Built on

M. Gonzalez-Espinoza and D. Pavón, Does the second law hold at cosmic scales? , Mon. Not. Roy. Astron. Soc. 484
Original
1902
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples , 1910.13970
Original
1910
Earlier work this paper cites.
D. Bak and S. Rey, Cosmic holography , Class. Quantum Grav. 17
2000
Earlier work this paper cites.
M. Moresco, R. Jimenez, L. Verde, A. Cimatti and L. Pozzetti, Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix , Astrophys. J. 898
Original
2003
Earlier work this paper cites.
J.M. Cline, S. Jeon and J.D. Moore, The phantom menaced: Constraints on low-energy effective ghosts , Phys. Rev. D 70
2004
Earlier work this paper cites.
C.E. Rasmussen and C.K.I. Williams Gaussian Processes for Machine Learning , The MIT Press, Cambridge (2005)
2005
Earlier work this paper cites.
Y. Yang and Y. Gong, Measurement on the cosmic curvature using the Gaussian process method , Mon. Not. Roy. Astron. Soc. 504
Original
2007
Earlier work this paper cites.
J.E. Bautista et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
H. Gil-Marin et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0 , Mon. Not. Roy. Astron. Soc. 498
Original
2007
Earlier work this paper cites.
R. Neveux et al., The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
J. Hou et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
A. Tamone et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample , Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
A. de Mattia et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1 , Mon. Not. Roy. Astron. Soc. 501
Original
2007
Earlier work this paper cites.
R.A. Daly et al., Improved constraints on the acceleration history of the Universe and the properties of the dark energy , Astrophys. J. 677
Original
2008
Earlier work this paper cites.

Similar

C. A. Egan and C.H. Lineweaver, A larger estimate of the entropy of the Universe , Astrophys. J. 710
2010
Cited alongside, same era.
D. Stern, R. Jimenez, L. Verde, M. Kamionkowski and S.A. Stanford, Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H ⁡ ( z ) H(z) Measurements , JCAP 02
Original
2010
Cited alongside, same era.
M. Seikel, C. Clarkson and M. Smith, Reconstruction of dark energy and expansion dynamics using Gaussian processes , JCAP 06
Original
2012
Cited alongside, same era.
A. Shafieloo, A.G. Kim and E.V. Linder, Gaussian Process Cosmography , Phys. Rev. D 85
Original
2012
Cited alongside, same era.
M. Moresco, A. Cimatti, R. Jimenez, L. Pozzetti et al., Improved constraints on the expansion rate of the universe up to z ∼ 1.1 z\sim 1.1 from the spectroscopic evolution of cosmic chronometers , JCAP 08

Then

J.E. Bautista et al., Measurement of baryon acoustic oscillation correlations at z = 2.3 z=2.3 with SDSS DR12 Ly α \alpha -Forests , Astron. Astrophys. 603
Original
2017
Later among the works it cites.
J.P. Mimoso and D. Pavón, Fluctuations of the flux of energy on the apparent horizon , Phys. Rev. D 97
2018
Later among the works it cites.
Planck collaboration: N. Aghanim et al. Planck2018 results.VI. Cosmological parameters , Astron. Astrophys. 641
2020
Later among the works it cites.
P. Mukherjee and N. Banerjee, Constraining the curvature density parameter in cosmology , Phys. Rev. D 105
Original
2022
Later among the works it cites.
N. Borghi, M. Moresco and A. Cimatti, Toward a Better Understanding of Cosmic Chronometers: A New Measurement of H(z) at z ∼ \sim 0.7 , Astrophys. J. Lett. 928
Original

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2023

Checking the second law at cosmic scales

Banerjee, Narayan, Mukherjee, Purba, Pavón, Diego

Understand

Based on recent data about the history of the Hubble factor, it is argued that the second law of thermodynamics holds at the largest scales accessible to observation.

This is consistent with previous studies of the same question.

