Fetching the paper…

Reading the bibliography…

2019

Forecasting Interacting Vacuum-Energy Models using Gravitational Waves

Yang, Weiqiang, Pan, Supriya, Di Valentino, Eleonora et al.

Original
PDF
Post on X

Understand

The physics of the dark sector has remained one of the controversial areas of modern cosmology at present and hence it naturally attracts massive attention to the scientific community.

With the developments of the astronomical data, the physics of the dark sector is becoming much more transparent than it was some twenty years back.
The detection of gravitational waves (GWs) has now opened a cluster of possibilities in the cosmological regime.
Being motivated by the detection of GWs and its possible impact on the physics of dark matter and dark energy, in this work we focus on the interacting dark energy models.

Forecasting Interacting Vacuum-Energy Models using Gravitational Waves · Around

Built on

J. Mifsud and C. van de Bruck, An interacting dark sector and the first gravitational-wave standard siren detection,
Original
1901
Earlier work this paper cites.
M. Asghari, J. B. Jiménez, S. Khosravi and D. F. Mota, On structure formation from a small-scales-interacting dark sector,
Original
1902
Earlier work this paper cites.
J. Z. Qi, S. Cao, Y. Pan and J. Li, Cosmic opacity: cosmological-model-independent tests from gravitational waves and Type Ia Supernova,
Original
1902
Earlier work this paper cites.
L. Feng, H-L. Li, J.-F. Zhang, X. Zhang, Exploring neutrino mass and mass hierarchy in interacting dark energy models
Original
1903
Earlier work this paper cites.
A. Paliathanasis, S. Pan and W. Yang, Dynamics of nonlinear interacting dark energy models,
Original
1903
Earlier work this paper cites.
S. Pan, W. Yang, C. Singha and E. N. Saridakis, Observational constraints on sign-changeable interaction models and alleviation of the H 0 H_{0} tension,
Original
1903
Earlier work this paper cites.
S. Kumar, R. C. Nunes and S. K. Yadav, Dark sector interaction: a remedy of the tensions between CMB and LSS data,
Original
1903
Earlier work this paper cites.
A. Palmese et al
Original
1903
Earlier work this paper cites.
W. Yang, S. Vagnozzi, E. Di Valentino, R. C. Nunes, S. Pan and D. F. Mota, Listening to the sound of dark sector interactions with gravitational wave standard sirens,
Original
1905
Earlier work this paper cites.
V. F. Mukhanov, H. A. Feldman and R. H. Brandenberger, Theory of cosmological perturbations,
1992
Earlier work this paper cites.
C. P. Ma and E. Bertschinger, Cosmological perturbation theory in the synchronous and conformal Newtonian gauges,
1995
Earlier work this paper cites.
A. G. Riess et al
1998
Earlier work this paper cites.
S. Perlmutter et al
1999
Earlier work this paper cites.
L. Amendola, Coupled Quintessence,
2000
Earlier work this paper cites.
A. Lewis, A. Challinor and A. Lasenby, Efficient computation of CMB anisotropies in closed FRW models,
2000
Earlier work this paper cites.
R. Schneider, V. Ferrari, S. Matarrese and S. F. Portegies Zwart, Gravitational waves from cosmological compact binaries,
2001
Earlier work this paper cites.
A. Lewis and S. Bridle, Cosmological parameters from CMB and other data: A Monte Carlo approach,
2002
Earlier work this paper cites.
L. Amendola and C. Quercellini, Tracking and coupled dark energy as seen by WMAP,
2003
Earlier work this paper cites.
D. Pavón and W. Zimdahl, Holographic dark energy and cosmic coincidence,
2005
Earlier work this paper cites.
B. Wang, Y. g. Gong and E. Abdalla, Transition of the dark energy equation of state in an interacting holographic dark energy model,
2005
Earlier work this paper cites.
J. H. He and B. Wang, Effects of the interaction between dark energy and dark matter on cosmological parameters,
Original
2008
Earlier work this paper cites.
S. del Campo, R. Herrera and D. Pavón, Toward a solution of the coincidence problem,
Original
2008
Earlier work this paper cites.
J. Väliviita, E. Majerotto and R. Maartens, Instability in interacting dark energy and dark matter fluids,
Original
2008
Earlier work this paper cites.
J. H. He, B. Wang and Y. P. Jing, Effects of dark sectors’ mutual interaction on the growth of structures,
Original
2009
Earlier work this paper cites.
S. del Campo, R. Herrera and D. Pavón, Interacting models may be key to solve the cosmic coincidence problem,
Original
2009
Earlier work this paper cites.
K. A. Malik and D. Wands, Cosmological perturbations,
Original
2009
Earlier work this paper cites.
C. Cutler and D. E. Holz, Ultra-high precision cosmology from gravitational waves,
Original
2009
Earlier work this paper cites.
J. H. He, B. Wang, E. Abdalla and D. Pavón, The Imprint of the interaction between dark sectors in galaxy clusters,
Original
2010
Earlier work this paper cites.
E. Majerotto, J. Valiviita and R. Maartens, Adiabatic initial conditions for perturbations in interacting dark energy models,
Original
2010
Earlier work this paper cites.
F. Beutler et al
Original
2011
Earlier work this paper cites.
W. Zhao, C. Van Den Broeck, D. Baskaran and T. G. F. Li, Determination of Dark Energy by the Einstein Telescope: Comparing with CMB, BAO and SNIa Observations,
Original
2011
Earlier work this paper cites.
T. Clemson, K. Koyama, G. B. Zhao, R. Maartens and J. Valiviita, Interacting Dark Energy – constraints and degeneracies,
Original
2012
Earlier work this paper cites.
C. Heymans et al
Original
2013
Earlier work this paper cites.
A. Lewis, Efficient sampling of fast and slow cosmological parameters,
Original
2013
Earlier work this paper cites.
B. Sathyaprakash et al
Original
2013
Earlier work this paper cites.

