The Equation of State of Novel Double-Field Pure K-Essence for Inflation, Dark Matter and Dark Energy - INSPIRE

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The Equation of State of Novel Double-Field Pure K-Essence for Inflation, Dark Matter and Dark Energy

Changjun Gao
(
- NAOC, Beijing and
- Beijing, GUCAS
)

Feb 6, 2024

13 pages

Published in:

Universe 10 (2024) 6, 235,
Universe 10 (2024) 235

Published: May 24, 2024

e-Print:

2402.04460 [gr-qc]

DOI:

10.3390/universe10060235

View in:

ADS Abstract Service

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Abstract: (MDPI)

K-essence theories are usually studied in the framework of a single scalar field . Namely, the Lagrangian of K-essence is the function of the single scalar field and its covariant derivative. However, in this paper, we explore a double-field pure K-essence, i.e., the corresponding Lagrangian is the function of covariant derivatives of double scalar fields without a dependency on scalar fields themselves. This is why we call it double-field pure K-essence. The novelty of this K-essence is that its Lagrangian contains the quotient term of the kinetic energies from the two scalar fields. This results in the presence of many interesting features; for example, the equation of state can be arbitrarily small and arbitrarily large. In comparison, the range of the equation of state for quintessence is to . Interestingly, this novel K-essence can play the role of an inflation field, dark matter, or dark energy by appropriately selecting the expressions of Lagrangian.

Note:

12 pages,18 figures

K-essence
dark energy
field theory: scalar: multiple
derivative: covariance
energy: kinetic
dark energy
black hole
dark matter
equation of state
inflation: model

References(40)

Figures(18)

[1]

k - inflation

C. Armendariz-Picon
(
- Munich U.
)
,
T. Damour
(
- IHES, Bures-sur-Yvette and
- Stanford U., HEPL
)
,
Viatcheslav F. Mukhanov
(
- Munich U.
)

- Phys.Lett.B 458 (1999) 209-218
•
e-Print:
- hep-th/9904075
•
DOI:
- 10.1016/S0370-2693(99)00603-6

[2]

Perturbations in k-inflation

Jaume Garriga
(
- Munich U. and
- Barcelona, Autonoma U.
)
,
Viatcheslav F. Mukhanov
(
- Munich U.
)

- Phys.Lett.B 458 (1999) 219-225
•
e-Print:
- hep-th/9904176
•
DOI:
- 10.1016/S0370-2693(99)00602-4

[3]

Kinetically driven quintessence

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

[4]

A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration

C. Armendariz-Picon
(
- Munich U.
)
,
Viatcheslav F. Mukhanov
(
- Munich U.
)
,
Paul J. Steinhardt
(
- Princeton U.
)

- Phys.Rev.Lett. 85 (2000) 4438-4441
•
e-Print:
- astro-ph/0004134
•
DOI:
- 10.1103/PhysRevLett.85.4438

[5]

Essentials of k essence

C. Armendariz-Picon
(
- Munich U.
)
,
Viatcheslav F. Mukhanov
(
- Munich U.
)
,
Paul J. Steinhardt
(
- Princeton U.
)

- Phys.Rev.D 63 (2001) 103510
•
e-Print:
- astro-ph/0006373
•
DOI:
- 10.1103/PhysRevD.63.103510

[6]

Tracking K-essence

Takeshi Chiba
(
- Kyoto U.
)

- Phys.Rev.D 66 (2002) 063514
•
e-Print:
- astro-ph/0206298
•
DOI:
- 10.1103/PhysRevD.66.063514

[7]

Power - law expansion in k-essence cosmology

- Mod.Phys.Lett.A 19 (2004) 761-768
•
e-Print:
- astro-ph/0305007
•
DOI:
- 10.1142/S0217732304013507

[8]

Extended tachyon field, Chaplygin gas and solvable k-essence cosmologies

Luis P. Chimento
(
- Buenos Aires U.
)

- Phys.Rev.D 69 (2004) 123517
•
e-Print:
- astro-ph/0311613
•
DOI:
- 10.1103/PhysRevD.69.123517

[9]

K-essence and the coincidence problem

- Phys.Rev.D 68 (2003) 023512
•
e-Print:
- astro-ph/0304277
•
DOI:
- 10.1103/PhysRevD.68.023512

[10]

Purely kinetic k-essence as unified dark matter

Robert J. Scherrer
(
- Vanderbilt U.
)

- Phys.Rev.Lett. 93 (2004) 011301
•
e-Print:
- astro-ph/0402316
•
DOI:
- 10.1103/PhysRevLett.93.011301

[11]

Atypical k-essence cosmologies

Luis P. Chimento
(
- Buenos Aires U.
)
,
Ruth Lazkoz
(
- Basque U., Bilbao
)

- Phys.Rev.D 71 (2005) 023505
•
e-Print:
- astro-ph/0404494
•
DOI:
- 10.1103/PhysRevD.71.023505

[12]

On the stability of phantom k-essence theories

- Phys.Rev.D 73 (2006) 063522
•
e-Print:
- astro-ph/0511562
•
DOI:
- 10.1103/PhysRevD.73.063522

[13]

