Imperial College London

Professor Andrew H Jaffe

Faculty of Natural SciencesDepartment of Physics

Professor of Astrophysics and Cosmology
 
 
 
//

Contact

 

+44 (0)20 7594 7526a.jaffe Website

 
 
//

Assistant

 

Miss Louise Hayward +44 (0)20 7594 7679

 
//

Location

 

1018BBlackett LaboratorySouth Kensington Campus

//

Summary

 

Publications

Citation

BibTex format

@unpublished{Collaboration:2019,
author = {Collaboration, P and Akrami, Y and Arroja, F and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, AJ and Barreiro, RB and Bartolo, N and Basak, S and Benabed, K and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bond, JR and Borrill, J and Bouchet, FR and Bucher, M and Burigana, C and Butler, RC and Calabrese, E and Cardoso, J-F and Casaponsa, B and Challinor, A and Chiang, HC and Colombo, LPL and Combet, C and Crill, BP and Cuttaia, F and Bernardis, PD and Rosa, AD and Zotti, GD and Delabrouille, J and Delouis, J-M and Valentino, ED and Diego, JM and Doré, O and Douspis, M and Ducout, A and Dupac, X and Dusini, S and Efstathiou, G and Elsner, F and Enßlin, TA and Eriksen, HK and Fantaye, Y and Fergusson, J and Fernandez-Cobos, R and Finelli, F and Frailis, M and Fraisse, AA and Franceschi, E and Frolov, A and Galeotta, S and Ganga, K and Génova-Santos, RT and Gerbino, M and González-Nuevo, J and Górski, KM and Gratton, S and Gruppuso, A and Gudmundsson, J},
publisher = {arXiv},
title = {Planck 2018 results. IX. Constraints on primordial non-Gaussianity},
url = {http://arxiv.org/abs/1905.05697v1},
year = {2019}
}

RIS format (EndNote, RefMan)

