Fetching the paper…

Reading the bibliography…

2023

Towards a possible solution to the Hubble tension with Horndeski gravity

Tiwari, Yashi, Ghosh, Basundhara, Jain, Rajeev Kumar

Original
PDF
Post on X

Understand

The Hubble tension refers to the discrepancy in the value of the Hubble constant $H_0$ inferred from the cosmic microwave background observations, assuming the concordance $\Lambda$CDM model of the Universe, and that from the distance ladder and other direct measurements.

In order to alleviate this tension, we construct a plausible dark energy scenario, within the framework of Horndeski gravity which is one of the most general scalar-tensor theories yielding second-order equations.
In our set-up, we include the self-interactions and nonminimal coupling of the dynamical dark energy scalar field which enable very interesting dynamics leading to a phantom behaviour at low redshifts along with negative dark energy densities at high redshifts.
These two features together make this model a promising scenario to alleviate the Hubble tension for appropriate choices of the model parameters.

Towards a possible solution to the Hubble tension with Horndeski gravity · Around

Built on

C. D. Kreisch, F.-Y. Cyr-Racine, and O. Doré,
Original
1902
Earlier work this paper cites.
O. Akarsu, J. D. Barrow, C. V. R. Board, N. M. Uzun, and J. A. Vazquez,
Original
1903
Earlier work this paper cites.
P. Agrawal, F.-Y. Cyr-Racine, D. Pinner, and L. Randall, (2019),
Original
1904
Earlier work this paper cites.
S. Alexander and E. McDonough,
Original
1904
Earlier work this paper cites.
M.-X. Lin, G. Benevento, W. Hu, and M. Raveri,
Original
1905
Earlier work this paper cites.
E. Di Valentino, R. Z. Ferreira, L. Visinelli, and U. Danielsson,
Original
1906
Earlier work this paper cites.
X. Li and A. Shafieloo,
Original
1906
Earlier work this paper cites.
L. Verde, T. Treu, and A. G. Riess,
Original
1907
Earlier work this paper cites.
N. Schöneberg, J. Lesgourgues, and D. C. Hooper,
Original
1907
Earlier work this paper cites.
S. Vagnozzi,
Original
1907
Earlier work this paper cites.
L. Visinelli, S. Vagnozzi, and U. Danielsson,
Original
1907
Earlier work this paper cites.
L. Knox and M. Millea,
Original
1908
Earlier work this paper cites.
T. L. Smith, V. Poulin, and M. A. Amin,
Original
1908
Earlier work this paper cites.
E. Di Valentino, A. Melchiorri, and J. Silk,
Original
1908
Earlier work this paper cites.
F. Niedermann and M. S. Sloth,
Original
1910
Earlier work this paper cites.
A. Lewis, (2019),
Original
1910
Earlier work this paper cites.
K. V. Berghaus and T. Karwal,
Original
1911
Earlier work this paper cites.
J. Sakstein and M. Trodden,
Original
1911
Earlier work this paper cites.
O. Akarsu, J. D. Barrow, L. A. Escamilla, and J. A. Vazquez,
Original
1912
Earlier work this paper cites.
S. Tsujikawa,
Original
1961
Earlier work this paper cites.
A. I. Vainshtein,
1972
Earlier work this paper cites.
G. W. Horndeski,
1974
Earlier work this paper cites.
A. G. Riess
1998
Earlier work this paper cites.
S. Perlmutter
1999
Earlier work this paper cites.
D. W. Pesce
Original
2001
Earlier work this paper cites.
C. Krishnan, E. O. Colgáin, Ruchika, A. A. Sen, M. M. Sheikh-Jabbari, and T. Yang,
Original
2002
Earlier work this paper cites.
M. Zumalacarregui,
Original
2003
Earlier work this paper cites.
M. Moresco, R. Jimenez, L. Verde, A. Cimatti, and L. Pozzetti,
Original
2003
Earlier work this paper cites.
J. Khoury and A. Weltman,
2004
Earlier work this paper cites.
M. Braglia, M. Ballardini, W. T. Emond, F. Finelli, A. E. Gumrukcuoglu, K. Koyama, and D. Paoletti,
Original
2004
Earlier work this paper cites.
G. Alestas, L. Kazantzidis, and L. Perivolaropoulos,
Original
2004
Earlier work this paper cites.
B. Bayarsaikhan, S. Koh, E. Tsedenbaljir, and G. Tumurtushaa,
Original
2005
Earlier work this paper cites.
E. Di Valentino, A. Mukherjee, and A. A. Sen,
Original
2005
Earlier work this paper cites.

