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Related papers: Testing multi-field inflation with LiteBIRD

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The measurement of B-mode polarization of the cosmic microwave background at large angular scales by the BICEP experiment suggests a stochastic gravitational wave background from early-universe inflation with a surprisingly large amplitude.…

Cosmology and Nongalactic Astrophysics · Physics 2014-05-21 Jerod Caligiuri , Arthur Kosowsky

The recently released BICEP2 data detected the primordial B-mode polarization in the Cosmic Microwave Background (CMB) map which strongly supports for a large tensor-to-scalar ratio, and thus, is found to be in tension with the Planck…

Cosmology and Nongalactic Astrophysics · Physics 2014-07-30 Youping Wan , Siyu Li , Mingzhe Li , Taotao Qiu , Yifu Cai , Xinmin Zhang

We study the mixed scalar-tensor two-point function in icosahedral inflation. Within the regime of validity of the effective field theory, this has to be perturbatively small; in particular, much smaller than the scalar spectrum. However,…

High Energy Physics - Theory · Physics 2021-05-05 Alberto Nicolis , Guanhao Sun

We derive power spectra of the scalar- and tensor-type structures generated in an inflation model based on a massive non-minimally coupled scalar field with the strong coupling assumption. We make analyses in both the original-frame and the…

Astrophysics · Physics 2009-12-30 J. Hwang , H. Noh

We revisit arguments that simple models of inflation with a small red tilt in the scalar power spectrum generically yield an observable tensor spectrum. We show that criteria for fine-tuning based upon the algebraic simplicity of the…

Astrophysics · Physics 2008-12-18 Simeon Bird , Hiranya V. Peiris , Richard Easther

In conventional model independent approaches, the power spectrum of primordial perturbations is characterized by such free parameters as spectral index, its running, the running of running, and the tensor-to-scalar ratio. In this work we,…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-15 Moslem Zarei

We present the power spectra of the scalar- and tensor-type structures generated in an inflation model based on the nonminimally coupled scalar field with a self coupling. By comparing the contributions of these structures to the anisotropy…

Astrophysics · Physics 2013-07-09 H. Noh , J. Hwang

In the previous work, a new kind of inflation model was proposed, which has the interesting property that its perturbation equation of motion gets a correction of k^4, due to the non-linearity of the kinetic term. Nonetheless, the…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-16 Jun Chen , Hou Wenjie , Defu Hou , Taotao Qiu

Inflation is the leading theory of the first instant of the universe. Inflation, which postulates that the universe underwent a period of rapid expansion an instant after its birth, provides convincing explanation for cosmological…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 A. Suzuki , P. A. R. Ade , Y. Akiba , D. Alonso , K. Arnold , J. Aumont , C. Baccigalupi , D. Barron , S. Basak , S. Beckman , J. Borrill , F. Boulanger , M. Bucher , E. Calabrese , Y. Chinone , H-M. Cho , A. Cukierman , D. W. Curtis , T. de Haan , M. Dobbs , A. Dominjon , T. Dotani , L. Duband , A. Ducout , J. Dunkley , J. M. Duval , T. Elleflot , H. K. Eriksen , J. Errard , J. Fischer , T. Fujino , T. Funaki , U. Fuskeland , K. Ganga , N. Goeckner-Wald , J. Grain , N. W. Halverson , T. Hamada , T. Hasebe , M. Hasegawa , K. Hattori , M. Hattori , L. Hayes , M. Hazumi , N. Hidehira , C. A. Hill , G. Hilton , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , M. Inoue , Y. Inoue , K. D. , H. Ishino , O. Jeong , H. Kanai , D. Kaneko , S. Kashima , N. Katayama , T. Kawasaki , S. A. Kernasovskiy , R. Keskitalo , A. Kibayashi , Y. Kida , K. Kimura , T. Kisner , K. Kohri , E. Komatsu , K. Komatsu , C. L. Kuo , N. A. Kurinsky , A. Kusaka , A. Lazarian , A. T. Lee , D. Li , E. Linder , B. Maffei , A. Mangilli , M. Maki , T. Matsumura , S. Matsuura , D. Meilhan , S. Mima , Y. Minami , K. Mitsuda , L. Montier , M. Nagai , T. Nagasaki , R. Nagata , M. Nakajima , S. Nakamura , T. Namikawa , M. Naruse , H. Nishino , T. Nitta , T. Noguchi , H. Ogawa , S. Oguri , N. Okada , A. Okamoto , T. Okamura , C. Otani , G. Patanchon , G. Pisano , G. Rebeiz , M. Remazeilles , P. L. Richards , S. Sakai , Y. Sakurai , Y. Sato , N. Sato , M. Sawada , Y. Segawa , Y. Sekimoto , U. Seljak , B. D. Sherwin , T. Shimizu , K. Shinozaki , R. Stompor , H. Sugai , H. Sugita , J. Suzuki , O. Tajima , S. Takada , R. Takaku , S. Takakura , S. Takatori , D. Tanabe , E. Taylor , K. L. Thompson , B. Thorne , T. Tomaru , T. Tomida , N. Tomita , M. Tristram , C. Tucker , P. Turin , M. Tsujimoto , S. Uozumi , S. Utsunomiya , Y. Uzawa , F. Vansyngel , I. K. Wehus , B. Westbrook , M. Willer , N. Whitehorn , Y. Yamada , R. Yamamoto , N. Yamasaki , T. Yamashita , M. Yoshida

