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Physics Letters B, ISSN 0370-2693, 2007, Volume 654, Issue 1, pp. 7 - 12
Modified gravity models are subject to a number of consistency requirements which restrict the form that the function can take. We study a particular class of... 
Journal Article
Physical Review Letters, ISSN 0031-9007, 02/2014, Volume 112, Issue 5, p. 051303
We discuss whether massive neutrinos (either active or sterile) can reconcile some of the tensions within cosmological data that have been brought into focus... 
BARYON ACOUSTIC-OSCILLATIONS | MODEL | TELESCOPE | PHYSICS, MULTIDISCIPLINARY | COSMOLOGICAL CONSTRAINTS
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 07/2010, Volume 82, Issue 2
We reexamine the constraints on the cosmic string tension from cosmic microwave background (CMB) and matter power spectra, and also from limits on a stochastic... 
ANGULAR POWER SPECTRUM | EVOLUTION | COSMOLOGICAL PARAMETERS | TEMPERATURE | MODELS | SCALE STRUCTURE | MICROWAVE BACKGROUND ANISOTROPIES | ASTRONOMY & ASTROPHYSICS | GRAVITATIONAL-RADIATION | PROBE | HYBRID INFLATION | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Journal Article
PHYSICS LETTERS B, ISSN 0370-2693, 10/2007, Volume 654, Issue 1-2, pp. 7 - 12
Journal Article
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 05/2015, Volume 91, Issue 10
There is a tension between measurements of the amplitude of the power spectrum of density perturbations inferred using the cosmic microwave background (CMB)... 
COSMOLOGICAL PARAMETERS | TELESCOPE | MICROWAVE BACKGROUND ANISOTROPIES | NEUTRINO OSCILLATIONS | ASTRONOMY & ASTROPHYSICS | 6DF GALAXY SURVEY | PROBE WMAP OBSERVATIONS | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | CMB | MASSIVE NEUTRINOS | PHYSICS, PARTICLES & FIELDS | Physics - Cosmology and Nongalactic Astrophysics
Journal Article
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 06/2010, Volume 2010, Issue 6, p. 005
Journal Article
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, ISSN 1475-7516, 09/2019, Volume 2019, Issue 9, pp. 18 - 18
We use the Equation of State (EoS) approach to study the evolution of the dark sector in Horndeski models, the most general scalar-tensor theories with second... 
modified gravity | QUINTESSENCE | ENERGY | COSMOLOGY | gravity | ASTRONOMY & ASTROPHYSICS | dark energy theory | SUPERNOVAE | PHYSICS, PARTICLES & FIELDS
Journal Article
Proceedings of the Royal Society A: Mathematical, Physical and Engineering Science, ISSN 1364-5021, 01/2007, Volume 463, Issue 2077, pp. 261 - 279
We compute new solutions of the Skyrme model with massive pions. Concentrating on baryon numbers which are multiples of four, we find low-energy Skyrmion... 
Nuclear models | Isospin | Pions | Maps | Cubic crystals | Energy | Crystals | Cubes | Baryons | Symmetry | Nuclei | Skyrmions | α-particles | nuclei | PION MASSES | MULTIDISCIPLINARY SCIENCES | FIELD THEORY | O-16 | STATE | alpha-particles | RATIONAL MAPS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2014, Volume 444, Issue 1, p. 162
  We consider a novel null test for contamination which can be applied to cosmic microwave background (CMB) polarization data that involves analysis of the... 
Data analysis | Anisotropy | Cosmic microwave background temperature | Cosmology
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2014, Volume 444, Issue 1, pp. 162 - 162
We consider a novel null test for contamination which can be applied to cosmic microwave background (CMB) polarization data that involves analysis of the... 
Histograms | Polarization | Errors | Correlation | Maps | Systematic errors | Cosmic microwave background | Pixels
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2014, Volume 444, Issue 1, pp. 162 - 162
We consider a novel null test for contamination which can be applied to cosmic microwave background (CMB) polarization data that involves analysis of the... 
