Built on

A. Cohen, A. Fialkov, R. Barkana and M. Lotem, Charting the Parameter Space of the Global 21-cm Signal , Mon. Not. Roy. Astron. Soc. 472
Original
1931
Earlier work this paper cites.
J. S. B. Wyithe and A. Loeb, The 21-cm power spectrum after reionization , MNRAS 397
Original
1934
Earlier work this paper cites.
E. J. Copeland, M. Sami and S. Tsujikawa, Dynamics of dark energy , Int. J. Mod. Phys. D15
1936
Earlier work this paper cites.
C. Wetterich, The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’ , Astron. Astrophys. 301
1995
Earlier work this paper cites.
Supernova Cosmology Project
1997
Earlier work this paper cites.
M. Tegmark, A. N. Taylor and A. F. Heavens, Karhunen-Loève Eigenvalue Problems in Cosmology: How Should We Tackle Large Data Sets? , ApJ 480
1997
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
L. Amendola, Coupled quintessence , Phys. Rev. D62
2000
Earlier work this paper cites.
L. Amendola and D. Tocchini-Valentini, Stationary dark energy: The Present universe as a global attractor , Phys. Rev. D64
2001
Earlier work this paper cites.
L. Amendola, Dark energy and the Boomerang data , Phys. Rev. Lett. 86
2001
Earlier work this paper cites.
L. P. Chimento, A. S. Jakubi, D. Pavon and W. Zimdahl, Interacting quintessence solution to the coincidence problem , Phys. Rev. D67
2003
Earlier work this paper cites.
A. Gomez-Valent, V. Pettorino and L. Amendola, Update on Coupled Dark Energy and the H 0 H_{0} tension , 2004.00610
Original
2004
Earlier work this paper cites.
S. Furlanetto, M. Zaldarriaga and L. Hernquist, The Growth of HII regions during reionization , Astrophys. J. 613
2004
Earlier work this paper cites.
G. Olivares, F. Atrio-Barandela and D. Pavon, Observational constraints on interacting quintessence models , Phys. Rev. D71
2005
Earlier work this paper cites.
S. R. Furlanetto, S. P. Oh and F. H. Briggs, Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe , Phys. Rep. 433
2006
Earlier work this paper cites.

Similar

M. McQuinn, O. Zahn, M. Zaldarriaga, L. Hernquist and S. R. Furlanetto, Cosmological parameter estimation using 21 cm radiation from the epoch of reionization , Astrophys. J. 653
2006
Cited alongside, same era.
Z.-K. Guo, N. Ohta and S. Tsujikawa, Probing the Coupling between Dark Components of the Universe , Phys. Rev. D76
2007
Cited alongside, same era.
B. Wang, J. Zang, C.-Y. Lin, E. Abdalla and S. Micheletti, Interacting Dark Energy and Dark Matter: Observational Constraints from Cosmological Parameters , Nucl. Phys. B778
2007
Cited alongside, same era.
J. D. Bowman, A. E. E. Rogers and J. N. Hewitt, Toward Empirical Constraints on the Global Redshifted 21 cm Brightness Temperature During the Epoch of Reionization , Astrophys. J. 676
Original
2008
Cited alongside, same era.
A. de Oliveira-Costa, M. Tegmark, B. M. Gaensler, J. Jonas, T. L. Landecker and P. Reich, A model of diffuse Galactic radio emission from 10 MHz to 100 GHz , MNRAS 388

Then

A. Liu, J. R. Pritchard, M. Tegmark and A. Loeb, Global 21 cm signal experiments: A designer’s guide , Phys. Rev. D87
Original
2013
Later among the works it cites.
L. Koopmans, J. Pritchard, G. Mellema, J. Aguirre, K. Ahn, R. Barkana et al., The Cosmic Dawn and Epoch of Reionisation with SKA , PoS (AASKA14) (Apr., 2015) 1, [ 1505.07568 ]
Original
2015
Later among the works it cites.
SKA EoR/CD SWG
Original
2015
Later among the works it cites.
Cosmology-SWG, EoR/CD-SWG
Original
2015
Later among the works it cites.
1501.03989
Original
M. Santos, P. Bull, D. Alonso, S. Camera, P. Ferreira, G. Bernardi et al., Cosmology from a SKA HI intensity mapping survey , in Advancing Astrophysics with the Square Kilometre Array (AASKA14) , p. 19, Apr., 2015 · 2015

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2019

Constraining coupled quintessence with the 21cm signal

Liu, Xue-Wen, Heneka, Caroline, Amendola, Luca

Understand

The 21cm line probes the evolution of matter perturbations over a wide range of redshifts, from the dark ages down to the completion of reionization.

Observing the 21cm cosmological signal will extend our understanding of the evolution of the Universe and it is thus important to investigate the predictions of different cosmological models.
In this paper we focus on the prospect of constraining coupled quintessence models during the Epoch of Reionization both for global signal experiments and for intensity mapping surveys.
To derive the all-sky 21cm signal and fluctuations in coupled quintessence, we simulate cosmological volumes of the 21cm signal including the coupling between dark matter and the quintessence field, where the strength of the coupling is labeled by the parameter $Q$.