TY  - UNPB
AB - We analyse the Planck full-mission cosmic microwave background (CMB)temperature and E-mode polarization maps to obtain constraints on primordialnon-Gaussianity (NG). We compare estimates obtained from separabletemplate-fitting, binned, and modal bispectrum estimators, finding consistentvalues for the local, equilateral, and orthogonal bispectrum amplitudes. Ourcombined 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 extensivebattery of tests, and are stable with respect to our 2015 measurements.Polarization bispectra display a significant improvement in robustness; theycan now be used independently to set NG constraints. We consider a large numberof additional cases, e.g. scale-dependent feature and resonance bispectra,isocurvature primordial NG, and parity-breaking models, where we also placetight constraints but do not detect any signal. The non-primordial lensingbispectrum is detected with an improved significance compared to 2015,excluding the null hypothesis at 3.5 sigma. We present model-independentreconstructions and analyses of the CMB bispectrum. Our final constraint on thelocal trispectrum shape is g_NLl^local = (-5.8 +\-6.5) x 10^4 (68%CL,statistical), while constraints for other trispectra are also determined. Weconstrain the parameter space of different early-Universe scenarios, includinggeneral single-field models of inflation, multi-field and axion fieldparity-breaking models. Our results provide a high-precision test forstructure-formation scenarios, in complete agreement with the basic picture ofthe LambdaCDM cosmology regarding the statistics of the initial conditions(abridged).
AU - Collaboration,P
AU - Akrami,Y
AU - Arroja,F
AU - Ashdown,M
AU - Aumont,J
AU - Baccigalupi,C
AU - Ballardini,M
AU - Banday,AJ
AU - Barreiro,RB
AU - Bartolo,N
AU - Basak,S
AU - Benabed,K
AU - Bernard,J-P
AU - Bersanelli,M
AU - Bielewicz,P
AU - Bond,JR
AU - Borrill,J
AU - Bouchet,FR
AU - Bucher,M
AU - Burigana,C
AU - Butler,RC
AU - Calabrese,E
AU - Cardoso,J-F
AU - Casaponsa,B
AU - Challinor,A
AU - Chiang,HC
AU - Colombo,LPL
AU - Combet,C
AU - Crill,BP
AU - Cuttaia,F
AU - Bernardis,PD
AU - Rosa,AD
AU - Zotti,GD
AU - Delabrouille,J
AU - Delouis,J-M
AU - Valentino,ED
AU - Diego,JM
AU - Doré,O
AU - Douspis,M
AU - Ducout,A
AU - Dupac,X
AU - Dusini,S
AU - Efstathiou,G
AU - Elsner,F
AU - Enßlin,TA
AU - Eriksen,HK
AU - Fantaye,Y
AU - Fergusson,J
AU - Fernandez-Cobos,R
AU - Finelli,F
AU - Frailis,M
AU - Fraisse,AA
AU - Franceschi,E
AU - Frolov,A
AU - Galeotta,S
AU - Ganga,K
AU - Génova-Santos,RT
AU - Gerbino,M
AU - González-Nuevo,J
AU - Górski,KM
AU - Gratton,S
AU - Gruppuso,A
AU - Gudmundsson,JE
AU - Hamann,J
AU - Handley,W
AU - Hansen,FK
AU - Herranz,D
AU - Hivon,E
AU - Huang,Z
AU - Jaffe,AH
AU - Jones,WC
AU - Jung,G
AU - Keihänen,E
AU - Keskitalo,R
AU - Kiiveri,K
AU - Kim,J
AU - Krachmalnicoff,N
AU - Kunz,M
AU - Kurki-Suonio,H
AU - Lamarre,J-M
AU - Lasenby,A
AU - Lattanzi,M
AU - Lawrence,CR
AU - Jeune,ML
AU - Levrier,F
AU - Lewis,A
AU - Liguori,M
AU - Lilje,PB
AU - Lindholm,V
AU - López-Caniego,M
AU - Ma,Y-Z
AU - Macías-Pérez,JF
AU - Maggio,G
AU - Maino,D
AU - Mandolesi,N
AU - Marcos-Caballero,A
AU - Maris,M
AU - Martin,PG
AU - Martínez-González,E
AU - Matarrese,S
AU - Mauri,N
AU - McEwen,JD
AU - Meerburg,PD
AU - Meinhold,PR
AU - Melchiorri,A
AU - Mennella,A
AU - Migliaccio,M
AU - Miville-Deschênes,M-A
AU - Molinari,D
AU - Moneti,A
AU - Montier,L
AU - Morgante,G
AU - Moss,A
AU - Münchmeyer,M
AU - Natoli,P
AU - Oppizzi,F
AU - Pagano,L
AU - Paoletti,D
AU - Partridge,B
AU - Patanchon,G
AU - Perrotta,F
AU - Pettorino,V
AU - Piacentini,F
AU - Polenta,G
AU - Puget,J-L
AU - Rachen,JP
AU - Racine,B
AU - Reinecke,M
AU - Remazeilles,M
AU - Renzi,A
AU - Rocha,G
AU - Rubiño-Martín,JA
AU - Ruiz-Granados,B
AU - Salvati,L
AU - Savelainen,M
AU - Scott,D
AU - Shellard,EPS
AU - Shiraishi,M
AU - Sirignano,C
AU - Sirri,G
AU - Smith,K
AU - Spencer,LD
AU - Stanco,L
AU - Sunyaev,R
AU - Suur-Uski,A-S
AU - Tauber,JA
AU - Tavagnacco,D
AU - Tenti,M
AU - Toffolatti,L
AU - Tomasi,M
AU - Trombetti,T
AU - Valiviita,J
AU - Tent,BV
AU - Vielva,P
AU - Villa,F
AU - Vittorio,N
AU - Wandelt,BD
AU - Wehus,IK
AU - Zacchei,A
AU - Zonca,A
PB - arXiv
PY - 2019///
TI - Planck 2018 results. IX. Constraints on primordial non-Gaussianity
UR - http://arxiv.org/abs/1905.05697v1
UR - http://hdl.handle.net/10044/1/82460
ER -