A no-go theorem for k-essence dark energy

- Phys.Rev.Lett. 97 (2006) 081303
•
e-Print:
- astro-ph/0606584
•
DOI:
- 10.1103/PhysRevLett.97.081303

[14]

A k-essence Model Of Inflation, Dark Matter and Dark Energy

- Phys.Rev.D 79 (2009) 103517
•
e-Print:
- 0812.4131
•
DOI:
- 10.1103/PhysRevD.79.103517

[15]

Unified Model of $k$ -Inflation, Dark Matter & Dark Energy

- Phys.Rev.D 80 (2009) 103508
•
e-Print:
- 0907.2330
•
DOI:
- 10.1103/PhysRevD.80.103508

[16]

Early dark energy in $k$ -essence

S.X. Tian
(
- Beijing Normal U.
)
,
Zong-Hong Zhu
(
- Beijing Normal U. and
- Wuhan U.
)

- Phys.Rev.D 103 (2021) 4, 043518
•
e-Print:
- 2102.06399
•
DOI:
- 10.1103/PhysRevD.103.043518

[17]

Cosmic Distances Calibrated to 1% Precision with Gaia EDR3 Parallaxes and Hubble Space Telescope Photometry of 75 Milky Way Cepheids Confirm Tension with $\Lambda$ CDM

et al.

- Astrophys.J.Lett. 908 (2021) 1, L6
•
e-Print:
- 2012.08534
•
DOI:
- 10.3847/2041-8213/abdbaf

[18]

Measurements of the Hubble Constant: Tensions in Perspective

Wendy L. Freedman
(
- Chicago U.
)

- Astrophys.J. 919 (2021) 1, 16
•
e-Print:
- 2106.15656
•
DOI:
- 10.3847/1538-4357/ac0e95

[19]

Is local H $_{0}$ at odds with dark energy EFT?

Bum-Hoon Lee
(
- CQUeST, Seoul and
- Sogang U.
)
,
Wonwoo Lee
(
- CQUeST, Seoul
)
,
Eoin Ó. Colgáin
(
- CQUeST, Seoul and
- Sogang U.
)
,
M.M. Sheikh-Jabbari
(
- IPM, Tehran
)
,
Somyadip Thakur
(
- CQUeST, Seoul and
- Sogang U.
)

- JCAP 04 (2022) 04, 004
•
e-Print:
- 2202.03906
•
DOI:
- 10.1088/1475-7516/2022/04/004

[20]

Late-time acceleration due to a generic modification of gravity and the Hubble tension

- Phys.Rev.D 104 (2021) 10, 103534
•
e-Print:
- 2106.03093
•
DOI:
- 10.1103/PhysRevD.104.103534

[21]

New generic evolution for $k$ -essence dark energy with $w \approx -1$

- Phys.Rev.D 100 (2019) 2, 023525
•
e-Print:
- 1905.05628
•
DOI:
- 10.1103/PhysRevD.100.023525

[22]

Dynamical Stability and Geometrical Diagnostic of the Power Law K-Essence Dark Energy Model with Interaction

Bo-Hai Chen
(
- Liaoning Normal U. and
- Langfang, Inst. Aerosp. Engin.
)
,
Ya-Bo Wu
(
- Liaoning Normal U.
)
,
Dong-Fang Xu
(
- Liaoning Normal U.
)
,
Wei Dong
(
- Liaoning Normal U.
)
,
Nan Zhang
(
- Liaoning Normal U. and
- PCFT, Hefei
)

- Universe 6 (2020) 12, 244
•
DOI:
- 10.3390/universe6120244

[23]

The Phase Space Analysis of Interacting K-Essence Dark Energy Models in Loop Quantum Cosmology

Bohai Chen
(
- Liaoning Normal U. and
- Goyang, Korea Aerospace U.
)
,
Yabo Wu
(
- Liaoning Normal U.
)
,
Jianan Chi
(
- Liaoning Normal U.
)
,
Wenzhong Liu
(
- Liaoning Normal U.
)
,
Yiliang Hu
(
- Liaoning Normal U.
)

- Universe 8 (2022) 10, 520
•
DOI:
- 10.3390/universe8100520

[24]

k-Essence Inflation Evading Swampland Conjectures and Inflationary Parameters

Abdul Jawad
(
- COMSATS, Lahore
)
,
Shamaila Rani
(
- COMSATS, Lahore
)
,
Abdul Malik Sultan
(
- COMSATS, Lahore and
- Education U., Okara
)
,
Kashaf Embreen
(
- COMSATS, Lahore
)

- Universe 8 (2022) 10, 532
•
DOI:
- 10.3390/universe8100532

[25]

Quintom Fields from Chiral K-Essence Cosmology

José Socorro
(
- Guanajuato U.
)
,
Sinuhé Pérez-Payán
(
- UPII, IPN
)
,
Rafael Hernández-Jiménez
(
- Guadalajara U.
)
,
Abraham Espinoza-García
(
- UPII, IPN
)
,
Luis Rey Díaz-Barrón
(
- UPII, IPN
)

- Universe 8 (2022) 10, 548,
- Universe 8 (2022) 00548
•
e-Print:
- 2204.12083
•
DOI:
- 10.3390/universe8100548

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