Tightening the reins on nonminimal dark sector physics: Interacting dark energy with dynamical and nondynamical equation of state - INSPIRE

DataBETA

Tightening the reins on nonminimal dark sector physics: Interacting dark energy with dynamical and nondynamical equation of state

William Giarè
(
- Sheffield U.
)
,
Yuejia Zhai
(
- Sheffield U.
)
,
Supriya Pan
(
- DUT, Durban and
- Presidency U., Kolkata
)
,
Eleonora Di Valentino
(
- Sheffield U.
)
,
Rafael C. Nunes
(
- Sao Jose, INPE and
- Rio Grande do Sul U.
)

Apr 2, 2024

21 pages

Published in:

Phys.Rev.D 110 (2024) 6, 063527

Published: Sep 11, 2024

e-Print:

2404.02110 [astro-ph.CO]

DOI:

10.1103/PhysRevD.110.063527 (publication)

View in:

ADS Abstract Service

reference search20 citations

Citations per year

Abstract: (APS)

We present a comprehensive reassessment of the state of interacting dark energy (DE) cosmology, namely models featuring a nongravitational interaction between dark matter and DE. To achieve high generality, we extend the dark sector physics by considering two different scenarios: a nondynamical DE equation of state

w_{0} \neq - 1

, and a dynamical

w (a) = w_{0} + w_{a} (1 - a)

. In both cases, we distinguish two different physical regimes resulting from a phantom or quintessence equation of state. To circumvent early time superhorizon instabilities, the energy-momentum transfer should occur in opposing directions within the two regimes, resulting in distinct phenomenological outcomes. We study quintessence and phantom nondynamical and dynamical models in light of two independent cosmic microwave background (CMB) experiments—the Planck satellite and the Atacama Cosmology Telescope. We analyze CMB data both independently and in combination with supernovae distance moduli measurements from the Pantheon-Plus catalog and baryon acoustic oscillations from the SDSS-IV eBOSS survey. Our results update and extend the state-of-the-art analyses, significantly narrowing the parameter space allowed for these models and limiting their overall ability to reconcile cosmological tensions. Although considering different combinations of data leaves some freedom to increase

H_{0}

towards the value measured by the SH0ES collaboration, our most constraining dataset (

CMB + baryon

acoustic

oscillations + supernovae

) indicates that fully reconciling the tension solely within the framework of interacting DE remains challenging.

Note:

21 pages, 4 figures, 9 tables. V2: additional references added, clarified some aspects of the results, their interpretation, and implications. Version accepted for publication in PRD

satellite: Planck
dark energy: equation of state
oscillation: acoustic
cosmic background radiation
phantom
tension
quintessence
dark matter: hidden sector
cosmological model: parameter space
moduli

References(176)

Figures(4)

[1]

Snowmass2021 - Letter of interest cosmology intertwined II: The hubble constant tension

Eleonora Di Valentino
(
- Manchester U.
)
,
Luis A. Anchordoqui
(
- New York U.
)
,
Ozgur Akarsu
(
- Istanbul, Tech. U.
)
,
Yacine Ali-Haimoud
(
- New York U.
)
,
Luca Amendola
(
- Heidelberg U.
)

et al.

- Astropart.Phys. 131 (2021) 102605
•
e-Print:
- 2008.11284
•
DOI:
- 10.1016/j.astropartphys.2021.102605

[2]

Cosmology Intertwined III: $f \sigma_8$ and $S_8$

Eleonora Di Valentino
(
- Jodrell Bank
)
,
Luis A. Anchordoqui
(
- CUNY, Graduate School - U. Ctr.
)
,
Özgür Akarsu
(
- Istanbul, Tech. U.
)
,
Yacine Ali-Haimoud
(
- New York U.
)
,
Luca Amendola
(
- U. Heidelberg, ITP
)

et al.

- Astropart.Phys. 131 (2021) 102604
•
e-Print:
- 2008.11285
•
DOI:
- 10.1016/j.astropartphys.2021.102604

[3]

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

[4]

Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies

Elcio Abdalla
(
- Sao Paulo U.
)
,
Guillermo Franco Abellán
(
- U. Montpellier 2, LUPM
)
,
Amin Aboubrahim
(
- Munster U., ITP
)
,
Adriano Agnello
(
- DARK Cosmology Ctr.
)
,
Ozgur Akarsu
(
- Istanbul, Tech. U.
)

et al.

