We consider contributions to non-Gaussianity of the cosmic microwave background (CMB) from remnants of phase transitions in the very early Universe. Such signatures can optimistically be used to discover evidence of new particle physics through cosmological observations. More conservatively they may provide an obstacle to extracting information about the non-Gaussian nature of primordial density fluctuations from any detection in the CMB. We study this explicitly by computing the bispectrum from global textures, which occur in a wide class of particle physics models
We discuss how primordial (e.g. inflationary) non-Gaussianity in the cosmological perturbations is l...
We study the degree to which the cosmic microwave background (CMB) can be used to constrain primordi...
We review recent results about the level of non-Gaussianity in the primordial density perturbations ...
We consider contributions to non-Gaussianity of the cosmic microwave background (CMB) from remnants ...
We consider contributions to non-Gaussianity of the cosmic microwave background (CMB) from remnants ...
The leading candidate for the very early universe is described by a period of rapid expansion known ...
In the last few decades, advances in observational cosmology have given us a standard model of cosmo...
The most direct probe of non-Gaussian initial conditions has come from bispectrum measurements of te...
The most direct probe of non-Gaussian initial conditions has come from bispectrum measurements of te...
We study non-Gaussian signatures on the cosmic microwave background (CMB) radiation predicted within...
The cosmic microwave background (CMB) provides unprecedented details about the history of our univer...
We revisit the predictions for the expected cosmic microwave background bispectrum signal from the c...
[Abridged version] A huge theoretical and experimental effort is being made by cosmologists and part...
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and b...
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and b...
We discuss how primordial (e.g. inflationary) non-Gaussianity in the cosmological perturbations is l...
We study the degree to which the cosmic microwave background (CMB) can be used to constrain primordi...
We review recent results about the level of non-Gaussianity in the primordial density perturbations ...
We consider contributions to non-Gaussianity of the cosmic microwave background (CMB) from remnants ...
We consider contributions to non-Gaussianity of the cosmic microwave background (CMB) from remnants ...
The leading candidate for the very early universe is described by a period of rapid expansion known ...
In the last few decades, advances in observational cosmology have given us a standard model of cosmo...
The most direct probe of non-Gaussian initial conditions has come from bispectrum measurements of te...
The most direct probe of non-Gaussian initial conditions has come from bispectrum measurements of te...
We study non-Gaussian signatures on the cosmic microwave background (CMB) radiation predicted within...
The cosmic microwave background (CMB) provides unprecedented details about the history of our univer...
We revisit the predictions for the expected cosmic microwave background bispectrum signal from the c...
[Abridged version] A huge theoretical and experimental effort is being made by cosmologists and part...
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and b...
A new and powerful probe of the origin and evolution of structures in the Universe has emerged and b...
We discuss how primordial (e.g. inflationary) non-Gaussianity in the cosmological perturbations is l...
We study the degree to which the cosmic microwave background (CMB) can be used to constrain primordi...
We review recent results about the level of non-Gaussianity in the primordial density perturbations ...