Planck 2013 results. XXII. Constraints on inflation

@article{Ade2014Planck2R,
  title={Planck 2013 results. XXII. Constraints on inflation},
  author={P. A. R. Ade and Nabila Aghanim and Charmaine Armitage-Caplan and Monique D. Arnaud and Mark Ashdown and F. Atrio-Barandela and J. Aumont and Carlo Baccigalupi and Anthony J. Banday and Rita Bel{\'e}n Barreiro and James G. Bartlett and Nicola Bartolo and Eduardo Battaner and Karim Benabed and Aur{\'e}lien Benoit and Aur{\'e}lien Benoit-L{\'e}vy and J-Ph. Bernard and M. Bersanelli and Pawel Bielewicz and J{\'e}r{\^o}me Bobin and James J. Bock and Anna Bonaldi and J. Richard Bond and Julian Borrill and Francois R. Bouchet and Michael Bridges and Manfred Bucher and Carlo Burigana and R. C. Butler and Erminia Calabrese and Jean-François Cardoso and A. Catalano and Anthony Challinor and A. Chamballu and H. C. Chiang and L. Y. Chiang and Philip R. Christensen and Sarah E. Church and David L. Clements and St{\'e}phane Colombi and Loris P. L. Colombo and François Couchot and A. Coulais and Brendan P. Crill and A. Fernandez Curto and F. Cuttaia and Luigi Danese and Rodney D. Davies and R. J. Davis and Paolo Bernardis and Alessandra De Rosa and Gianfranco De Zotti and Jacques Delabrouille and J. M. Delouis and F.-X. D{\'e}sert and Clive Dickinson and Jose M. Diego and Herve A. Dole and Simona Donzelli and Olivier Dor{\'e} and Marian Douspis and Jo Dunkley and Xavier Dupac and George P. Efstathiou and Torsten A. Ensslin and Hans Kristian Eriksen and Fabio Finelli and Olivier Forni and Marco Frailis and Enrico Franceschi and S. Galeotta and Ken Ganga and C. Gauthier and Martin Giard and Giovanna Giardino and Y. Giraud-Hiraud and Joaqu{\'i}n Gonz{\'a}lez-Nuevo and Krzysztof M. Gorski and Steven Gratton and Anna Gregorio and Alessandro Gruppuso and Jan Hamann and F. K. Hansen and Duncan Hanson and D. L. Harrison and S. Henrot-Versill{\'e} and Carlos Hernandez-Monteagudo and Diego Herranz and Sergi R. Hildebrandt and Eric Hivon and Michael P. Hobson and Warren Albert Holmes and Allan Hornstrup and W. Hovest and Kevin M. Huffenberger and Andrew H. Jaffe and Tess R. Jaffe and William C. Jones and Mika Juvela and Elina Keihanen and Reijo Keskitalo and Theodore Kisner and R{\"u}diger Kneissl and J{\"o}rg Knoche and Lloyd Knox and Martin Kunz and Hannu Kurki-Suonio and Guilaine Lagache and Anne Lahteenmaki and J-M. Lamarre and Anthony N. Lasenby and Ren{\'e} J. Laureijs and Charles R. Lawrence and Samuel M. Leach and Janet Leahy and Rodrigo Leonardi and Julien Lesgourgues and A. M. Lewis and Michele Liguori and Per B. Lilje and M. Linden-Vernle and Marcos L{\'o}pez-Caniego and Philip Lubin and J. F. Mac{\'i}as-P{\'e}rez and Bruno Maffei and Davide Maino and Nazzareno Mandolesi and Michele Maris and Douglas J. Marshall and P. G. Martin and Enrique Mart{\'i}nez-Gonz{\'a}lez and Silvia Masi and Marcella Massardi and S. Matarrese and Frank Matthai and Pasquale Mazzotta and Peter Meinhold and Alessandro Melchiorri and Luis Mendes and Aniello Mennella and Marina Migliaccio and Supriyo Mitra and Marc-Antoine Miville-Desch{\^e}nes and Andrea Moneti and Laurent Montier and G. Morgante and Daniel J. Mortlock and Adam Moss and Dipak Munshi and J. Anthony Murphy and Pavel D. Naselsky and Federico Nati and Paolo Natoli and Calvin Barth Netterfield and Hans Ulrik N{\o}rgaard-Nielsen and Fabio Noviello and Dmitri D Novikov and Ilya Novikov and Ian O'Dwyer and Shannon Osborne and Carol Anne Oxborrow and Francesco Paci and Luca Pagano and François Pajot and Rolando Paladini and Silvia Pandolfi and Daniela Paoletti and Bruce Partridge and Fabio Pasian and Guillaume Patanchon and Hiranya V. Peiris and Olivier Perdereau and L. Perotto and F. Perrotta and Francesco Piacentini and Michel Piat and Elena Pierpaoli and Davide Pietrobon and St{\'e}phane Plaszczynski and Etienne Pointecouteau and Gianluca Polenta and N. Ponthieu and L. A. Popa and Torsti J. Poutanen and Gabriel W. Pratt and Gary Marcel Prezeau and Simon Prunet and J-L. Puget and Jorg P. Rachen and Rafael Rebolo and Martin Reinecke and Mathieu Remazeilles and C'ecile Renault and Stefano Ricciardi and Thomas Riller and Isabelle Ristorcelli and Graca M. Rocha and C. Dutruc Rosset and Gael M. Roudier and Michael Rowan-Robinson and Jos{\'e} Alberto Rubi{\~n}o-Mart{\'i}n and Ben Rusholme and M. Sandri and D. Santos and Matti Savelainen and Giorgio Savini and Douglas Scott and Michael Dean Seiffert and E. P. S. Shellard and Locke D Spencer and J. L. Starck and Vasily Stolyarov and Radek Stompor and R. Sudiwala and Rashid Sunyaev and Florent Sureau and David O. Sutton and A.