- JHEAp 34 (2022) 49-211
•
e-Print:
- 2203.06142
•
DOI:
- 10.1016/j.jheap.2022.04.002

[5]

Tensions between the Early and the Late Universe

L. Verde
(
- ICREA, Barcelona and
- ICC, Barcelona U.
)
,
T. Treu
(
- UCLA, Los Angeles (main)
)
,
A.G. Riess
(
- Johns Hopkins U. (main) and
- Baltimore, Space Telescope Sci.
)

- Nature Astron. 3 (2019) 891
•
e-Print:
- 1907.10625
•
DOI:
- 10.1038/s41550-019-0902-0

[6]

In the realm of the Hubble tension—a review of solutions

Eleonora Di Valentino
(
- Durham U., IPPP
)
,
Olga Mena
(
- Valencia U., IFIC
)
,
Supriya Pan
(
- Presidency U., Kolkata
)
,
Luca Visinelli
(
- Frascati
)
,
Weiqiang Yang
(
- Liaoning Normal U.
)

et al.

- Class.Quant.Grav. 38 (2021) 15, 153001
•
e-Print:
- 2103.01183
•
DOI:
- 10.1088/1361-6382/ac086d

[7]

The Hubble Tension and Early Dark Energy

- Ann.Rev.Nucl.Part.Sci. 73 (2023) 153-180
•
e-Print:
- 2211.04492
•
DOI:
- 10.1146/annurev-nucl-111422-024107

[8]

Review of Hubble tension solutions with new SH0ES and SPT-3G data

Ali Rida Khalife
(
- Paris, Inst. Astrophys.
)
,
Maryam Bahrami Zanjani
(
- RWTH Aachen U.
)
,
Silvia Galli
(
- Paris, Inst. Astrophys.
)
,
Sven Günther
(
- RWTH Aachen U.
)
,
Julien Lesgourgues
(
- RWTH Aachen U.
)

et al.

- JCAP 04 (2024) 059
•
e-Print:
- 2312.09814
•
DOI:
- 10.1088/1475-7516/2024/04/059

[9]

Planck 2018 results. VI. Cosmological parameters

Planck

Collaboration

•

N. Aghanim
(
- Orsay, IAS
)

et al.

- Astron.Astrophys. 641 (2020) A6,
- Astron.Astrophys. 652 (2021) C4 (erratum)
•
e-Print:
- 1807.06209
•
DOI:
- 10.1051/0004-6361/201833910

[9]

Planck 2018 results. VI. Cosmological parameters

Planck

Collaboration

•

N. Aghanim
(
- Orsay, IAS
)

et al.

- Astron.Astrophys. 641 (2020) A6,
- Astron.Astrophys. 652 (2021) C4 (erratum)
•
e-Print:
- 1807.06209
•
DOI:
- 10.1051/0004-6361/201833910

[10]

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

[11]

Leveraging SN Ia spectroscopic similarity to improve the measurement of H $_{0}$

et al.

- JCAP 11 (2023) 046
•
e-Print:
- 2306.00070
•
DOI:
- 10.1088/1475-7516/2023/11/046

[12]

Instability in interacting dark energy and dark matter fluids

Jussi Valiviita
(
- Portsmouth U.
)
,
Elisabetta Majerotto
(
- Portsmouth U.
)
,
Roy Maartens
(
- Portsmouth U.
)

- JCAP 07 (2008) 020
•
e-Print:
- 0804.0232
•
DOI:
- 10.1088/1475-7516/2008/07/020

[13]

Dark coupling

M.B. Gavela
(
- Madrid, IFT and
- Madrid, Autonoma U.
)
,
D. Hernandez
(
- Madrid, IFT and
- Madrid, Autonoma U.
)
,
L. Lopez Honorez
(
- Madrid, IFT and
- Madrid, Autonoma U. and
- Brussels U.
)
,
O. Mena
(
- Valencia U., IFIC and
- Valencia U.
)
,
S. Rigolin
(
- Padua U. and
- INFN, Padua
)

- JCAP 07 (2009) 034,
- JCAP 05 (2010) E01 (erratum)
•
e-Print:
- 0901.1611
•
DOI:
- 10.1088/1475-7516/2009/07/034

[13]

Dark coupling

M.B. Gavela
(
- Madrid, IFT and
- Madrid, Autonoma U.
)
,
D. Hernandez
(
- Madrid, IFT and
- Madrid, Autonoma U.
)
,
L. Lopez Honorez
(
- Madrid, IFT and
- Madrid, Autonoma U. and
- Brussels U.
)
,
O. Mena
(
- Valencia U., IFIC and
- Valencia U.
)
,
S. Rigolin
(
- Padua U. and
- INFN, Padua
)

- JCAP 07 (2009) 034,
- JCAP 05 (2010) E01 (erratum)
•
e-Print:
- 0901.1611
•
DOI:
- 10.1088/1475-7516/2009/07/034