A rigorous constraint analysis on cosmic inflation entails several probes which collectively survey an extensive range of energy scales. We complement the cosmic microwave background data with an updated compilation of the cosmic abundance…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-23 Jurgen Mifsud , Carsten van de Bruck

The latest results from PLANCK impose strong constraints on features in the spectrum of the curvature perturbations from inflation. We analyse the possibility of particle production induced by sharp turns of the trajectory in field space in…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 Maciej Konieczka , Raquel H. Ribeiro , Krzysztof Turzynski

We investigate the Lyth relationship between the tensor-scalar ratio, r, and the variation of the inflaton field, Delta phi, over the course of inflation. For inflationary models that produce at least 55 e-folds of inflation, there is a…

Astrophysics · Physics 2009-11-10 George Efstathiou , Katherine J. Mack

The recent measurements of cosmological parameters by the Planck collaboration favors inflationary models with a redshifted spectrum and a very low tensor-to-scalar ratio. Two well-studied scenarios in the particle physics/string theory…

High Energy Physics - Phenomenology · Physics 2014-01-31 Sean Downes

We investigate the possibility of utilising 21cm intensity mapping, optical galaxy, and Cosmic Microwave Background (CMB) surveys to constrain the power spectrum of primordial fluctuations predicted by single-field slow-roll inflation…

Cosmology and Nongalactic Astrophysics · Physics 2017-01-09 Alkistis Pourtsidou

We discuss a new test of inflation from the harmonic pattern of peaks in the cosmic microwave background radiation angular power spectrum. By characterizing the features of alternate models and revealing signatures essentially unique to…

Astrophysics · Physics 2009-08-18 Wayne Hu , Martin White

Recent fits of cosmological parameters by the Wilkinson Microwave Anisotropy Probe (WMAP) measurement favor a primordial scalar spectrum with varying index. This result, if stands, could severely constrain inflation model buildings. Most…

Astrophysics · Physics 2008-11-26 Bo Feng , Mingzhe Li , Ren-Jie Zhang , Xinmin Zhang

LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency…

Instrumentation and Methods for Astrophysics · Physics 2023-03-28 LiteBIRD Collaboration , E. Allys , K. Arnold , J. Aumont , R. Aurlien , S. Azzoni , C. Baccigalupi , A. J. Banday , R. Banerji , R. B. Barreiro , N. Bartolo , L. Bautista , D. Beck , S. Beckman , M. Bersanelli , F. Boulanger , M. Brilenkov , M. Bucher , E. Calabrese , P. Campeti , A. Carones , F. J. Casas , A. Catalano , V. Chan , K. Cheung , Y. Chinone , S. E. Clark , F. Columbro , G. D'Alessandro , P. de Bernardis , T. de Haan , E. de la Hoz , M. De Petris , S. Della Torre , P. Diego-Palazuelos , M. Dobbs , T. Dotani , J. M. Duval , T. Elleflot , H. K. Eriksen , J. Errard , T. Essinger-Hileman , F. Finelli , R. Flauger , C. Franceschet , U. Fuskeland , M. Galloway , K. Ganga , M. Gerbino , M. Gervasi , R. T. Génova-Santos , T. Ghigna , S. Giardiello , E. Gjerløw , J. Grain , F. Grupp , A. Gruppuso , J. E. Gudmundsson , N. W. Halverson , P. Hargrave , T. Hasebe , M. Hasegawa , M. Hazumi , S. Henrot-Versillé , B. Hensley , L. T. Hergt , D. Herman , E. Hivon , R. A. Hlozek , A. L. Hornsby , Y. Hoshino , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , H. Ishino , G. Jaehnig , N. Katayama , A. Kato , R. Keskitalo , T. Kisner , Y. Kobayashi , A. Kogut , K. Kohri , E. Komatsu , K. Komatsu , K. Konishi , N. Krachmalnicoff , C. L. Kuo , L. Lamagna , M. Lattanzi , A. T. Lee , C. Leloup , F. Levrier , E. Linder , G. Luzzi , J. Macias-Perez , T. Maciaszek , B. Maffei , D. Maino , S. Mandelli , E. Martínez-González , S. Masi , M. Massa , S. Matarrese , F. T. Matsuda , T. Matsumura , L. Mele , M. Migliaccio , Y. Minami , A. Moggi , J. Montgomery , L. Montier , G. Morgante , B. Mot , Y. Nagano , T. Nagasaki , R. Nagata , R. Nakano , T. Namikawa , F. Nati , P. Natoli , S. Nerval , F. Noviello , K. Odagiri , S. Oguri , H. Ohsaki , L. Pagano , A. Paiella , D. Paoletti , A. Passerini , G. Patanchon , F. Piacentini , M. Piat , G. Pisano , G. Polenta , D. Poletti , T. Prouvé , G. Puglisi , D. Rambaud , C. Raum , S. Realini , M. Reinecke , M. Remazeilles , A. Ritacco , G. Roudil , J. A. Rubino-Martin , M. Russell , H. Sakurai , Y. Sakurai , M. Sasaki , D. Scott , Y. Sekimoto , K. Shinozaki , M. Shiraishi , P. Shirron , G. Signorelli , F. Spinella , S. Stever , R. Stompor , S. Sugiyama , R. M. Sullivan , A. Suzuki , T. L. Svalheim , E. Switzer , R. Takaku , H. Takakura , Y. Takase , A. Tartari , Y. Terao , J. Thermeau , H. Thommesen , K. L. Thompson , M. Tomasi , M. Tominaga , M. Tristram , M. Tsuji , M. Tsujimoto , L. Vacher , P. Vielva , N. Vittorio , W. Wang , K. Watanuki , I. K. Wehus , J. Weller , B. Westbrook , J. Wilms , B. Winter , E. J. Wollack , J. Yumoto , M. Zannoni

