Built on

J. C. Jackson, Fingers of God: A critique of Rees’ theory of primoridal gravitational radiation , Mon. Not. Roy. Astron. Soc. 156
Original
1972
Earlier work this paper cites.
A. Mead, J. Peacock, C. Heymans, S. Joudaki and A. Heavens, An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models , Mon. Not. Roy. Astron. Soc. 454
Original
1975
Earlier work this paper cites.
R. B. Tully and J. R. Fisher, Nearby small groups of galaxies , in Large Scale Structures in the Universe (M. S. Longair and J. Einasto, eds.), vol. 79 of IAU Symposium , pp. 31–45, 1978
1978
Earlier work this paper cites.
N. Kaiser, Clustering in real space and in redshift space , Mon. Not. Roy. Astron. Soc. 227
1987
Earlier work this paper cites.
H. A. Feldman, N. Kaiser and J. A. Peacock, Power spectrum analysis of three-dimensional redshift surveys , Astrophys. J. 426
1994
Earlier work this paper cites.
A. F. Heavens, S. Matarrese and L. Verde, The Nonlinear redshift-space power spectrum of galaxies , Mon. Not. Roy. Astron. Soc. 301
1998
Earlier work this paper cites.
M. Chevallier and D. Polarski, Accelerating universes with scaling dark matter , Int. J. Mod. Phys. D10
2001
Earlier work this paper cites.
R. Teyssier, Cosmological hydrodynamics with adaptive mesh refinement: a new high resolution code called ramses , Astron. Astrophys. 385
2002
Earlier work this paper cites.
VIRGO Consortium
2003
Earlier work this paper cites.
S. Bashinsky and U. Seljak, Neutrino perturbations in CMB anisotropy and matter clustering , Phys. Rev. D69
2004
Earlier work this paper cites.
P. Crotty, J. Lesgourgues and S. Pastor, Current cosmological bounds on neutrino masses and relativistic relics , Phys. Rev. D69
2004
Earlier work this paper cites.
V. Springel, The Cosmological simulation code GADGET-2 , Mon. Not. Roy. Astron. Soc. 364
2005
Earlier work this paper cites.
G. Mangano, G. Miele, S. Pastor, T. Pinto, O. Pisanti and P. D. Serpico, Relic neutrino decoupling including flavor oscillations , Nucl. Phys. B729
2005
Earlier work this paper cites.
S. Furlanetto, S. P. Oh and F. Briggs, Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe , Phys. Rept. 433
2006
Earlier work this paper cites.
J. Lesgourgues and S. Pastor, Massive neutrinos and cosmology , Phys. Rept. 429
2006
Earlier work this paper cites.
A. Lewis and A. Challinor, The 21cm angular-power spectrum from the dark ages , Phys. Rev. D76
2007
Earlier work this paper cites.
Y. Mao, M. Tegmark, M. McQuinn, M. Zaldarriaga and O. Zahn, How accurately can 21 cm tomography constrain cosmology? , Phys. Rev. D78
Original
2008
Earlier work this paper cites.
J. E. Geach et al., Empirical H-alpha emitter count predictions for dark energy surveys , Mon. Not. Roy. Astron. Soc. 402
Original
2010
Earlier work this paper cites.
R. Jimenez, T. Kitching, C. Pena-Garay and L. Verde, Can we measure the neutrino mass hierarchy in the sky? , JCAP 1005
Original
2010
Earlier work this paper cites.
S. Hannestad, Neutrino physics from precision cosmology , Prog. Part. Nucl. Phys. 65
Original
2010
Earlier work this paper cites.
M. P. van Daalen, J. Schaye, C. M. Booth and C. D. Vecchia, The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology , Mon. Not. Roy. Astron. Soc. 415
Original
2011
Earlier work this paper cites.
J. Bonn, K. Eitel, F. Gluck, D. Sevilla-Sanchez and N. Titov, The KATRIN sensitivity to the neutrino mass and to right-handed currents in beta decay , Phys. Lett. B703
Original
2011
Earlier work this paper cites.
D. Blas, J. Lesgourgues and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes , JCAP 1107
Original
2011
Earlier work this paper cites.
M. Archidiacono, E. Calabrese and A. Melchiorri, The Case for Dark Radiation , Phys. Rev. D84
Original
2011
Earlier work this paper cites.
R. Takahashi, M. Sato, T. Nishimichi, A. Taruya and M. Oguri, Revising the Halofit Model for the Nonlinear Matter Power Spectrum , Astrophys. J. 761
Original
2012
Earlier work this paper cites.
P. Brax, A.-C. Davis, B. Li, H. A. Winther and G.-B. Zhao, Systematic Simulations of Modified Gravity: Symmetron and Dilaton Models , JCAP 1210
Original
2012
Earlier work this paper cites.
S. Clesse, L. Lopez-Honorez, C. Ringeval, H. Tashiro and M. H. G. Tytgat, Background reionization history from omniscopes , Phys. Rev. D86
Original
2012
Earlier work this paper cites.
S. Bird, M. Viel and M. G. Haehnelt, Massive Neutrinos and the Non-linear Matter Power Spectrum , Mon. Not. Roy. Astron. Soc. 420
Original
2012
Earlier work this paper cites.
Y. Ali-Haimoud and S. Bird, An efficient implementation of massive neutrinos in non-linear structure formation simulations , Mon. Not. Roy. Astron. Soc. 428
Original
2012
Earlier work this paper cites.
J. Hamann, S. Hannestad and Y. Y. Y. Wong, Measuring neutrino masses with a future galaxy survey , JCAP 1211
Original
2012
Earlier work this paper cites.
M. Archidiacono, E. Giusarma, A. Melchiorri and O. Mena, Dark Radiation in extended cosmological scenarios , Phys. Rev. D86
Original
2012
Earlier work this paper cites.
Euclid Theory Working Group
Original
2013
Earlier work this paper cites.
P. Brax, A.-C. Davis, B. Li, H. A. Winther and G.-B. Zhao, Systematic simulations of modified gravity: chameleon models , JCAP 1304
Original
2013
Earlier work this paper cites.

