Coupled quintessence scalar field model in light of observational datasets - INSPIRE

DataBETA

Coupled quintessence scalar field model in light of observational datasets

Trupti Patil
(
- IISER, Bhopal
)
,
Ruchika
(
- Indian Inst. Tech., Mumbai and
- INFN, Rome
)
,
Sukanta Panda
(
- IISER, Bhopal
)

Jul 7, 2023

22 pages

Published in:

JCAP 05 (2024) 033

Published: May 3, 2024

e-Print:

2307.03740 [astro-ph.CO]

DOI:

10.1088/1475-7516/2024/05/033

View in:

ADS Abstract Service

reference search5 citations

Citations per year

Abstract: (IOP)

We do a detailed analysis of a well-theoretically motivated interacting dark energy scalar field model with a time-varying interaction term. Using current cosmological datasets from CMB, BAO, Type Ia Supernova, H(z) measurements from cosmic chronometers, angular diameter measurements from Megamasers, growth measurements, and local SH0ES measurements, we found that dark energy component may act differently than a cosmological constant at early times. The observational data also does not disfavor a small interaction between dark energy and dark matter at late times.When using all these datasets in combination, our value of H

_{0}

agrees well with SH0ES results but in 2.5σ tension with Planck results. We also did AIC and BIC analysis, and we found that the cosmological data prefer coupled quintessence model over ΛCDM, although the chi-square per number of degrees of freedom test prefers the latter.

Note:

22 pages, 9 figures, and 7 tables; Accepted for publication in JCAP

dark energy theory
dark matter theory
quintessence: coupling
field theory: scalar
dark energy: interaction
tension
dark matter: density
time dependence
supernova
cosmological constant

References(112)

Figures(8)

[1]

Discovery of a supernova explosion at half the age of the Universe and its cosmological implications

Supernova Cosmology Project

Collaboration

•

S. Perlmutter
(
- LBL, Berkeley and
- UC, Berkeley, CfPA
)

et al.

- Nature 391 (1998) 51-54
•
e-Print:
- astro-ph/9712212
•
DOI:
- 10.1038/34124

[2]

Observational evidence from supernovae for an accelerating universe and a cosmological constant

et al.

- Astron.J. 116 (1998) 1009-1038
•
e-Print:
- astro-ph/9805201
•
DOI:
- 10.1086/300499

[3]

Measurements of $\Omega$ and $\Lambda$ from 42 High Redshift Supernovae

Supernova Cosmology Project

Collaboration

•

S. Perlmutter
(
- UC, Berkeley, CfPA
)

et al.

- Astrophys.J. 517 (1999) 565-586
•
e-Print:
- astro-ph/9812133
•
DOI:
- 10.1086/307221

[4]

The Cosmological Constant and Dark Energy

P.J.E. Peebles
(
- Princeton U.
)
,
Bharat Ratra
(
- Kansas State U.
)

- Rev.Mod.Phys. 75 (2003) 559-606,
•
e-Print:
- astro-ph/0207347
•
DOI:
- 10.1103/RevModPhys.75.559

[5]

Type Ia supernova discoveries at z > 1 from the Hubble Space Telescope: Evidence for past deceleration and constraints on dark energy evolution

et al.

- Astrophys.J. 607 (2004) 665-687
•
e-Print:
- astro-ph/0402512
•
DOI:
- 10.1086/383612

[6]

The Supernova Legacy Survey: Measurement of $\Omega_M$ , $\Omega_\Lambda$ and ${\cal w}$ from the first year data set

SNLS

Collaboration

•

P. Astier
(
- Paris U., VI-VII
)

et al.

- Astron.Astrophys. 447 (2006) 31-48
•
e-Print:
- astro-ph/0510447
•
DOI:
- 10.1051/0004-6361:20054185

[7]

Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies

SDSS

Collaboration

•

Daniel J. Eisenstein
(
- Arizona U.
)

et al.

- Astrophys.J. 633 (2005) 560-574
•
e-Print:
- astro-ph/0501171
•
DOI:
- 10.1086/466512

[8]

Cosmological parameters from the 2003 flight of BOOMERANG

C.J. MacTavish
(
- Toronto U.
)
,
P.A.R. Ade
(
- Cardiff U.
)
,
J.J. Bock
(
- Caltech, JPL
)
,
J.R. Bond
(
- Canadian Inst. Theor. Astrophys.
)
,
J. Borrill
(
- LBL, Berkeley
)

et al.

- Astrophys.J. 647 (2006) 799-812
•
e-Print:
- astro-ph/0507503
•
DOI:
- 10.1086/505558

[9]

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

WMAP

Collaboration

•

E. Komatsu
(
- Texas U.
)

et al.

- Astrophys.J.Suppl. 180 (2009) 330-376
•
e-Print:
- 0803.0547
•
DOI:
- 10.1088/0067-0049/180/2/330

[10]

Cosmological parameters from SDSS and WMAP

SDSS

Collaboration

•

Max Tegmark
(
- Pennsylvania U. and
- MIT
)

et al.

- Phys.Rev.D 69 (2004) 103501
•
e-Print:
- astro-ph/0310723
•
DOI:
- 10.1103/PhysRevD.69.103501

[11]

Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

WMAP

Collaboration

•

G. Hinshaw
(
- NASA, Goddard
)

et al.

