent work on the subject by taking into account also the effects of the perturbations of the scalar field and showing their relative importance on the evolution of the mass function. By working in the framework of the spherical collapse model, we show that perturbations of the scalar field have a limited impact on the growth factor (for small coupling constant) and on the mass function with respect to the case where perturbations are neglecte