Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM , Astrophys. J. 876
Original
1903
Earlier work this paper cites.
V. de Sainte Agathe et al., Baryon acoustic oscillations at z = 2.34 from the correlations of Ly α \alpha absorption in eBOSS DR14 , Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
M. Blomqvist et al., Baryon acoustic oscillations from the cross-correlation of Ly α \alpha absorption and quasars in eBOSS DR14 , Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
T. Konstandin, R. A. Porto and H. Rubira, The Effective Field Theory of Large Scale Structure at Three Loops , 1906.00997
Original
1906
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos and A. Font-Ribera, Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future , JCAP 1910
Original
1906
Earlier work this paper cites.
1907.10625
Original
L. Verde, T. Treu and A. G. Riess, Tensions between the Early and the Late Universe , in Nature Astronomy 2019 , 2019 · 1907
Earlier work this paper cites.
The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.05271
Original
1909
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters from the BOSS Galaxy Power Spectrum , 1909.05277
Original
1909
Earlier work this paper cites.
T. Colas, G. D’amico, L. Senatore, P. Zhang and F. Beutler, Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.07951
Original
1909
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data , 1912.08208
Original
1912
Earlier work this paper cites.
C. Hahn, R. Scoccimarro, M. R. Blanton, J. L. Tinker and S. A. Rodriguez-Torres, The effect of fibre collisions on the galaxy power spectrum multipoles , Mon. Not. Roy. Astron. Soc. 467
Original
1956
Earlier work this paper cites.
C. Alcock and B. Paczynski, An evolution free test for non-zero cosmological constant , Nature 281
1979
Earlier work this paper cites.
A. J. S. Hamilton, Uncorrelated modes of the nonlinear power spectrum , Mon. Not. Roy. Astron. Soc. 312
2000
Earlier work this paper cites.
O. H. E. Philcox, M. M. Ivanov, M. Simonović and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0 , 2002.04035
Original
2002
Earlier work this paper cites.
2dFGRS Team
2002
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga and R. Scoccimarro, Large scale structure of the universe and cosmological perturbation theory , Phys. Rept. 367
2002
Earlier work this paper cites.
T. Nishimichi, G. D’Amico, M. M. Ivanov, L. Senatore, M. Simonović, M. Takada et al., Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum , 2003.08277
Original
2003
Earlier work this paper cites.
V. F. Mukhanov, CMB-slow, or how to estimate cosmological parameters by hand , Int. J. Theor. Phys. 43
2004
Earlier work this paper cites.
P. McDonald and A. Roy, Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS , JCAP 0908
Original
2009
Earlier work this paper cites.
F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, L. Campbell et al., The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant , Mon. Not. Roy. Astron. Soc. 416
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.
S. van der Walt, S. C. Colbert and G. Varoquaux, The numpy array: A structure for efficient numerical computation , Computing in Science Engineering 13
2011
Earlier work this paper cites.

Similar

D. Blas, J. Lesgourgues and T. Tram, The cosmic linear anisotropy solving system (CLASS). part II: Approximation schemes , Journal of Cosmology and Astroparticle Physics 2011
2011
Cited alongside, same era.
D. Baumann, A. Nicolis, L. Senatore and M. Zaldarriaga, Cosmological Non-Linearities as an Effective Fluid , JCAP 1207
Original
2012
Cited alongside, same era.
J. J. M. Carrasco, M. P. Hertzberg and L. Senatore, The Effective Field Theory of Cosmological Large Scale Structures , JHEP 09
Original
2012
Cited alongside, same era.
C. Howlett, A. Lewis, A. Hall and A. Challinor, CMB power spectrum parameter degeneracies in the era of precision cosmology , JCAP 1204
Original
2012
Cited alongside, same era.
E. Pajer and M. Zaldarriaga, On the Renormalization of the Effective Field Theory of Large Scale Structures , JCAP 1308

Then

A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden and M. Manera, The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 , Mon. Not. Roy. Astron. Soc. 449
Original
2015
Later among the works it cites.
T. Baldauf, E. Schaan and M. Zaldarriaga, On the reach of perturbative methods for dark matter density fields , JCAP 1603
Original
2016
Later among the works it cites.
S. Foreman, H. Perrier and L. Senatore, Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations , JCAP 1605
Original
2016
Later among the works it cites.
A. A. Abolhasani, M. Mirbabayi and E. Pajer, Systematic Renormalization of the Effective Theory of Large Scale Structure , JCAP 1605
Original
2016
Later among the works it cites.

