# Planck 2013 results. XXII. Constraints on inflation

@article{Ade2014Planck2R, title={Planck 2013 results. XXII. Constraints on inflation}, author={P. Ade and N. Aghanim and C. Armitage-Caplan and M. Arnaud and M. Ashdown and F. Atrio-Barandela and J. Aumont and C. Baccigalupi and A. Banday and R. B. Barreiro and J. Bartlett and N. Bartolo and E. Battaner and K. Benabed and A. Benoit and A. Benoit-L{\'e}vy and J. Bernard and M. Bersanelli and P. Bielewicz and J. Bobin and J. Bock and A. Bonaldi and J. Bond and J. Borrill and F. Bouchet and M. Bridges and M. Bucher and C. Burigana and R. C. Butler and E. Calabrese and J. Cardoso and A. Catalano and A. Challinor and A. Chamballu and H. Chiang and L. Chiang and P. Christensen and S. Church and D. Clements and S. Colombi and L. Colombo and F. Couchot and A. Coulais and B. Crill and A. Curto and F. Cuttaia and L. Danese and R. Davies and R. Davis and P. Bernardis and A. Rosa and G. Zotti and J. Delabrouille and J. Delouis and F. D{\'e}sert and C. Dickinson and J. Diego and H. Dole and S. Donzelli and O. Dor{\'e} and M. Douspis and J. Dunkley and X. Dupac and G. Efstathiou and T. Ensslin and H. Eriksen and F. Finelli and O. Forni and M. Frailis and E. Franceschi and S. Galeotta and K. Ganga and C. Gauthier and M. Giard and G. Giardino and Y. Giraud-Hiraud and J. Gonz{\'a}lez-Nuevo and K. G{\'o}rski and S. Gratton and A. Gregorio and A. Gruppuso and J. Hamann and F. Hansen and D. Hanson and D. Harrison and S. Henrot-Versill{\'e} and C. Hernandez-Monteagudo and D. Herranz and S. Hildebrandt and E. Hivon and M. Hobson and W. Holmes and A. Hornstrup and W. Hovest and K. Huffenberger and A. Jaffe and T. Jaffe and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and R. Kneissl and J. Knoche and L. Knox and M. Kunz and H. Kurki-Suonio and G. Lagache and A. Lahteenmaki and J. Lamarre and A. Lasenby and R. Laureijs and C. Lawrence and S. Leach and J. Leahy and R. Leonardi and J. Lesgourgues and A. Lewis and M. Liguori and P. Lilje and M. Linden-Vernle and M. L{\'o}pez-Caniego and P. Lubin and J. Macias-P{\'e}rez and B. Maffei and D. Maino and N. Mandolesi and M. Maris and D. Marshall and P. Martin and E. Martinez-Gonzalez and S. Masi and M. Massardi and S. Matarrese and F. Matthai and P. Mazzotta and P. Meinhold and A. Melchiorri and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. Miville-Desch{\^e}nes and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and C. Netterfield and H. N{\o}rgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and I. O'Dwyer and S. Osborne and C. A. Oxborrow and F. Paci and L. Pagano and F. Pajot and R. Paladini and S. Pandolfi and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and H. Peiris and O. Perdereau and L. Perotto and F. Perrotta and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and N. Ponthieu and L. Popa and T. Poutanen and G. Pratt and G. Prezeau and S. Prunet and J. Puget and J. Rachen and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and S. Ricciardi and T. Riller and I. Ristorcelli and G. Rocha and C. Rosset and G. Roudier and M. Rowan-Robinson and J. Rubi{\~n}o-Mart{\'i}n and B. Rusholme and M. Sandri and D. Santos and M. Savelainen and G. Savini and D. Scott and M. Seiffert and E. Shellard and L. Spencer and J. Starck and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and F. Sureau and D. Sutton and A. Suur-Uski and J. Sygnet and J. Tauber and D. Tavagnacco and L. Terenzi and L. Toffolatti and M. Tomasi and J. Tr{\'e}guer-Goudineau and M. Tristram and M. Tucci and J. Tuovinen and L. Valenziano and J. Valiviita and B. Tent and J. Varis and P. Vielva and F. Villa and N. Vittorio and L. Wade and B. Wandelt and M. White and A. Wilkinson and D. Yvon and A. Zacchei and J. P. Zibin and A. 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… Expand

#### Figures and Tables from this paper

table 1 figure 1 figure 10 table 10 figure 11 table 11 figure 12 table 12 figure 13 figure 14 figure 15 figure 16 figure 17 figure 18 figure 19 table 2 figure 2 figure 20 figure 21 figure 22 figure 23 figure 24 table 3 figure 3 table 4 figure 4 table 5 figure 5 figure 6 table 6 figure 7 table 7 figure 8 table 8 figure 9 table 9 figure A.1 figure A.3

#### 916 Citations

#### References

SHOWING 1-10 OF 547 REFERENCES