Abstract
We study detectability of the deviation in interacting and non-interacting cubic Galileon models from the \(\Lambda \)CDM model through the 21-cm power spectrum. We show that the interferometric observations like the upcoming SKA1-mid can detect the deviations in both interacting and non-interacting cubic Galileon model from the \(\Lambda \)CDM model depending on the parameter values.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Abbott B. P., et al. (LIGO Scientific, Virgo, Fermi-GBM, INTEGRAL), 2017a, Astrophys. J. Lett., 848, L13. https://doi.org/10.3847/2041-8213/aa920c, arXiv:1710.05834
Abbott B. P., et al. (LIGO Scientific, Virgo), 2017b, Phys. Rev. Lett., 119, 161101. https://doi.org/10.1103/PhysRevLett.119.161101, arXiv:1710.05832
Abbott B. P., et al. 2017c, Astrophys. J. Lett., 848, L12. https://doi.org/10.3847/2041-8213/aa91c9, arXiv: 1710.05833
Ade P. A. R., et al. (Planck), 2016, Astron. Astrophys., 594, A13. https://doi.org/10.1051/0004-6361/201525830, arXiv:1502.01589
Aghanim N., et al. (Planck), 2020, Astron. Astrophys., 641, A6. https://doi.org/10.1051/0004-6361/201833910, arXiv:1807.06209 (Erratum: Astron. Astrophys. 652, C4 (2021))
Ali A., Gannouji R., Hossain M. W., Sami M. 2012, Phys. Lett. B, 718, 5. https://doi.org/10.1016/j.physletb.2012.10.009, arXiv: 1207.3959
Ali A., Gannouji R., Sami M. 2010, Phys. Rev. D, 82, 103015. https://doi.org/10.1103/PhysRevD.82.103015. arXiv:1008.1588
Ali S. S., Bharadwaj S., Pandey S. K. 2006, Mon. Not. Roy. Astron. Soc., 366, 213. https://doi.org/10.1111/j.1365-2966.2005.09847.x. arXiv:astro-ph/0510118
Andriot D., 2018. Phys. Lett. B, 785, 570. https://doi.org/10.1016/j.physletb.2018.09.022, arXiv:1806.10999
Bacon D. J., et al. (SKA), 2020, Publ. Astron. Soc. Austral., 37, e007. https://doi.org/10.1017/pasa.2019.51, arXiv:1811.02743
Ballinger W. E., Peacock J. A., Heavens A. F. 1996, Mon. Not. Roy. Astron. Soc., 282, 877. https://doi.org/10.1093/mnras/282.3.877. arXiv:astro-ph/9605017
Barreira A., Li B., Hellwing W. A., Baugh C. M., Pascoli S. 2013, JCAP, 10, 027. https://doi.org/10.1088/1475-7516/2013/10/027. arXiv:1306.3219
Bartolo N., Bellini E., Bertacca D., Matarrese S. 2013, JCAP, 03, 034. https://doi.org/10.1088/1475-7516/2013/03/034. arXiv:1301.4831
Bellini E., Jimenez R. 2013, Phys. Dark Univ., 2, 179. https://doi.org/10.1016/j.dark.2013.11.001, arXiv:1306.1262
Bharadwaj S., Ali S. S. 2005, Mon. Not. Roy. Astron. Soc., 356, 1519. https://doi.org/10.1111/j.1365-2966.2004.08604.x. arXiv:astro-ph/0406676
Brahma S., Hossain M. W. 2019, JHEP, 06, 070. https://doi.org/10.1007/JHEP06(2019)070, arXiv:1902.11014
Brahma S., Hossain M. W. 2021, Universe, 7, 167. https://doi.org/10.3390/universe7060167, arXiv:2007.06425
Braun R., Bonaldi A., Bourke T., Keane E., Wagg J. 2019, arXiv:1912.12699
Bull P., Ferreira P. G., Patel P., Santos M. G. 2015, Astrophys. J., 803, 21. https://doi.org/10.1088/0004-637X/803/1/21. arXiv:1405.1452
Chow N., Khoury J. 2009, Phys. Rev. D, 80, 024037. https://doi.org/10.1103/PhysRevD.80.024037. arXiv:0905.1325
Clifton T., Ferreira P. G., Padilla A., Skordis C. 2012, Phys. Rept., 513, 1. https://doi.org/10.1016/j.physrep.2012.01.001. arXiv:1106.2476
Copeland E. J., Sami M., Tsujikawa S. 2006, Int. J. Mod. Phys. D, 15, 1753. https://doi.org/10.1142/S021827180600942X. arXiv:hep-th/0603057
Datta K. K., Choudhury T. R., Bharadwaj S. 2007, Mon. Not. Roy. Astron. Soc., 378, 119. https://doi.org/10.1111/j.1365-2966.2007.11747.x. arXiv:astro-ph/0605546
De Felice A., Mukohyama S., Tsujikawa S. 2010, Phys. Rev. D, 82, 023524. https://doi.org/10.1103/PhysRevD.82.023524. arXiv: 1006.0281