Beyond the bibliography

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

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2020

Limits on $w$CDM from the EFTofLSS with the PyBird code

D'Amico, Guido, Senatore, Leonardo, Zhang, Pierre

Understand

We apply the Effective Field Theory of Large-Scale Structure to analyze the $w$CDM cosmological model.

By using the full shape of the power spectrum and the BAO post-reconstruction measurements from BOSS, the Supernovae from Pantheon, and a prior from BBN, we set the competitive CMB-independent limit $w=-1.046_{-0.052}^{+0.055}$ at $68\%$ C.L..
After adding the Planck CMB data, we find $w=-1.023_{-0.030}^{+0.033}$ at $68\%$ C.L..
Our results are obtained using PyBird, a new, fast Python-based code which we make publicly available.

Built on

A. G. Riess, S. Casertano, W. Yuan, L. M. Macri and D. Scolnic, Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond Λ \Lambda CDM , Astrophys. J. 876
Original
1903
Earlier work this paper cites.
V. de Sainte Agathe et al., Baryon acoustic oscillations at z = 2.34 from the correlations of Ly α \alpha absorption in eBOSS DR14 , Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
M. Blomqvist et al., Baryon acoustic oscillations from the cross-correlation of Ly α \alpha absorption and quasars in eBOSS DR14 , Astron. Astrophys. 629
Original
1904
Earlier work this paper cites.
T. Konstandin, R. A. Porto and H. Rubira, The Effective Field Theory of Large Scale Structure at Three Loops , 1906.00997
Original
1906
Earlier work this paper cites.
A. Cuceu, J. Farr, P. Lemos and A. Font-Ribera, Baryon Acoustic Oscillations and the Hubble Constant: Past, Present and Future , JCAP 1910
Original
1906
Earlier work this paper cites.
1907.10625
Original
L. Verde, T. Treu and A. G. Riess, Tensions between the Early and the Late Universe , in Nature Astronomy 2019 , 2019 · 1907
Earlier work this paper cites.
The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.05271
Original
1909
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters from the BOSS Galaxy Power Spectrum , 1909.05277
Original
1909
Earlier work this paper cites.
T. Colas, G. D’amico, L. Senatore, P. Zhang and F. Beutler, Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure , 1909.07951
Original
1909
Earlier work this paper cites.
M. M. Ivanov, M. Simonović and M. Zaldarriaga, Cosmological Parameters and Neutrino Masses from the Final Planck and Full-Shape BOSS Data , 1912.08208
Original
1912
Earlier work this paper cites.
C. Hahn, R. Scoccimarro, M. R. Blanton, J. L. Tinker and S. A. Rodriguez-Torres, The effect of fibre collisions on the galaxy power spectrum multipoles , Mon. Not. Roy. Astron. Soc. 467
Original
1956
Earlier work this paper cites.
C. Alcock and B. Paczynski, An evolution free test for non-zero cosmological constant , Nature 281
1979
Earlier work this paper cites.
A. J. S. Hamilton, Uncorrelated modes of the nonlinear power spectrum , Mon. Not. Roy. Astron. Soc. 312
2000
Earlier work this paper cites.
O. H. E. Philcox, M. M. Ivanov, M. Simonović and M. Zaldarriaga, Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0 , 2002.04035
Original
2002
Earlier work this paper cites.
2dFGRS Team
2002
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga and R. Scoccimarro, Large scale structure of the universe and cosmological perturbation theory , Phys. Rept. 367
2002
Earlier work this paper cites.
T. Nishimichi, G. D’Amico, M. M. Ivanov, L. Senatore, M. Simonović, M. Takada et al., Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum , 2003.08277
Original
2003
Earlier work this paper cites.
V. F. Mukhanov, CMB-slow, or how to estimate cosmological parameters by hand , Int. J. Theor. Phys. 43
2004
Earlier work this paper cites.
P. McDonald and A. Roy, Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS , JCAP 0908
Original
2009
Earlier work this paper cites.
F. Beutler, C. Blake, M. Colless, D. H. Jones, L. Staveley-Smith, L. Campbell et al., The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant , Mon. Not. Roy. Astron. Soc. 416
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.
S. van der Walt, S. C. Colbert and G. Varoquaux, The numpy array: A structure for efficient numerical computation , Computing in Science Engineering 13
2011
Earlier work this paper cites.

