activity
20092026
most citedPlanck 2018 results. X. Constraints on inflation

2.4k citations · 6.8k across the 80 of their papers we have counts for

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Showing 2015Show all

8 papers · 1 filter

astro-ph.CO2015★ 28 cited

Primordial trispectra and CMB spectral distortions

Nicola Bartolo, Michele Liguori, Maresuke Shiraishi

We study the bispectrum, generated by correlations between Cosmic Microwave Background temperature (T) anisotropies and chemical potential () distortions, and we analyze i…

astro-ph.CO2015★ 176 cited

Scale-dependent gravitational waves from a rolling axion

Ryo Namba, Marco Peloso, Maresuke Shiraishi +2

We consider a model in which a pseudo-scalar field rolls for some e-folds during inflation, sourcing one helicity of a gauge field. These fields are only gravitationally couple…

astro-ph.CO2015

Future Constraints on Angle-Dependent Non-Gaussianity from Large Radio Surveys

Alvise Raccanelli, Maresuke Shiraishi, Nicola Bartolo +5

We investigate how well future large-scale radio surveys could measure different shapes of primordial non-Gaussianity; in particular we focus on angle-dependent non-Gaussianity ari…

astro-ph.CO2015★ 11 cited

Antisymmetric galaxy cross-correlations as a cosmological probe

Liang Dai, Marc Kamionkowski, Ely D. Kovetz +2

The auto-correlation between two members of a galaxy population is symmetric under the interchange of the two galaxies being correlated. The cross-correlation between two different…

astro-ph.CO2015★ 19 cited

Measuring primordial anisotropic correlators with CMB spectral distortions

Maresuke Shiraishi, Michele Liguori, Nicola Bartolo +1

We show that inflationary models with broken rotational invariance generate testable off-diagonal signatures in the correlation between the -type distortion and temperature fluc…

astro-ph.CO2015★ 70 cited

Parity-violating CMB correlators with non-decaying statistical anisotropy

Nicola Bartolo, Sabino Matarrese, Marco Peloso +1

We examine the cosmological correlators induced by the simultaneous breaking of parity and of statistical isotropy, e.g., in presence of the coupling ${\cal L} = f(ϕ) ( - \frac{1}{…