We develop a general formalism for analyzing linear perturbations in multiple-field cosmological inflation based on the gauge-ready approach. Our inflationary model consists of an arbitrary number of scalar fields with non-minimal kinetic…

Astrophysics · Physics 2009-11-13 Joydev Lahiri , Gautam Bhattacharya

We study multifield contributions to the scalar power spectrum in an ensemble of six-field inflationary models obtained in string theory. We identify examples in which inflation occurs by chance, near an approximate inflection point, and we…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Liam McAllister , Sébastien Renaux-Petel , Gang Xu

We study the possibility of using the $LiteBIRD$ satellite $B$-mode survey to constrain models of inflation producing specific features in CMB angular power spectra. We explore a particular model example, i.e. spectator axion-SU(2) gauge…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-25 P. Campeti , E. Komatsu , C. Baccigalupi , M. Ballardini , N. Bartolo , A. Carones , J. Errard , F. Finelli , R. Flauger , S. Galli , G. Galloni , S. Giardiello , M. Hazumi , S. Henrot-Versillé , L. T. Hergt , K. Kohri , C. Leloup , J. Lesgourgues , J. Macias-Perez , E. Martínez-González , S. Matarrese , T. Matsumura , L. Montier , T. Namikawa , D. Paoletti , D. Poletti , M. Remazeilles , M. Shiraishi , B. van Tent , M. Tristram , L. Vacher , N. Vittorio , G. Weymann-Despres , A. Anand , J. Aumont , R. Aurlien , A. J. Banday , R. B. Barreiro , A. Basyrov , M. Bersanelli , D. Blinov , M. Bortolami , T. Brinckmann , E. Calabrese , F. Carralot , F. J. Casas , L. Clermont , F. Columbro , G. Conenna , A. Coppolecchia , F. Cuttaia , G. D'Alessandro , P. de Bernardis , M. De Petris , S. Della Torre , E. Di Giorgi , P. Diego-Palazuelos , H. K. Eriksen , C. Franceschet , U. Fuskeland , M. Galloway , M. Georges , M. Gerbino , M. Gervasi , T. Ghigna , C. Gimeno-Amo , E. Gjerløw , A. Gruppuso , J. Gudmundsson , N. Krachmalnicoff , L. Lamagna , M. Lattanzi , M. Lembo , A. I. Lonappan , S. Masi , M. Massa , S. Micheli , A. Moggi , M. Monelli , G. Morgante , B. Mot , L. Mousset , R. Nagata , P. Natoli , A. Novelli , I. Obata , L. Pagano , A. Paiella , V. Pavlidou , F. Piacentini , M. Pinchera , G. Pisano , G. Puglisi , N. Raffuzzi , A. Ritacco , A. Rizzieri , M. Ruiz-Granda , G. Savini , D. Scott , G. Signorelli , S. L. Stever , N. Stutzer , R. M. Sullivan , A. Tartari , K. Tassis , L. Terenzi , K. L. Thompson , P. Vielva , I. K. Wehus , Y. Zhou