Cosmic acceleration in non-canonical scalar field model - An interacting scenario - INSPIRE

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Cosmic acceleration in non-canonical scalar field model - An interacting scenario

Sudipta Das
(
- Visva Bharati U.
)
,
Abdulla Al Mamon
(
- Visva Bharati U.
)

Jul 7, 2014

10 pages

Published in:

Astrophys.Space Sci. 355 (2015) 2, 371-380

Published: Dec 4, 2014

e-Print:

1407.1666 [gr-qc]

DOI:

10.1007/s10509-014-2168-4

View in:

ADS Abstract Service

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Abstract: (Springer)

In this paper we have studied the dynamics of accelerating scenario within the framework of scalar field models possessing a non-canonical kinetic term. In this toy model, the scalar field is allowed to interact with the dark matter component through a source term. We have assumed a specific form for the coupling term and then have studied the dynamics of the scalar field having a constant equation of state parameter. We have also carried out the dynamical system study of such interacting non-canonical scalar field models for power law potentials for some physically relevant specific values of the model parameters. It has been found that the only for two particular stable fixed points of the system, an accelerating solution is possible and the universe will settle down to a ΛCDM universe in future and thus there is no future singularity in this model.

Note:

15 pages, 7 figures; Included few missing expressions; typos corrected •
18 pages, 10 figures; typos corrected, added more figures, matches published version

Dark energy
Non-canonical scalar field
Interaction
field theory: scalar
expansion: acceleration
equation of state
dynamical system
cosmological model
gravitation: model
dark matter

References(66)

Figures(7)

[1]

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

[2]

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

[3]

Quintessence: a mini-review

Jerome Martin

- Mod.Phys.Lett.A 23 (2008) 1252-1265
•
e-Print:
- 0803.4076
•
DOI:
- 10.1142/S0217732308027631

[4]

Dark matter and dark energy

Varun Sahni
(
- IUCAA, Pune
)

- Lect.Notes Phys. 653 (2004) 141-180,
•
e-Print:
- astro-ph/0403324
•
DOI:
- 10.1007/b99562

[5]

:

S. Tsujikawa

- Class.Quant.Grav. 30 (2013) 21400

[6]

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

[7]

Unified cosmic history in modified gravity: from F(R) theory to Lorentz non-invariant models

Shin'ichi Nojiri
(
- KMI, Nagoya and
- Nagoya U.
)
,
Sergei D. Odintsov
(
- ICE, Bellaterra and
- ICREA, Barcelona
)

- Phys.Rept. 505 (2011) 59-144
•
e-Print:
- 1011.0544
•
DOI:
- 10.1016/j.physrep.2011.04.001

[8]

An Alternative to quintessence

Alexander Yu. Kamenshchik
(
- Landau Inst. and
- Landau Network Centro Volta
)
,
Ugo Moschella
(
- Insubria U., Como and
- INFN, Milan
)
,
Vincent Pasquier
(
- Saclay
)

- Phys.Lett.B 511 (2001) 265-268
•
e-Print:
- gr-qc/0103004
•
DOI:
- 10.1016/S0370-2693(01)00571-8

[9]

Generalized Chaplygin gas, accelerated expansion and dark energy matter unification

- Phys.Rev.D 66 (2002) 043507
•
e-Print:
- gr-qc/0202064
•
DOI:
- 10.1103/PhysRevD.66.043507

[10]

A Quintessence scalar field in Brans-Dicke theory

- Class.Quant.Grav. 18 (2001) 593
•
e-Print:
- gr-qc/0012098
•
DOI:
- 10.1088/0264-9381/18/4/302

[11]

Nonminimal coupling and quintessence

O. Bertolami
(
- New York U.
)
,
P.J. Martins
(
- Lisbon, IST
)

- Phys.Rev.D 61 (2000) 064007
•
e-Print:
- gr-qc/9910056
•
DOI:
- 10.1103/PhysRevD.61.064007

[12]

Late-time cosmology in (phantom) scalar-tensor theory: Dark energy and the cosmic speed-up