Built on

A. Cohen, A. Fialkov, R. Barkana and M. Lotem, Charting the Parameter Space of the Global 21-cm Signal , Mon. Not. Roy. Astron. Soc. 472
Original
1931
Earlier work this paper cites.
J. S. B. Wyithe and A. Loeb, The 21-cm power spectrum after reionization , MNRAS 397
Original
1934
Earlier work this paper cites.
E. J. Copeland, M. Sami and S. Tsujikawa, Dynamics of dark energy , Int. J. Mod. Phys. D15
1936
Earlier work this paper cites.
C. Wetterich, The Cosmon model for an asymptotically vanishing time dependent cosmological ’constant’ , Astron. Astrophys. 301
1995
Earlier work this paper cites.
Supernova Cosmology Project
1997
Earlier work this paper cites.
M. Tegmark, A. N. Taylor and A. F. Heavens, Karhunen-Loève Eigenvalue Problems in Cosmology: How Should We Tackle Large Data Sets? , ApJ 480
1997
Earlier work this paper cites.
Supernova Search Team
1998
Earlier work this paper cites.
L. Amendola, Coupled quintessence , Phys. Rev. D62
2000
Earlier work this paper cites.
L. Amendola and D. Tocchini-Valentini, Stationary dark energy: The Present universe as a global attractor , Phys. Rev. D64
2001
Earlier work this paper cites.
L. Amendola, Dark energy and the Boomerang data , Phys. Rev. Lett. 86
2001
Earlier work this paper cites.
L. P. Chimento, A. S. Jakubi, D. Pavon and W. Zimdahl, Interacting quintessence solution to the coincidence problem , Phys. Rev. D67
2003
Earlier work this paper cites.
A. Gomez-Valent, V. Pettorino and L. Amendola, Update on Coupled Dark Energy and the H 0 H_{0} tension , 2004.00610
Original
2004
Earlier work this paper cites.
S. Furlanetto, M. Zaldarriaga and L. Hernquist, The Growth of HII regions during reionization , Astrophys. J. 613
2004
Earlier work this paper cites.
G. Olivares, F. Atrio-Barandela and D. Pavon, Observational constraints on interacting quintessence models , Phys. Rev. D71
2005
Earlier work this paper cites.
S. R. Furlanetto, S. P. Oh and F. H. Briggs, Cosmology at low frequencies: The 21 cm transition and the high-redshift Universe , Phys. Rep. 433
2006
Earlier work this paper cites.

Similar

M. McQuinn, O. Zahn, M. Zaldarriaga, L. Hernquist and S. R. Furlanetto, Cosmological parameter estimation using 21 cm radiation from the epoch of reionization , Astrophys. J. 653
2006
Cited alongside, same era.
Z.-K. Guo, N. Ohta and S. Tsujikawa, Probing the Coupling between Dark Components of the Universe , Phys. Rev. D76
2007
Cited alongside, same era.
B. Wang, J. Zang, C.-Y. Lin, E. Abdalla and S. Micheletti, Interacting Dark Energy and Dark Matter: Observational Constraints from Cosmological Parameters , Nucl. Phys. B778
2007
Cited alongside, same era.
J. D. Bowman, A. E. E. Rogers and J. N. Hewitt, Toward Empirical Constraints on the Global Redshifted 21 cm Brightness Temperature During the Epoch of Reionization , Astrophys. J. 676
Original
2008
Cited alongside, same era.
A. de Oliveira-Costa, M. Tegmark, B. M. Gaensler, J. Jonas, T. L. Landecker and P. Reich, A model of diffuse Galactic radio emission from 10 MHz to 100 GHz , MNRAS 388

Then

A. Liu, J. R. Pritchard, M. Tegmark and A. Loeb, Global 21 cm signal experiments: A designer’s guide , Phys. Rev. D87
Original
2013
Later among the works it cites.
L. Koopmans, J. Pritchard, G. Mellema, J. Aguirre, K. Ahn, R. Barkana et al., The Cosmic Dawn and Epoch of Reionisation with SKA , PoS (AASKA14) (Apr., 2015) 1, [ 1505.07568 ]
Original
2015
Later among the works it cites.
SKA EoR/CD SWG
Original
2015
Later among the works it cites.
Cosmology-SWG, EoR/CD-SWG
Original
2015
Later among the works it cites.
1501.03989
Original
M. Santos, P. Bull, D. Alonso, S. Camera, P. Ferreira, G. Bernardi et al., Cosmology from a SKA HI intensity mapping survey , in Advancing Astrophysics with the Square Kilometre Array (AASKA14) , p. 19, Apr., 2015 · 2015

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

2008

Cited alongside, same era.

J. D. Bowman and A. E. E. Rogers, A lower limit of dz > 0.06 for the duration of the reionization epoch , Nature 468

Original

2010

Cited alongside, same era.

Cambridge University Press, 2010

L. Amendola and S. Tsujikawa, Dark Energy: Theory and Observations · 2010

Cited alongside, same era.

1009.0666

Original

P. A. Henning, S. W. Ellingson, G. B. Taylor, J. Craig, Y. Pihlström, L. J. Rickard et al., The First Station of the Long Wavelength Array , in ISKAF2010 Science Meeting , p. 24, Jan., 2010 · 2010

Cited alongside, same era.

J. R. Pritchard and A. Loeb, Constraining the unexplored period between the dark ages and reionization with observations of the global 21 cm signal , Phys. Rev. D82

Original

2010

Cited alongside, same era.

A. Mesinger, S. Furlanetto and R. Cen, 21CMFAST: a fast, seminumerical simulation of the high-redshift 21-cm signal , MNRAS 411

Original

2011

Cited alongside, same era.

M. F. Morales, B. Hazelton, I. Sullivan and A. Beardsley, Four Fundamental Foreground Power Spectrum Shapes for 21 cm Cosmology Observations , Astrophys. J. 752

Original

2012