Similar

W. Yang and L. Xu, Cosmological constraints on interacting dark energy with redshift-space distortion after Planck data,
Original
2014
Cited alongside, same era.
W. Yang and L. Xu, Coupled dark energy with perturbed Hubble expansion rate,
Original
2014
Cited alongside, same era.
A. A. Costa, X. D. Xu, B. Wang, E. G. M. Ferreira and E. Abdalla, Testing the Interaction between Dark Energy and Dark Matter with Planck Data,
Original
2014
Cited alongside, same era.
V. Salvatelli, N. Said, M. Bruni, A. Melchiorri and D. Wands, Indications of a late-time interaction in the dark sector,
Original
2014
Cited alongside, same era.
S. Pan and S. Chakraborty, A cosmographic analysis of holographic dark energy models,

Then

B. P. Abbott et al
Original
2017
Later among the works it cites.
B. P. Abbott et al
Original
2017
Later among the works it cites.
B. P. Abbott et al
Original
2017
Later among the works it cites.
B. P. Abbott et al
Original
2017
Later among the works it cites.
P. Creminelli and F. Vernizzi, Dark Energy after GW170817 and GRB170817A,
Original
2017
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…

2014

Cited alongside, same era.

Y. Wang, D. Wands, G. B. Zhao and L. Xu, Post- P l a n c k Planck constraints on interacting vacuum energy,

2014

Cited alongside, same era.

M. Betoule et al

2014

Cited alongside, same era.

S. Pan, S. Bhattacharya and S. Chakraborty, An analytic model for interacting dark energy and its observational constraints,

2015

Cited alongside, same era.

Y. L. Bolotin, A. Kostenko, O. A. Lemets and D. A. Yerokhin, Cosmological Evolution With Interaction Between Dark Energy And Dark Matter,

2015

Cited alongside, same era.

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 ,

2015

Cited alongside, same era.

Tjonnie G. F. Li, Extracting Physics from Gravitational Waves

2015

Cited alongside, same era.

P. A. R. Ade et al

2016

Cited alongside, same era.

J. M. Ezquiaga and M. Zumalacárregui, Dark Energy After GW170817: Dead Ends and the Road Ahead,

2017

Later among the works it cites.

J. Sakstein and B. Jain, Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories,

2017

Later among the works it cites.

H. Gil-Marín et al

2017

Later among the works it cites.

M. Asgari, C. Heymans, C. Blake, J. Harnois-Deraps, P. Schneider and L. Van Waerbeke, Revisiting CFHTLenS cosmic shear: Optimal E/B mode decomposition using COSEBIs and compressed COSEBIs,

2017

Later among the works it cites.