- Astrophys.J.Suppl. 180 (2009) 225-245
•
e-Print:
- 0803.0732
•
DOI:
- 10.1088/0067-0049/180/2/225

[12]

Cosmological constraints from the Hubble diagram of quasars at high redshifts

Guido Risaliti
(
- Florence U.
)
,
Elisabeta Lusso
(
- Durham U.
)

- Nature Astron. 3 (2019) 3, 272-277
•
e-Print:
- 1811.02590
•
DOI:
- 10.1038/s41550-018-0657-z

[13]

A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km s $^{−1}$ Mpc $^{−1}$ Uncertainty from the Hubble Space Telescope and the SH0ES Team

Adam G. Riess
(
- Baltimore, Space Telescope Sci. and
- Johns Hopkins U.
)
,
Wenlong Yuan
(
- Johns Hopkins U.
)
,
Lucas M. Macri
(
- Texas A-M
)
,
Dan Scolnic
(
- Duke U.
)
,
Dillon Brout
(
- Harvard-Smithsonian Ctr. Astrophys.
)

et al.

- Astrophys.J.Lett. 934 (2022) 1, L7
•
e-Print:
- 2112.04510
•
DOI:
- 10.3847/2041-8213/ac5c5b

[14]

Model independent constraints on dark energy evolution from low-redshift observations

Salvatore Capozziello
(
- Naples U. and
- INFN, Naples and
- GSSI, Aquila
)
,
Ruchika
(
- Jamia Millia Islamia
)
,
Anjan A. Sen
(
- Jamia Millia Islamia
)

- Mon.Not.Roy.Astron.Soc. 484 (2019) 4484
•
e-Print:
- 1806.03943
•
DOI:
- 10.1093/mnras/stz176

[15]

Dynamics of dark energy

Edmund J. Copeland
(
- Nottingham U.
)
,
M. Sami
(
- Jamia Millia Islamia
)
,
Shinji Tsujikawa
(
- Gunma Coll. Tech.
)

- Int.J.Mod.Phys.D 15 (2006) 1753-1936
•
e-Print:
- hep-th/0603057
•
DOI:
- 10.1142/S021827180600942X

[16]

Beyond $\Lambda$ CDM: Problems, solutions, and the road ahead

Philip Bull
(
- Caltech and
- Oslo U.
)
,
Yashar Akrami
(
- Heidelberg U. and
- Oslo U.
)
,
Julian Adamek
(
- Montpellier U.
)
,
Tessa Baker
(
- Oxford U.
)
,
Emilio Bellini
(
- Barcelona, IEEC
)

et al.

- Phys.Dark Univ. 12 (2016) 56-99
•
e-Print:
- 1512.05356
•
DOI:
- 10.1016/j.dark.2016.02.001

[17]

Challenges for $Λ$ CDM: An update

Leandros Perivolaropoulos
(
- Ioannina U.
)
,
Foteini Skara
(
- Ioannina U.
)

- New Astron.Rev. 95 (2022) 101659
•
e-Print:
- 2105.05208
•
DOI:
- 10.1016/j.newar.2022.101659

[18]

The $H_{0}$ Olympics: A fair ranking of proposed models

et al.

- Phys.Rept. 984 (2022) 1-55
•
e-Print:
- 2107.10291
•
DOI:
- 10.1016/j.physrep.2022.07.001

[19]

Quintessence, cosmic coincidence, and the cosmological constant

Ivaylo Zlatev
(
- Pennsylvania U.
)
,
Li-Min Wang
(
- Pennsylvania U.
)
,
Paul J. Steinhardt
(
- Pennsylvania U. and
- Princeton U.
)

- Phys.Rev.Lett. 82 (1999) 896-899
•
e-Print:
- astro-ph/9807002
•
DOI:
- 10.1103/PhysRevLett.82.896

[20]

Kinetically driven quintessence

- Phys.Rev.D 62 (2000) 023511
•
e-Print:
- astro-ph/9912463
•
DOI:
- 10.1103/PhysRevD.62.023511

[21]

Kinetic k-essence and Quintessence

Roland de Putter
(
- LBL, Berkeley and
- UC, Berkeley
)
,
Eric V. Linder
(
- LBL, Berkeley and
- UC, Berkeley
)

- Astropart.Phys. 28 (2007) 263-272
•
e-Print:
- 0705.0400
•
DOI:
- 10.1016/j.astropartphys.2007.05.011

[22]

Cosmological models from quintessence

Pedro F. Gonzalez-Diaz
(
- Newton Inst. Math. Sci., Cambridge and
- Madrid, IMAFF
)

- Phys.Rev.D 62 (2000) 023513
•
e-Print:
- astro-ph/0004125
•
DOI:
- 10.1103/PhysRevD.62.023513

[23]

Thawing and Freezing Quintessence Models: A thermodynamic Consideration

- Eur.Phys.J.C 79 (2019) 11, 888
•
e-Print:
- 1906.10408
•
DOI:
- 10.1140/epjc/s10052-019-7406-z

[24]

The Limits of quintessence

R.R. Caldwell
(
- Dartmouth Coll.
)
,
Eric V. Linder
(
- LBL, Berkeley
)

- Phys.Rev.Lett. 95 (2005) 141301
•
e-Print:
- astro-ph/0505494
•
DOI:
- 10.1103/PhysRevLett.95.141301

[25]

Quintessence and the rest of the world

Sean M. Carroll
(
- Santa Barbara, KITP
)

- Phys.Rev.Lett. 81 (1998) 3067-3070
•
e-Print:
- astro-ph/9806099
•
DOI:
- 10.1103/PhysRevLett.81.3067

1-25 of 112
1
2
3
4
5
25 / page