-S. Suur-Uski and J. -F. Sygnet and Jan Tauber and Daniele Tavagnacco and Luca Terenzi and Luigi Toffolatti and Maurizio Tomasi and J. Tr{\'e}guer-Goudineau and M. Tristram and Marco Tucci and Jussi Tuovinen and Luca Valenziano and Jussi Valiviita and Bartjan van Tent and Juha Varis and Patricio Vielva and Fabrizio Villa and Nicola Vittorio and Lawrence A. Wade and Benjamin D. Wandelt and Martin White and Althea Wilkinson and D. Yvon and Andrea Zacchei and James P. Zibin and Andrea Zonca},
  journal={Astronomy and Astrophysics},
  year={2014},
  volume={571},
  pages={1-65}
}
We present the implications for cosmic inflation of the Planck measurements of the cosmic microwave background (CMB) anisotropies in both temperature and polarization based on the full Planck survey, which includes more than twice the integration time of the nominal survey used for the 2013 release papers. The Planck full mission temperature data and a first release of polarization data on large angular scales measure the spectral index of curvature perturbations to be ns = 0.968 ± 0.006 and… 
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References

SHOWING 1-10 OF 541 REFERENCES
Planck 2015. XX. Constraints on inflation
We analyse the implications of the Planck data for cosmic inflation. The Planck nominal mission temperature anisotropy measurements, combined with the WMAP large-angle polarization, constrain the
Planck 2015 results - XIII. Cosmological parameters
This paper presents cosmological results based on full-mission Planck observations of temperature and polarization anisotropies of the cosmic microwave background (CMB) radiation. Our results are in
Planck 2013 results. XVI. Cosmological parameters
This paper presents the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra. We find that the Planck
Planck 2015 results - XV. Gravitational lensing
We present the most significant measurement of the cosmic microwave background (CMB) lensing potential to date (at a level of 40σ), using temperature and polarization data from the Planck 2015
A joint analysis of Planck and BICEP2 B modes including dust polarization uncertainty
We analyze BICEP2 and Planck data using a model that includes CMB lensing, gravity waves, and polarized dust. Recently published Planck dust polarization maps have highlighted the difficulty of
Planck 2013 results. XVII. Gravitational lensing by large-scale structure
On the arcminute angular scales probed by Planck, the cosmic microwave background (CMB) anisotropies are gently perturbed by gravitational lensing. Here we present a detailed study of this e_ect,
Planck 2015 results - XI. CMB power spectra, likelihoods, and robustness of parameters
This paper presents the Planck 2015 likelihoods, statistical descriptions of the 2-point correlationfunctions of the cosmic microwave background (CMB) temperature and polarization fluctuations that
Planck 2018 results. VII. Isotropy and Statistics of the CMB
Analysis of the Planck 2018 data set indicates that the statistical properties of the cosmic microwave background (CMB) temperature anisotropies are in excellent agreement with previous studies using
Planck 2015 results. IX. Diffuse component separation: CMB maps
We present foreground-reduced cosmic microwave background (CMB) maps derived from the full Planck data set in both temperature and polarization. Compared to the corresponding Planck 2013 temperature
Planck2013 results. XXIII. Isotropy and statistics of the CMB
We test the statistical isotropy and Gaussianity of the cosmic microwave background (CMB) anisotropies using observations made by the Planck satellite. Our results are based mainly on the full Planck
...
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