Planck 2018 results. IX. Constraints on primordial non-Gaussianity
We analyse the Planck full-mission cosmic microwave background (CMB) temperature and E-mode polarization maps to obtain constraints on primordial non-Gaussianity (NG). We compare estimates obtained from separable template-fitting, binned, and modal bispectrum estimators, finding consistent values for the local, equilateral, and orthogonal bispectrum amplitudes. Our combined temperature and polarization analysis produces the following results: f_NL^local = -0.9 +\- 5.1; f_NL^equil = -26 +\- 47; and f_NL^ortho = - 38 +\- 24 (68%CL, statistical). These results include the low-multipole (4 <= l < 40) polarization data, not included in our previous analysis, pass an extensive battery of tests, and are stable with respect to our 2015 measurements. Polarization bispectra display a significant improvement in robustness; they can now be used independently to set NG constraints. We consider a large number of additional cases, e.g. scale-dependent feature and resonance bispectra, isocurvature primordial NG, and parity-breaking models, where we also place tight constraints but do not detect any signal. The non-primordial lensing bispectrum is detected with an improved significance compared to 2015, excluding the null hypothesis at 3.5 sigma. We present model-independent reconstructions and analyses of the CMB bispectrum. Our final constraint on the local trispectrum shape is g_NLl^local = (-5.8 +\-6.5) x 10^4 (68%CL, statistical), while constraints for other trispectra are also determined. We constrain the parameter space of different early-Universe scenarios, including general single-field models of inflation, multi-field and axion field parity-breaking models. Our results provide a high-precision test for structure-formation scenarios, in complete agreement with the basic picture of the LambdaCDM cosmology regarding the statistics of the initial conditions (abridged).
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05/14/19 06:02PM
Masa_S3: Planck 2018 results. IX. Constraints on primordial non-Gaussianity
emulenews: Planck 2018 results. IX. Constraints on primordial non-Gaussianity. No signal detected. The non-primordial lensing bispectrum is detected with an improved significance compared to 2015, excluding the null hypothesis at 3.5 σ.
Fulguritics: @memcculloch Shape/polariz.-defined coherent structure averaged out. Results are moot, as the BB cannot be Gaussian. Is CMB itself primordial? Can it be both - a mixture model w/unknowable nodes? Many smoothed non-Gauss. distributions fit skewed Gaussians 3/3
dagushh: RT @skdh: New Planck Results
VergaraLautaro: SCIENCE (technical) Planck 2018 results Constraints on primordial non-Gaussianity Our results ... show complete agreement with the basic picture of the ΛCDM cosmology...
GregorioBaquer5: RT @skdh: New Planck Results
gravitesque: RT @skdh: New Planck Results
cmbearg: Nuevos resultados de Planck sobre no gaussianidad primordial: incluyen los datos de polarización a bajos multipolos. A grandes rasgos, los datos indican que no hay evidencia de no gaussianidad.
196884: f_NL^local = -0.9 +\- 5.1 f_NL^equil = -26 +\- 47 f_NL^ortho = - 38 +\- 24 g_NLl^local = (-5.8 +\-6.5) x 10^4 (68%CL)
life_wont_wait: オルソゴナルはワンチャンあるように見えなくもない(見えない)/Planck 2018 results. IX. Constraints on primordial non-Gaussianity
emulenews: RT @skdh: New Planck Results
kainoeske: RT @skdh: New Planck Results
skdh: New Planck Results
RelativityPaper: Planck 2018 results. IX. Constraints on primordial non-Gaussianity.