Built on

M. Gonzalez-Espinoza and D. Pavón, Does the second law hold at cosmic scales? , Mon. Not. Roy. Astron. Soc. 484
Original
1902
Earlier work this paper cites.
A. Lewis, GetDist: a Python package for analysing Monte Carlo samples , 1910.13970
Original
1910
Earlier work this paper cites.
D. Bak and S. Rey, Cosmic holography , Class. Quantum Grav. 17
2000
Earlier work this paper cites.
M. Moresco, R. Jimenez, L. Verde, A. Cimatti and L. Pozzetti, Setting the Stage for Cosmic Chronometers. II. Impact of Stellar Population Synthesis Models Systematics and Full Covariance Matrix , Astrophys. J. 898
Original
2003
Earlier work this paper cites.
J.M. Cline, S. Jeon and J.D. Moore, The phantom menaced: Constraints on low-energy effective ghosts , Phys. Rev. D 70
2004
Earlier work this paper cites.
C.E. Rasmussen and C.K.I. Williams Gaussian Processes for Machine Learning , The MIT Press, Cambridge (2005)
2005
Earlier work this paper cites.
Y. Yang and Y. Gong, Measurement on the cosmic curvature using the Gaussian process method , Mon. Not. Roy. Astron. Soc. 504
Original
2007
Earlier work this paper cites.
J.E. Bautista et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic correlation function between redshifts 0.6 and 1 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
H. Gil-Marin et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the luminous red galaxy sample from the anisotropic power spectrum between redshifts 0.6 and 1.0 , Mon. Not. Roy. Astron. Soc. 498
Original
2007
Earlier work this paper cites.
R. Neveux et al., The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from the anisotropic power spectrum of the quasar sample between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
J. Hou et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: BAO and RSD measurements from anisotropic clustering analysis of the Quasar Sample in configuration space between redshift 0.8 and 2.2 , Mon. Not. Roy. Astron. Soc. 500
Original
2007
Earlier work this paper cites.
A. Tamone et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Growth rate of structure measurement from anisotropic clustering analysis in configuration space between redshift 0.6 and 1.1 for the Emission Line Galaxy sample , Mon. Not. Roy. Astron. Soc. 499
Original
2007
Earlier work this paper cites.
A. de Mattia et al., The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1 , Mon. Not. Roy. Astron. Soc. 501
Original
2007
Earlier work this paper cites.
R.A. Daly et al., Improved constraints on the acceleration history of the Universe and the properties of the dark energy , Astrophys. J. 677
Original
2008
Earlier work this paper cites.

Similar

C. A. Egan and C.H. Lineweaver, A larger estimate of the entropy of the Universe , Astrophys. J. 710
2010
Cited alongside, same era.
D. Stern, R. Jimenez, L. Verde, M. Kamionkowski and S.A. Stanford, Cosmic Chronometers: Constraining the Equation of State of Dark Energy. I: H ⁡ ( z ) H(z) Measurements , JCAP 02
Original
2010
Cited alongside, same era.
M. Seikel, C. Clarkson and M. Smith, Reconstruction of dark energy and expansion dynamics using Gaussian processes , JCAP 06
Original
2012
Cited alongside, same era.
A. Shafieloo, A.G. Kim and E.V. Linder, Gaussian Process Cosmography , Phys. Rev. D 85
Original
2012
Cited alongside, same era.
M. Moresco, A. Cimatti, R. Jimenez, L. Pozzetti et al., Improved constraints on the expansion rate of the universe up to z ∼ 1.1 z\sim 1.1 from the spectroscopic evolution of cosmic chronometers , JCAP 08

Then

J.E. Bautista et al., Measurement of baryon acoustic oscillation correlations at z = 2.3 z=2.3 with SDSS DR12 Ly α \alpha -Forests , Astron. Astrophys. 603
Original
2017
Later among the works it cites.
J.P. Mimoso and D. Pavón, Fluctuations of the flux of energy on the apparent horizon , Phys. Rev. D 97
2018
Later among the works it cites.
Planck collaboration: N. Aghanim et al. Planck2018 results.VI. Cosmological parameters , Astron. Astrophys. 641
2020
Later among the works it cites.
P. Mukherjee and N. Banerjee, Constraining the curvature density parameter in cosmology , Phys. Rev. D 105
Original
2022
Later among the works it cites.
N. Borghi, M. Moresco and A. Cimatti, Toward a Better Understanding of Cosmic Chronometers: A New Measurement of H(z) at z ∼ \sim 0.7 , Astrophys. J. Lett. 928
Original

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

2012

Cited alongside, same era.

D. Foreman-Mackey, D.W. Hogg, D. Lang and J. Goodman, emcee: The MCMC Hammer , Publ. Astron. Soc. Pac. 125

Original

2013

Cited alongside, same era.

C. Zhang, H. Zhang, S. Yuan, T.-J. Zhang and Y.-C. Sun, Four new observational H ⁡ ( z ) H(z) data from luminous red galaxies in the Sloan Digital Sky Survey data release seven , Res. Astron. Astrophys. 14

Original

2014

Cited alongside, same era.

M. Moresco, Raising the bar: new constraints on the Hubble parameter with cosmic chronometers at z ∼ \sim 2 , Mon. Not. Roy. Astron. Soc. 450

Original

2015

Cited alongside, same era.

M.P. Dabrowski, Puzzles of the dark energy in the universe - phantom , Eur. J. Phys. C 36

2015

Cited alongside, same era.

R.-G. Cai, Z.-K. Guo and T. Yang, Null test of the cosmic curvature using H ⁡ ( z ) H(z) and supernovae data , Phys. Rev. D 93

Original

2016

Cited alongside, same era.

M. Moresco, L. Pozzetti, A. Cimatti, R. Jimenez, C. Maraston, L. Verde et al., A 6% measurement of the Hubble parameter at z ∼ 0.45 z\sim 0.45 : direct evidence of the epoch of cosmic re-acceleration , JCAP 05

Original

2016

Cited alongside, same era.

A.L. Ratsimbazafy, S.I. Loubser, S.M. Crawford, C.M. Cress, B.A. Bassett, R.C. Nichol et al., Age-dating Luminous Red Galaxies observed with the Southern African Large Telescope , Mon. Not. Roy. Astron. Soc. 467

Original

2017

Cited alongside, same era.

2022