De Felice A., Tsujikawa S. 2010a, Phys. Rev. Lett., 105, 111301. https://doi.org/10.1103/PhysRevLett.105.111301. arXiv: 1007.2700
De Felice A., Tsujikawa S. 2010b, Living Rev. Relativ., 13, 3. https://doi.org/10.12942/lrr-2010-3, arXiv: 1002.4928
Deffayet C., Esposito-Farese G., Vikman A. 2009, Phys. Rev. D, 79, 084003. https://doi.org/10.1103/PhysRevD.79.084003. arXiv: 0901.1314
Deffayet C., Pujolas O., Sawicki I., Vikman A. 2010, JCAP, 10, 026. https://doi.org/10.1088/1475-7516/2010/10/026. arXiv:1008.0048
de Rham C. 2012, Comptes Rendus Physique, 13, 666. https://doi.org/10.1016/j.crhy.2012.04.006. arXiv: 1204.54929
de Rham C. 2014, Living Rev. Relativ., 17, 7. https://doi.org/10.12942/lrr-2014-7, arXiv:1401.4173
de Rham C., Gabadadze G., Heisenberg L., Pirtskhalava D. 2011, Phys. Rev. D, 83, 103516. https://doi.org/10.1103/PhysRevD.83.103516. arXiv:1010.1780
de Rham C., Heisenberg L. 2011, Phys. Rev. D, 84, 043503. https://doi.org/10.1103/PhysRevD.84.043503. arXiv:1106.3312
Dinda B. R. 2018, JCAP, 06, 017. https://doi.org/10.1088/1475-7516/2018/06/017, arXiv: 1801.01741
Dinda B. R. 2022, Phys. Rev. D 105, 063524. https://doi.org/10.1103/PhysRevD.105.063524, arXiv: 2106.02963
Dinda B. R., Sen A. A., Choudhury T. R. 2018a, arXiv: 1804.11137
Dinda B. R., Wali Hossain M., Sen A. A. 2018b, JCAP, 01, 045. https://doi.org/10.1088/1475-7516/2018/01/045, arXiv: 1706.00567
Dvali G. R., Gabadadze G., Porrati M. 2000, Phys. Lett. B, 485, 208. https://doi.org/10.1016/S0370-2693(00)00669-9. arXiv: hep-th/0005016
Eisenstein D. J., Hu W. 1998, Astrophys. J., 496, 605. https://doi.org/10.1086/305424. arXiv: astro-ph/9709112
Ezquiaga J. M., Zumalacárregui M. 2017, Phys. Rev. Lett., 119, 251304. https://doi.org/10.1103/PhysRevLett.119.251304, arXiv: 1710.05901
Furlanetto S., Zaldarriaga M., Hernquist L. 2004, Astrophys. J., 613, 1. https://doi.org/10.1086/423025. arXiv: astro-ph/0403697
Gannouji R., Sami M. 2010, Phys. Rev. D, 82, 24011. https://doi.org/10.1103/PhysRevD.82.024011. arXiv:1004.2808
Geil P. M., Gaensler B. M. 2010, Mon. Not. Roy. Astron. Soc., 418, 516
Horndeski G. W. 1974, Int. J. Theor. Phys., 10, 363. DOI: 10.1007/BF01807638.
Hossain M. W. 2017, Phys. Rev. D, 96, 023506. https://doi.org/10.1103/PhysRevD.96.023506, arXiv:1704.07956
Hossain M. W., Sen A. A. 2012, Phys. Lett. B, 713, 140. https://doi.org/10.1016/j.physletb.2012.06.016, arXiv:1201.6192
Hotinli S. C., Binnie T., Muñoz J. B., Dinda B. R., Kamionkowski M. 2021, Phys. Rev. D, 104, 063536. https://doi.org/10.1103/PhysRevD.104.063536, arXiv: 2106.11979
Hussain A., Thakur S., Guha Sarkar T., Sen A. A. 2016, Mon. Not. Roy. Astron. Soc., 463, 3492. https://doi.org/10.1093/mnras/stw2246, arXiv:1603.02087
Kobayashi T. 2010, Phys. Rev. D, 81, 103533. https://doi.org/10.1103/PhysRevD.81.103533. arXiv:1003.3281
Kobayashi T., Tashiro H., Suzuki D. 2010, Phys. Rev. D, 81, 063513. https://doi.org/10.1103/PhysRevD.81.063513.
Kobayashi T., Yamaguchi M., Yokoyama J. 2011, Prog. Theor. Phys., 126, 511. https://doi.org/10.1143/PTP.126.511. arXiv:1105.5723
Linder E. V. 2008, Rept. Prog. Phys., 71, 056901. https://doi.org/10.1088/0034-4885/71/5/056901. arXiv: 0801.2968
Liu A., Parsons A. R. 2016, Mon. Not. Roy. Astron. Soc., 457, 1864. https://doi.org/10.1093/mnras/stw071, arXiv:1510.08815
Loeb A., Wyithe S. 2008, Phys. Rev. Lett., 100, 161301. https://doi.org/10.1103/PhysRevLett.100.161301. arXiv: 0801.1677
Luty M. A., Porrati M., Rattazzi R. 2003, JHEP, 09, 029. https://doi.org/10.1088/1126-6708/2003/09/029. arXiv:hep-th/0303116
Martin J., 2012, Comptes Rendus Physique, 13, 566. DOI: 10.1016/j.crhy.2012.04.008, arXiv:1205.3365.
