Andere Kunden interessierten sich auch für
![An Introduction to the Theory of the Cosmic Microwave Background]( "An Introduction to the Theory of the Cosmic Microwave Background")
An Introduction to the Theory of the Cosmic Microwave Background44,99 €![Present and Future of the Cosmic Microwave Background]( "Present and Future of the Cosmic Microwave Background")
Present and Future of the Cosmic Microwave Background37,99 €![The Limiting Background in a Detector Testing Facility for SuperCDMS]( "The Limiting Background in a Detector Testing Facility for SuperCDMS")
The Limiting Background in a Detector Testing Facility for SuperCDMS32,99 €![Infrared Atmospheric Background Modeling]( "Infrared Atmospheric Background Modeling")
Infrared Atmospheric Background Modeling32,99 €![Discovery of cosmic microwave background radiation]( "Discovery of cosmic microwave background radiation")
Discovery of cosmic microwave background radiation22,99 €![The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background]( "The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background")
The Universe at High-z, Large-Scale Structure and the Cosmic Microwave Background39,99 €![Surface Contaminations In Low Background Experiments]( "Surface Contaminations In Low Background Experiments")
Surface Contaminations In Low Background Experiments44,99 €
The main aim of this book is to study the Cosmological Principle, the basic assumption of cosmological standard model, through observations. The possible violation of global isotropy in the Cosmic Microwave Background has been a subject of intense research after the publication of WMAP data. The possible alignment of axes corresponding to several diverse data sets in the direction of the Virgo cluster makes this extremely interesting. In recent years, there have been a large number of studies which claim the CMB temperature fluctuations are not consistent with statistical isotropy and thus questioning the cosmological principle. Meanwhile there are some studies which also found no inconsistency. Differences arise due to different independent statistical methods that are designed to study deviations from statistical isotropy. The reason is that statistical isotropy can be violated in many different ways and each independent statistical method is more sensitive to a special kind ofviolation of statistical isotropy. It is, therefore, necessary to explore new observables to determine whether the CMB sky is a realization of statistically isotropic or not.