Journal Article
by Ade, Peter and Aguirre, James and Ahmed, Zeeshan and Aiola, Simone and Ali, Aamir and Alonso, David and Alvarez, Marcelo A and Arnold, Kam and Ashton, Peter and Austermann, Jason and Awan, Humna and Baccigalupi, Carlo and Baildon, Taylor and Barron, Darcy and Battaglia, Nick and Battye, Richard and Baxter, Eric and Bazarko, Andrew and Beall, James A and Bean, Rachel and Beck, Dominic and Beckman, Shawn and Beringue, Benjamin and Bianchini, Federico and Boada, Steven and Boettger, David and Bond, J. Richard and Borrill, Julian and Brown, Michael L and Bruno, Sarah Marie and Bryan, Sean and Calabrese, Erminia and Calafut, Victoria and Calisse, Paolo and Carron, Julien and Challinor, Anthony and Chesmore, Grace and Chinone, Yuji and Chluba, Jens and Cho, Hsiao-Mei Sherry and Choi, Steve and Coppi, Gabriele and Cothard, Nicholas F and Coughlin, Kevin and Crichton, Devin and Crowley, Kevin D and Crowley, Kevin T and Cukierman, Ari and D'Ewart, John M and Dünner, Rolando and De Haan, Tijmen and Devlin, Mark and Dicker, Simon and Didier, Joy and Dobbs, Matt and Dober, Bradley and Duell, Cody J and Duff, Shannon and Duivenvoorden, Adri and Dunkley, Jo and Dusatko, John and Errard, Josquin and Fabbian, Giulio and Feeney, Stephen and Ferraro, Simone and Fluxà, Pedro and Freese, Katherine and Frisch, Josef C and Frolov, Andrei and Fuller, George and Fuzia, Brittany and Galitzki, Nicholas and Gallardo, Patricio A and Ghersi, Jose Tomas Galvez and Gao, Jiansong and Gawiser, Eric and Gerbino, Martina and Gluscevic, Vera and Goeckner-Wald, Neil and Golec, Joseph and Gordon, Sam and Gralla, Megan and Green, Daniel and Grigorian, Arpi and Groh, John and Groppi, Chris and Guan, Yilun and Gudmundsson, Jon E and Han, Dongwon and Hargrave, Peter and Hasegawa, Masaya and Hasselfield, Matthew and Hattori, Makoto and Haynes, Victor and Hazumi, Masashi and He, Yizhou and Healy, Erin and Henderson, Shawn W and Hervias-Caimapo, Carlos and Hill, Charles A and ... and Simons Observ Collaboration and The Simons Observatory collaboration and SLAC National Accelerator Lab., Menlo Park, CA (United States) and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States) and Fysikum and Naturvetenskapliga fakulteten and Stockholms universitet and Oskar Klein-centrum för kosmopartikelfysik (OKC)
Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, 02/2019, Volume 2019, Issue 2, pp. 56 - 56
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 466, Issue 1, pp. 425 - 442
The B-mode polarization power spectrum in the cosmic microwave background (CMB) is about four orders of magnitude fainter than the CMB temperature power... 
Methods: observational | Inflation | Cosmology: observations | Cosmic background radiation | methods: observational | cosmic background radiation | MAPS | MICROWAVE | ASTRONOMY & ASTROPHYSICS | PROBE WMAP OBSERVATIONS | cosmology: observations | inflation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 445, Issue 2, pp. 1836 - 1857
We develop a method for performing a weak lensing analysis using only measurements of galaxy position angles. By analysing the statistical properties of the... 
Cosmology: theory | Methods: analytical | Methods: statistical | Gravitational lensing: weak | methods: statistical | ASTRONOMY & ASTROPHYSICS | SHAPE MEASUREMENT | methods: analytical | DARK-MATTER | DISTORTIONS | WIDE | gravitational lensing: weak | COSMIC SHEAR | CFHTLENS | cosmology: theory | Physics - Cosmology and Nongalactic Astrophysics
Journal Article