The de Sitter universe is the second model of the universe just after the publications of the Einstein’s static and closed model. In 1917, Wilhelm de Sitter has developed this model which is a maximally symmetric solution of the Einstein field equation with zero density. The geometry of the de Sitter universe is theoretically more complicated than that of the Einstein universe. The model does not contain matter or radiation. But, it predicts that there is a redshift. This article tries to describe the de Sitter model in some detail but easier mathematical calculations. In this study an attempt has been taken to provide a brief discussion of de Sitter model to the common readers
A semi-classical analysis of vacuum energy in the expanding spacetime suggests that the cosmological...
It has recently been discovered that Einstein once attempted - and subsequently abandoned - a 'stead...
We present a translation and analysis of a cosmic model published by Einstein in 1931. The paper, wh...
The de Sitter universe is the second model of the universe just after the publications of the Einste...
We present some historical and philosophical reflections on the paper “On the Relation Between the E...
We present a first English translation and analysis of a little-known review of relativistic cosmolo...
Starting with the Friedmann-Lemaître (FL) metric g F L of an isotropic universe, we give the radiall...
Decaying vacuum cosmological models evolving smoothly between two extreme (very early and late time)...
peer reviewedThe Einstein–de Sitter cosmological model, a spatially flat Friedmann–Robertson–Walker ...
The de Sitter spacetime is a maximally symmetric spacetime. It is one of the vacuum solutions to Ein...
We present a first English translation and analysis of a little-known review of relativistic cosmolo...
In this work we analyze the development of de Sitter-Fantappie Relativity by analyzing, particularly...
One of the greatest scientists Albert Einstein laid the foundation of Special and General Relativity...
In 1917, both Einstein and de Sitter proposed a new interpretation of the universe as a whole: the s...
The present paper tries to answer the question: Can a de Sitter phase in presence of radiation be ...
A semi-classical analysis of vacuum energy in the expanding spacetime suggests that the cosmological...
It has recently been discovered that Einstein once attempted - and subsequently abandoned - a 'stead...
We present a translation and analysis of a cosmic model published by Einstein in 1931. The paper, wh...
The de Sitter universe is the second model of the universe just after the publications of the Einste...
We present some historical and philosophical reflections on the paper “On the Relation Between the E...
We present a first English translation and analysis of a little-known review of relativistic cosmolo...
Starting with the Friedmann-Lemaître (FL) metric g F L of an isotropic universe, we give the radiall...
Decaying vacuum cosmological models evolving smoothly between two extreme (very early and late time)...
peer reviewedThe Einstein–de Sitter cosmological model, a spatially flat Friedmann–Robertson–Walker ...
The de Sitter spacetime is a maximally symmetric spacetime. It is one of the vacuum solutions to Ein...
We present a first English translation and analysis of a little-known review of relativistic cosmolo...
In this work we analyze the development of de Sitter-Fantappie Relativity by analyzing, particularly...
One of the greatest scientists Albert Einstein laid the foundation of Special and General Relativity...
In 1917, both Einstein and de Sitter proposed a new interpretation of the universe as a whole: the s...
The present paper tries to answer the question: Can a de Sitter phase in presence of radiation be ...
A semi-classical analysis of vacuum energy in the expanding spacetime suggests that the cosmological...
It has recently been discovered that Einstein once attempted - and subsequently abandoned - a 'stead...
We present a translation and analysis of a cosmic model published by Einstein in 1931. The paper, wh...