Several experiments (including BOOMERanG, MAXIMA, DASI, VSA, CBI) have recently detected very low contrast structures in the Cosmic Microwave Background (CMB), the otherwise isotropic radiation coming from the early Universe. These structures have a contrast of the order of 25 ppm and a dominant angular size of one degree. In the current cosmological model, these structures result from acoustic oscillations of the primeval plasma within the horizon at recombination (z » 1100). In the framework of the Hot Big Bang theory with the inflationary hypothesis, the statistical properties of the image of the CMB allow us to measure most of the cosmological parameters
The blackbody radiation left over from the Big Bang has been transformed by the expansion of the Uni...
We discuss the cosmological implications of the new constraints on the power spectrum of the cosmic ...
An approach to obtain high-quality data of the early universe was presented by using cosmic microwav...
Several experiments (including BOOMERanG, MAXIMA, DASI, VSA, CBI) have recently detected very low c...
Several experiments (including BOOMERanG, MAXIMA, DASI, VSA,CBI) have recently detected very low con...
The BOOMERanG experiment has recently detected temperature fluctuations the Cosmic Microwave Backgro...
Several experiments have recently detected very low contrast, sub-horizon scale structures in the Co...
Several experiments have recently detected very low contrast, sub-horizon scale structures in the Co...
The existence and anisotropy of the cosmic microwave background (CMB), the large scale distribution ...
The cosmic microwave background radiation is the remnant heat from the Big Bang. It provides us with...
The existence and anisotropy of the cosmic microwave background (CMB), the large scale distribution ...
Abstract. The cosmic microwave background (CMB) is one of only a few physically observable remnants ...
The cosmic microwave background radiation is the remnant heat from the Big Bang. It provides us with...
Research on the Cosmic Microwave Background (CMB) has provided clean maps of the early Universe, dep...
The blackbody radiation left over from the Big Bang has been transformed by the expansion of the Uni...
We discuss the cosmological implications of the new constraints on the power spectrum of the cosmic ...
An approach to obtain high-quality data of the early universe was presented by using cosmic microwav...
Several experiments (including BOOMERanG, MAXIMA, DASI, VSA, CBI) have recently detected very low c...
Several experiments (including BOOMERanG, MAXIMA, DASI, VSA,CBI) have recently detected very low con...
The BOOMERanG experiment has recently detected temperature fluctuations the Cosmic Microwave Backgro...
Several experiments have recently detected very low contrast, sub-horizon scale structures in the Co...
Several experiments have recently detected very low contrast, sub-horizon scale structures in the Co...
The existence and anisotropy of the cosmic microwave background (CMB), the large scale distribution ...
The cosmic microwave background radiation is the remnant heat from the Big Bang. It provides us with...
The existence and anisotropy of the cosmic microwave background (CMB), the large scale distribution ...
Abstract. The cosmic microwave background (CMB) is one of only a few physically observable remnants ...
The cosmic microwave background radiation is the remnant heat from the Big Bang. It provides us with...
Research on the Cosmic Microwave Background (CMB) has provided clean maps of the early Universe, dep...
The blackbody radiation left over from the Big Bang has been transformed by the expansion of the Uni...
We discuss the cosmological implications of the new constraints on the power spectrum of the cosmic ...
An approach to obtain high-quality data of the early universe was presented by using cosmic microwav...