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24 April 2024
 
  » arxiv » 1903.4409

 Article overview



Primordial Non-Gaussianity
P. Daniel Meerburg ; Daniel Green ; Muntazir Abidi ; Mustafa A. Amin ; Peter Adshead ; Zeeshan Ahmed ; David Alonso ; Behzad Ansarinejad ; Robert Armstrong ; Santiago Avila ; Carlo Baccigalupi ; Tobias Baldauf ; Mario Ballardini ; Kevin Bandura ; Nicola Bartolo ; Nicholas Battaglia ; Daniel Baumann ; Chetan Bavdhankar ; José Luis Bernal ; Florian Beutler ; Matteo Biagetti ; Colin Bischoff ; Jonathan Blazek ; J. Richard Bond ; Julian Borrill ; François R. Bouchet ; Philip Bull ; Cliff Burgess ; Christian Byrnes ; Erminia Calabrese ; John E. Carlstrom ; Emanuele Castorina ; Anthony Challinor ; Tzu-Ching Chang ; Jonas Chaves-Montero ; Xingang Chen ; Christophe Yeche ; Asantha Cooray ; William Coulton ; Thomas Crawford ; Elisa Chisari ; Francis-Yan Cyr-Racine ; Guido D'Amico ; Paolo de Bernardis ; Axel de la Macorra ; Olivier Doré ; Adri Duivenvoorden ; Joanna Dunkley ; Cora Dvorkin ; Alexander Eggemeier ; Stephanie Escoffier ; Tom Essinger-Hileman ; Matteo Fasiello ; Simone Ferraro ; Raphael Flauger ; Andreu Font-Ribera ; Simon Foreman ; Oliver Friedrich ; Juan Garcia-Bellido ; Martina Gerbino ; Vera Gluscevic ; Garrett Goon ; Krzysztof M. Gorski ; Jon E. Gudmundsson ; Nikhel Gupta ; Shaul Hanany ; Will Handley ; Adam J. Hawken ; J. Colin Hill ; Christopher M. Hirata ; Renée Hložek ; Gilbert Holder ; Dragan Huterer ; Marc Kamionkowski ; Kirit S. Karkare ; Ryan E. Keeley ; William Kinney ; Theodore Kisner ; Jean-Paul Kneib ; Lloyd Knox ; Savvas M. Koushiappas ; Ely D. Kovetz ; Kazuya Koyama ; Benjamin L'Huillier ; Ofer Lahav ; Massimiliano Lattanzi ; Hayden Lee ; Michele Liguori ; Marilena Loverde ; Mathew Madhavacheril ; Juan Maldacena ; M.C. David Marsh ; Kiyoshi Masui ; Sabino Matarrese ; Liam McAllister ; Jeff McMahon ; Matthew McQuinn ; Joel Meyers ; Mehrdad Mirbabayi ; Azadeh Moradinezhad Dizgah ; Pavel Motloch ; Suvodip Mukherjee ; Julian B. Muñoz ; Adam D. Myers ; Johanna Nagy ; Pavel Naselsky ; Federico Nati ; Newburgh ; Alberto Nicolis ; Michael D. Niemack ; Gustavo Niz ; Andrei Nomerotski ; Lyman Page ; Enrico Pajer ; Hamsa Padmanabhan ; Gonzalo A. Palma ; Hiranya V. Peiris ; Will J. Percival ; Francesco Piacentni ; Guilherme L. Pimentel ; Levon Pogosian ; Chanda Prescod-Weinstein ; Clement Pryke ; Giuseppe Puglisi ; Benjamin Racine ; Radek Stompor ; Marco Raveri ; Mathieu Remazeilles ; Gracca Rocha ; Ashley J. Ross ; Graziano Rossi ; John Ruhl ; Misao Sasaki ; Emmanuel Schaan ; Alessandro Schillaci ; Marcel Schmittfull ; Neelima Sehgal ; Leonardo Senatore ; Hee-Jong Seo ; Huanyuan Shan ; Sarah Shandera ; Blake D. Sherwin ; Eva Silverstein ; Sara Simon ; Anže Slosar ; Suzanne Staggs ; Glenn Starkman ; Albert Stebbins ; Aritoki Suzuki ; Eric R. Switzer ; Peter Timbie ; Andrew J. Tolley ; Maurizio Tomasi ; Matthieu Tristram ; Mark Trodden ; Yu-Dai Tsai ; Cora Uhlemann ; Caterina Umilta ; Alexander van Engelen ; M. Vargas-Magaña ; Abigail Vieregg ; Benjamin Wallisch ; David Wands ; Benjamin Wandelt ; Yi Wang ; Scott Watson ; Mark Wise ; W. L. K. Wu ; Zhong-Zhi Xianyu ; Weishuang Xu ; Siavash Yasini ; Sam Young ; Duan Yutong ; Matias Zaldarriaga ; Michael Zemcov ; Gong-Bo Zhao ; Yi Zheng ; Ningfeng Zhu ;
Date 11 Mar 2019
AbstractOur current understanding of the Universe is established through the pristine measurements of structure in the cosmic microwave background (CMB) and the distribution and shapes of galaxies tracing the large scale structure (LSS) of the Universe. One key ingredient that underlies cosmological observables is that the field that sources the observed structure is assumed to be initially Gaussian with high precision. Nevertheless, a minimal deviation from Gaussianityis perhaps the most robust theoretical prediction of models that explain the observed Universe; itis necessarily present even in the simplest scenarios. In addition, most inflationary models produce far higher levels of non-Gaussianity. Since non-Gaussianity directly probes the dynamics in the early Universe, a detection would present a monumental discovery in cosmology, providing clues about physics at energy scales as high as the GUT scale.
Source arXiv, 1903.4409
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