[14]

Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests

Kazuharu Bamba
(
- KMI, Nagoya
)
,
Salvatore Capozziello
(
- INFN, Naples and
- Naples U.
)
,
Shin'ichi Nojiri
(
- Nagoya U. and
- KMI, Nagoya
)
,
Sergei D. Odintsov
(
- Eurasian Nat. U., Astana and
- Tomsk Pedagogical Inst. and
- Barcelona, IEEC and
- ICREA, Barcelona
)

- Astrophys.Space Sci. 342 (2012) 155-228
•
e-Print:
- 1205.3421
•
DOI:
- 10.1007/s10509-012-1181-8

[15]

Indications of a late-time interaction in the dark sector

Valentina Salvatelli
(
- INFN, Rome and
- Rome U.
)
,
Najla Said
(
- INFN, Rome and
- Rome U.
)
,
Marco Bruni
(
- Portsmouth U., ICG
)
,
Alessandro Melchiorri
(
- INFN, Rome and
- Rome U.
)
,
David Wands
(
- Portsmouth U., ICG
)

- Phys.Rev.Lett. 113 (2014) 18, 181301
•
e-Print:
- 1406.7297
•
DOI:
- 10.1103/PhysRevLett.113.181301

[16]

Dark matter-dark energy interaction for a time-dependent EoS parameter

Rafael C. Nunes
(
- Rio Grande do Norte U. and
- Brasilia U.
)
,
Edesio M. Barboza
(
- Rio Grande do Norte U.
)

- Gen.Rel.Grav. 46 (2014) 1820
•
e-Print:
- 1404.1620
•
DOI:
- 10.1007/s10714-014-1820-1

[17]

Exploring dark matter microphysics with galaxy surveys

Miguel Escudero
(
- Valencia U., IFIC
)
,
Olga Mena
(
- Valencia U., IFIC
)
,
Aaron C. Vincent
(
- Durham U., IPPP
)
,
Ryan J. Wilkinson
(
- Durham U., IPPP
)
,
Céline Bœhm
(
- Durham U., IPPP
)

- JCAP 09 (2015) 034
•
e-Print:
- 1505.06735
•
DOI:
- 10.1088/1475-7516/2015/9/034

[18]

First evidence of running cosmic vacuum: challenging the concordance model

Joan Solà
(
- Barcelona U., ECM and
- ICC, Barcelona U.
)
,
Adria Gómez-Valent
(
- Barcelona U., ECM and
- ICC, Barcelona U.
)
,
Javier de Cruz Pérez
(
- Barcelona U., ECM and
- ICC, Barcelona U.
)

- Astrophys.J. 836 (2017) 1, 43
•
e-Print:
- 1602.02103
•
DOI:
- 10.3847/1538-4357/836/1/43

[19]

Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures

- Rept.Prog.Phys. 79 (2016) 9, 096901
•
e-Print:
- 1603.08299
•
DOI:
- 10.1088/0034-4885/79/9/096901

[20]

Probing the interaction between dark matter and dark energy in the presence of massive neutrinos

- Phys.Rev.D 94 (2016) 12, 123511
•
e-Print:
- 1608.02454
•
DOI:
- 10.1103/PhysRevD.94.123511

[21]

Constraints on the Coupling between Dark Energy and Dark Matter from CMB data

Riccardo Murgia
(
- INFN, Turin and
- Turin U. and
- SISSA, Trieste
)
,
Stefano Gariazzo
(
- INFN, Turin and
- Turin U.
)
,
Nicolao Fornengo
(
- INFN, Turin and
- Turin U.
)

- JCAP 04 (2016) 014
•
e-Print:
- 1602.01765
•
DOI:
- 10.1088/1475-7516/2016/04/014

[22]

Reconciling CMB and structure growth measurements with dark energy interactions

- Phys.Rev.D 94 (2016) 4, 043518
•
e-Print:
- 1604.04222
•
DOI:
- 10.1103/PhysRevD.94.043518

[23]

Possible signals of vacuum dynamics in the Universe

Joan Solà Peracaula
(
- Barcelona U. and
- ICC, Barcelona U.
)
,
Javier de Cruz Pérez
(
- Barcelona U. and
- ICC, Barcelona U.
)
,
Adria Gomez-Valent
(
- Barcelona U. and
- ICC, Barcelona U.
)

- Mon.Not.Roy.Astron.Soc. 478 (2018) 4, 4357-4373
•
e-Print:
- 1703.08218
•
DOI:
- 10.1093/mnras/sty1253

1-25 of 176
1
2
3
4
5
•••
8
25 / page