Similar

E. J. Copeland, M. Sami, and S. Tsujikawa,
2006
Cited alongside, same era.
F. Niedermann and M. S. Sloth,
Original
2006
Cited alongside, same era.
Y. Fujii and K. Maeda,
2007
Cited alongside, same era.
H. du Mas des Bourboux
Original
2007
Cited alongside, same era.
T. Adi and E. D. Kovetz,
Original
2011
Cited alongside, same era.
A. Bonilla, S. Kumar, and R. C. Nunes,
Original
2011

Then

J. P. Blakeslee, J. B. Jensen, C.-P. Ma, P. A. Milne, and J. E. Greene,
Original
2021
Later among the works it cites.
P. Shah, P. Lemos, and O. Lahav,
Original
2021
Later among the works it cites.
S. A. Adil, M. R. Gangopadhyay, M. Sami, and M. K. Sharma,
Original
2021
Later among the works it cites.
M. Petronikolou, S. Basilakos, and E. N. Saridakis, (2021),
Original
2021
Later among the works it cites.
E. V. Linder, (2021),
Original
2021
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Cited alongside, same era.

T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis,

2012

Cited alongside, same era.

A. De Felice and S. Tsujikawa,

2012

Cited alongside, same era.

V. Sahni, A. Shafieloo, and A. A. Starobinsky,

2014

Cited alongside, same era.

Original

2014

Cited alongside, same era.

2015

Cited alongside, same era.

2015

Cited alongside, same era.

D. Camarena and V. Marra,

2021

Later among the works it cites.

2022

Later among the works it cites.

G. S. Anand, R. B. Tully, L. Rizzi, A. G. Riess, and W. Yuan,

2022

Later among the works it cites.

T. de Jaeger, L. Galbany, A. G. Riess, B. E. Stahl, B. J. Shappee, A. V. Filippenko, and W. Zheng,

2022

Later among the works it cites.

O. H. E. Philcox and M. M. Ivanov,

2022

Later among the works it cites.

L. Perivolaropoulos and F. Skara,

Original

2022

Later among the works it cites.

2022

Later among the works it cites.

L. Herold and E. G. M. Ferreira, (2022),

2022

Later among the works it cites.

K. Rezazadeh, A. Ashoorioon, and D. Grin, (2022),

2022

Later among the works it cites.

K. V. Berghaus and T. Karwal, (2022),

2022

Later among the works it cites.

A. Adil, A. Albrecht, and L. Knox, (2022),

2022

Later among the works it cites.

B.-H. Lee, W. Lee, E. O. Colgáin, M. M. Sheikh-Jabbari, and S. Thakur,

2022

Later among the works it cites.

S. Gariazzo, E. Di Valentino, O. Mena, and R. C. Nunes,

2022

Later among the works it cites.

S. Banerjee, M. Petronikolou, and E. N. Saridakis, (2022),

2022

Later among the works it cites.

C.-H. Chien, S. Koh, and G. Tumurtushaa,

2022

Later among the works it cites.

Y. Tiwari, N. Bhaumik, and R. K. Jain, (2022),

2022

Later among the works it cites.

A. Mehrabi and M. Vazirnia,

2022

Later among the works it cites.

A. A. Sen, S. A. Adil, and S. Sen,

2022

Later among the works it cites.

I. S. Matos, E. Bellini, M. O. Calvão, and M. Kunz, (2022),

2022

Later among the works it cites.

2023

Closest in time.

2023

Closest in time.

Y.-H. Yao and X.-H. Meng,

2023

Closest in time.

M. Petronikolou and E. N. Saridakis,

2023

Closest in time.

L. Heisenberg, H. Villarrubia-Rojo, and J. Zosso,

2023

Closest in time.

M. Malekjani, R. M. Conville, E. O. Colgáin, S. Pourojaghi, and M. M. Sheikh-Jabbari, (2023),

2023

Closest in time.

S. A. Adil, O. Akarsu, E. Di Valentino, R. C. Nunes, E. Ozulker, A. A. Sen, and E. Specogna, (2023),

Original

2023

Closest in time.

A. G. Ferrari, M. Ballardini, F. Finelli, D. Paoletti, and N. Mauri, (2023),

2023

Closest in time.

A. Gómez-Valent, A. Favale, M. Migliaccio, and A. A. Sen, (2023),

2023

Closest in time.