R. G. Cai and T. Yang, Estimating cosmological parameters by the simulated data of gravitational waves from the Einstein Telescope,

2017

Later among the works it cites.

N. Aghanim et al

2018

Later among the works it cites.

S. Pan, A. Mukherjee and N. Banerjee, Astronomical bounds on a cosmological model allowing a general interaction in the dark sector,

2018

Later among the works it cites.

W. Yang, S. Pan, R. Herrera and S. Chakraborty, Large-scale (in) stability analysis of an exactly solved coupled dark-energy model,

2018

Later among the works it cites.

W. Yang, S. Pan and J. D. Barrow, Large-scale Stability and Astronomical Constraints for Coupled Dark-Energy Models,

2018

Later among the works it cites.

W. Yang, S. Pan, E. Di Valentino, R. C. Nunes, S. Vagnozzi and D. F. Mota, Tale of stable interacting dark energy, observational signatures, and the H 0 H_{0} tension,

2018

Later among the works it cites.

W. Yang, A. Mukherjee, E. Di Valentino and S. Pan, Interacting dark energy with time varying equation of state and the H 0 H_{0} tension,

2018

Later among the works it cites.

C. Van De Bruck and J. Mifsud, Searching for dark matter - dark energy interactions: going beyond the conformal case,

2018

Later among the works it cites.

R. An, C. Feng and B. Wang, Relieving the Tension between Weak Lensing and Cosmic Microwave Background with Interacting Dark Matter and Dark Energy Models,

2018

Later among the works it cites.

A. A. Costa, R. C. G. Landim, B. Wang and E. Abdalla, Interacting Dark Energy: Possible Explanation for 21-cm Absorption at Cosmic Dawn,

2018

Later among the works it cites.

S. Chakraborty, K. Chakravarti, S. Bose and S. SenGupta, Signatures of extra dimensions in gravitational waves from black hole quasinormal modes,

2018

Later among the works it cites.

L. Visinelli, N. Bolis and S. Vagnozzi, Brane-world extra dimensions in light of GW170817,

2018

Later among the works it cites.

J. Oost, S. Mukohyama and A. Wang, Constraints on Einstein-aether theory after GW170817,

2018

Later among the works it cites.

A. Casalino, M. Rinaldi, L. Sebastiani and S. Vagnozzi, Mimicking dark matter and dark energy in a mimetic model compatible with GW170817,

2018

Later among the works it cites.

R. C. Nunes, S. Pan and E. N. Saridakis, New observational constraints on f ⁡ ( T ) f(T) gravity through gravitational-wave astronomy,

Original

2018

Later among the works it cites.

E. Di Valentino and A. Melchiorri, First cosmological constraints combining Planck with the recent gravitational-wave standard siren measurement of the Hubble constant,

2018

Later among the works it cites.

E. Di Valentino, D. E. Holz, A. Melchiorri and F. Renzi, The cosmological impact of future constraints on H 0 H_{0} from gravitational-wave standard sirens,

2018

Later among the works it cites.

D. M. Scolnic et al

2018

Later among the works it cites.

A. G. Riess et al

2018

Later among the works it cites.

R. G. Cai, T. B. Liu, X. W. Liu, S. J. Wang and T. Yang, Probing cosmic anisotropy with gravitational waves as standard sirens,

2018

Later among the works it cites.

L. F. Wang, X. N. Zhang, J. F. Zhang and X. Zhang, Impacts of gravitational-wave standard siren observation of the Einstein Telescope on weighing neutrinos in cosmology,

Original

2018

Later among the works it cites.

W. Yang, S. Pan, L. Xu and D. F. Mota, Effects of anisotropic stress in interacting dark matter – dark energy scenarios,

2019

Closest in time.

W. Yang, S. Pan and A. Paliathanasis, Cosmological constraints on an exponential interaction in the dark sector,

2019

Closest in time.

R. von Marttens, L. Casarini, D. F. Mota and W. Zimdahl, Cosmological constraints on parametrized interacting dark energy,

2019

Closest in time.

L. Xiao, R. An, L. Zhang, B. Yue, Y. Xu and B. Wang, Can conformal and disformal couplings between dark sectors explain the EDGES 21-cm anomaly?,

2019

Closest in time.