Similar

B. Audren, J. Lesgourgues, S. Bird, M. G. Haehnelt and M. Viel, Neutrino masses and cosmological parameters from a Euclid-like survey: Markov Chain Monte Carlo forecasts including theoretical errors , JCAP 1301
Original
2013
Cited alongside, same era.
P. Brax, S. Clesse and A.-C. Davis, Signatures of Modified Gravity on the 21-cm Power Spectrum at Reionisation , JCAP 1301
Original
2013
Cited alongside, same era.
Cambridge Univ. Press, Cambridge, 2013
J. Lesgourgues, G. Mangano, G. Miele and S. Pastor, Neutrino cosmology · 2013
Cited alongside, same era.
B. Audren, J. Lesgourgues, K. Benabed and S. Prunet, Conservative Constraints on Early Cosmology: an illustration of the Monte Python cosmological parameter inference code , JCAP 1302
Original
2013
Cited alongside, same era.
Z. Hou, R. Keisler, L. Knox, M. Millea and C. Reichardt, How Massless Neutrinos Affect the Cosmic Microwave Background Damping Tail , Phys. Rev. D87

Then

L. Pozzetti, C. M. Hirata, J. E. Geach, A. Cimatti, C. Baugh, O. Cucciati et al., Modelling the number density of H? emitters for future spectroscopic near-IR space missions , Astron. Astrophys. 590
Original
2016
Later among the works it cites.
P. Dewdney, T. Stevenson and A. M. McPherson, Ska1 system baseline design v2 , 2016
2016
Later among the works it cites.
P. Bull, Extending cosmological tests of General Relativity with the Square Kilometre Array , Astrophys. J. 817
Original
2016
Later among the works it cites.
I. Harrison, S. Camera, J. Zuntz and M. L. Brown, SKA weak lensing – I. Cosmological forecasts and the power of radio-optical cross-correlations , Mon. Not. Roy. Astron. Soc. 463
Original
2016
Later among the works it cites.
A. Bonaldi, I. Harrison, S. Camera and M. L. Brown, SKA weak lensing? II. Simulated performance and survey design considerations , Mon. Not. Roy. Astron. Soc. 463

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2018

Cosmology in the era of Euclid and the Square Kilometre Array

Sprenger, Tim, Archidiacono, Maria, Brinckmann, Thejs et al.

Understand

Theoretical uncertainties on non-linear scales are among the main obstacles to exploit the sensitivity of forthcoming galaxy and hydrogen surveys like Euclid or the Square Kilometre Array (SKA).

Here, we devise a new method to model the theoretical error that goes beyond the usual cut-off on small scales.
The advantage of this more efficient implementation of the non-linear uncertainties is tested through a Markov-Chain-Monte-Carlo (MCMC) forecast of the sensitivity of Euclid and SKA to the parameters of the standard $\Lambda$CDM model, including massive neutrinos with total mass $M_\nu$, and to 3 extended scenarios, including 1) additional relativistic degrees of freedom ($\Lambda$CDM + $M_\nu$ + $N_\mathrm{eff}$), 2) a deviation from the cosmological constant ($\Lambda$CDM + $M_\nu$ + $w_0$), and 3) a time-varying dark energy equation of state parameter ($\Lambda$CDM + $M_\nu$ + $\left(w_0,w_a \right)$).
We compare the sensitivity of 14 different combinations of cosmological probes and experimental configurations.