Similar

D. Blas, J. Lesgourgues and T. Tram, The cosmic linear anisotropy solving system (CLASS). part II: Approximation schemes , Journal of Cosmology and Astroparticle Physics 2011
2011
Cited alongside, same era.
D. Baumann, A. Nicolis, L. Senatore and M. Zaldarriaga, Cosmological Non-Linearities as an Effective Fluid , JCAP 1207
Original
2012
Cited alongside, same era.
J. J. M. Carrasco, M. P. Hertzberg and L. Senatore, The Effective Field Theory of Cosmological Large Scale Structures , JHEP 09
Original
2012
Cited alongside, same era.
C. Howlett, A. Lewis, A. Hall and A. Challinor, CMB power spectrum parameter degeneracies in the era of precision cosmology , JCAP 1204
Original
2012
Cited alongside, same era.
E. Pajer and M. Zaldarriaga, On the Renormalization of the Effective Field Theory of Large Scale Structures , JCAP 1308

Then

A. J. Ross, L. Samushia, C. Howlett, W. J. Percival, A. Burden and M. Manera, The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at z = 0.15 z=0.15 , Mon. Not. Roy. Astron. Soc. 449
Original
2015
Later among the works it cites.
T. Baldauf, E. Schaan and M. Zaldarriaga, On the reach of perturbative methods for dark matter density fields , JCAP 1603
Original
2016
Later among the works it cites.
S. Foreman, H. Perrier and L. Senatore, Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations , JCAP 1605
Original
2016
Later among the works it cites.
A. A. Abolhasani, M. Mirbabayi and E. Pajer, Systematic Renormalization of the Effective Theory of Large Scale Structure , JCAP 1605
Original
2016
Later among the works it cites.

Beyond the bibliography

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

Open on alphaXiv

alphaXiv is searching for related work…

Original

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.

R. A. Porto, L. Senatore and M. Zaldarriaga, The Lagrangian-space Effective Field Theory of Large Scale Structures , JCAP 1405

Original

2014

Cited alongside, same era.

J. J. M. Carrasco, S. Foreman, D. Green and L. Senatore, The 2-loop matter power spectrum and the IR-safe integrand , JCAP 1407

Original

2014

Cited alongside, same era.

J. J. M. Carrasco, S. Foreman, D. Green and L. Senatore, The Effective Field Theory of Large Scale Structures at Two Loops , JCAP 1407

Original

2014

Cited alongside, same era.

S. M. Carroll, S. Leichenauer and J. Pollack, Consistent effective theory of long-wavelength cosmological perturbations , Phys. Rev. D90

Original

2014

Cited alongside, same era.

L. Mercolli and E. Pajer, On the velocity in the Effective Field Theory of Large Scale Structures , JCAP 1403

Original

2014

Cited alongside, same era.

L. Senatore and M. Zaldarriaga, The IR-resummed Effective Field Theory of Large Scale Structures , JCAP 1502

Original

2015

Cited alongside, same era.

M. McQuinn and M. White, Cosmological perturbation theory in 1+1 dimensions , JCAP 1601

Original

2016