Emilio Elizalde
(
- CSIC, Catalunya and
- Barcelona, IEEC
)
,
Shin'ichi Nojiri
(
- Japan, Natl. Defence Academy
)
,
Sergei D. Odintsov
(
- ICREA, Barcelona and
- Barcelona, IEEC
)

- Phys.Rev.D 70 (2004) 043539
•
e-Print:
- hep-th/0405034
•
DOI:
- 10.1103/PhysRevD.70.043539

[13]

Superacceleration from massless, minimally coupled phi**4

V.K. Onemli
(
- Florida U.
)
,
R.P. Woodard
(
- Florida U.
)

- Class.Quant.Grav. 19 (2002) 4607
•
e-Print:
- gr-qc/0204065
•
DOI:
- 10.1088/0264-9381/19/17/311

[14]

Cosmology in scalar tensor theory and asymptotically de Sitter universe

- Mod.Phys.Lett.A 16 (2001) 1303-1314
•
e-Print:
- gr-qc/0103098
•
DOI:
- 10.1142/S021773230100442X

[15]

Selfinteracting Brans-Dicke cosmology and quintessence

- Int.J.Mod.Phys.D 12 (2003) 445-460
•
e-Print:
- gr-qc/0007079
•
DOI:
- 10.1142/S0218271803003049

[16]

:

S. Carloni
,
P.K.S. Dunsby
,
S. Capozziello
,
A. Troisi

- Class.Quant.Grav. 22 (2005) 48399

[17]

Is Cosmic Speed-Up Due to New Gravitational Physics?

Sean M. Carroll
(
- Chicago U., EFI and
- Chicago U. and
- Chicago U., KICP
)
,
Vikram Duvvuri
(
- Chicago U., EFI and
- Chicago U. and
- Chicago U., KICP
)
,
Mark Trodden
(
- Syracuse U.
)
,
Michael S. Turner
(
- Chicago U., EFI and
- Chicago U. and
- Chicago U., KICP and
- Chicago U., Astron. Astrophys. Ctr. and
- Fermilab
)

- Phys.Rev.D 70 (2004) 043528
•
e-Print:
- astro-ph/0306438
•
DOI:
- 10.1103/PhysRevD.70.043528

[18]

Modified gravity with negative and positive powers of the curvature: Unification of the inflation and of the cosmic acceleration

- Phys.Rev.D 68 (2003) 123512
•
e-Print:
- hep-th/0307288
•
DOI:
- 10.1103/PhysRevD.68.123512

[19]

1/R Curvature corrections as the source of the cosmological acceleration

Dan N. Vollick
(
- Okanagan Coll.
)

- Phys.Rev.D 68 (2003) 063510
•
e-Print:
- astro-ph/0306630
•
DOI:
- 10.1103/PhysRevD.68.063510

[20]

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

[21]

Haloes of k-essence

C. Armendariz-Picon
(
- Syracuse U.
)
,
Eugene A. Lim
(
- Yale U.
)

- JCAP 08 (2005) 007
•
e-Print:
- astro-ph/0505207
•
DOI:
- 10.1088/1475-7516/2005/08/007

[22]

Unified Dark Matter in Scalar Field Cosmologies

Daniele Bertacca
(
- Padua U. and
- INFN, Padua
)
,
Sabino Matarrese
(
- Padua U. and
- INFN, Padua
)
,
Massimo Pietroni
(
- INFN, Padua
)

- Mod.Phys.Lett.A 22 (2007) 2893-2907
•
e-Print:
- astro-ph/0703259
•
DOI:
- 10.1142/S0217732307025893

[23]

Halos of Unified Dark Matter Scalar Field

Daniele Bertacca
(
- Padua U. and
- INFN, Padua
)
,
Nicola Bartolo
(
- Padua U. and
- INFN, Padua
)
,
Sabino Matarrese
(
- Padua U. and
- INFN, Padua
)

- JCAP 05 (2008) 005
•
e-Print:
- 0712.0486
•
DOI:
- 10.1088/1475-7516/2008/05/005

[24]

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

[25]

Tachyon Field in Intermediate Inflation

- Phys.Rev.D 79 (2009) 083507
•
e-Print:
- 0904.1032
•
DOI:
- 10.1103/PhysRevD.79.083507

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