(Q60872164)

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Gauge-invariant second-order perturbations and non-Gaussianity from inflation

article by Viviana Acquaviva et al published September 2003 in Nuclear Physics B

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Gauge-invariant second-order perturbations and non-Gaussianity from inflation (English)

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Sabino Matarrese

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Antonio Riotto

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4

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Antonio Riotto

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Nicola Bartolo

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Nicola Bartolo

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Viviana Acquaviva

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September 2003

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Nuclear Physics B

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667

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1-2

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119-148

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Particle physics models of inflation and the cosmological density perturbation

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The three-point correlation function of the cosmic microwave background in inflationary models

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Cosmic microwave background bispectrum and inflation

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Nonlinear evolution of long-wavelength metric fluctuations in inflationary models

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Perturbations of spacetime: gauge transformations and gauge invariance at second order and beyond

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Relativistic second-order perturbations of the Einstein–de Sitter universe

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Theory of cosmological perturbations

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General relativistic dynamics of irrotational dust: Cosmological implications

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A relativistic approach to gravitational instability in the expanding Universe: second-order Lagrangian solutions

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Spontaneous creation of almost scale-free density perturbations in an inflationary universe

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Non-Gaussian signatures in the cosmic background radiation from warm inflation

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Large-scale structure, the cosmic microwave background and primordial non-Gaussianity

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Tests for primordial non-Gaussianity

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Measurement of the cosmic microwave background bispectrum on the COBE DMR sky maps

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Estimate of the cosmological bispectrum from the MAXIMA-1 cosmic microwave background map.

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DOI

10.1016/S0550-3213(03)00550-9

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zbMATH Open document ID

1038.83046

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(Q60872164)

Gauge-invariant second-order perturbations and non-Gaussianity from inflation

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