McQuinn M., Zahn O., Zaldarriaga M., Hernquist L., Furlanetto S. R. 2006, Astrophys. J., 653, 815. https://doi.org/10.1086/505167. arXiv:astro-ph/0512263
Mota D. F., Sandstad M., Zlosnik T. 2010, JHEP, 12, 051. https://doi.org/10.1007/JHEP12(2010)051. arXiv:1009.6151
Nicolis A., Rattazzi R. 2004, JHEP, 06, 059. https://doi.org/10.1088/1126-6708/2004/06/059. arXiv:hep-th/0404159
Nicolis A., Rattazzi R., Trincherini E. 2009, Phys. Rev. D, 79, 064036. https://doi.org/10.1103/PhysRevD.79.064036. arXiv: 0811.2197
Nojiri S., Odintsov S. D., Oikonomou V. K. 2017, Phys. Rept., 692, 1. https://doi.org/10.1016/j.physrep.2017.06.001, arXiv: 1705.11098
Obied G., Ooguri H., Spodyneiko L., Vafa C. 2018, De Sitter Space and the Swampland, arXiv:1806.08362
Perlmutter S., et al. (Supernova Cosmology Project) 1999, Astrophys. J., 517, 565. https://doi.org/10.1086/307221, arXiv:astro-ph/9812133
Pesce D. W., et al. 2020, Astrophys. J. Lett., 891, L1. https://doi.org/10.3847/2041-8213/ab75f0, arXiv:2001.09213
Raccanelli A., et al. 2015, Measuring redshift-space distortions with future SKA surveys, arXiv:1501.03821
Renk J., Zumalacárregui M., Montanari F., Barreira A. 2017, JCAP, 10, 020. https://doi.org/10.1088/1475-7516/2017/10/020, arXiv:1707.02263
Riess A. G., Casertano S., Yuan W., Macri L. M., Scolnic D. 2019, Astrophys. J., 876, 85. https://doi.org/10.3847/1538-4357/ab1422, arXiv:1903.07603
Riess A. G., et al. (Supernova Search Team), 1998, Astron. J., 116, 1009. https://doi.org/10.1086/300499, arXiv:astro-ph/9805201
Sahni V., Starobinsky A. A. 2000, Int. J. Mod. Phys. D, 9, 373. https://doi.org/10.1142/S0218271800000542. arXiv:astro-ph/9904398
Sarkar T. G., Datta K. K. 2015, JCAP, 08, 001. https://doi.org/10.1088/1475-7516/2015/08/001, arXiv:1501.02308
Sarkar T. G., Mitra S., Majumdar S., Choudhury T. R. 2011, Monthly Notices of the Royal Astronomical Society, 421, 3570
Silva F. P., Koyama K. 2009, Phys. Rev. D, 80, 121301. https://doi.org/10.1103/PhysRevD.80.121301. arXiv:0909.4538
Silvestri A., Trodden M. 2009, Rept. Prog. Phys., 72, 096901. https://doi.org/10.1088/0034-4885/72/9/096901. arXiv:0904.0024
Vafa C. 2005, The String landscape and the swampland, arXiv:hep-th/0509212
Vainshtein A. I. 1972, Phys. Lett. B, 39, 393. https://doi.org/10.1016/0370-2693(72)90147-5
Villaescusa-Navarro F., Viel M., Datta K. K., Choudhury T. R. 2014, JCAP, 09, 050. https://doi.org/10.1088/1475-7516/2014/09/050. arXiv:1405.6713
Wong K. C., et al. 2020, Mon. Not. Roy. Astron. Soc., 498, 1420. https://doi.org/10.1093/mnras/stz3094, arXiv:1907.04869
Wyithe S., Loeb A. 2008, Mon. Not. Roy. Astron. Soc., 383, 606. https://doi.org/10.1111/j.1365-2966.2007.12568.x. arXiv:0708.3392
Wyithe S., Loeb A. 2009, Mon. Not. Roy. Astron. Soc., 397, 1926. https://doi.org/10.1111/j.1365-2966.2009.15019.x. arXiv:0808.2323
Zhang J., Dinda B. R., Hossain M. W., Sen A. A., Luo W. 2020, Phys. Rev. D, 102, 043510. https://doi.org/10.1103/PhysRevD.102.043510, arXiv:2004.12659
Zlatev I., Wang L. M., Steinhardt P. J. 1999, Phys. Rev. Lett., 82, 896. https://doi.org/10.1103/PhysRevLett.82.896. arXiv:astro-ph/9807002
Zumalacarregui M. 2020, Phys. Rev. D, 102, 023523. https://doi.org/10.1103/PhysRevD.102.023523, arXiv: 2003.06396
Acknowledgements
AAS acknowledges the funding from SERB, Government of India, under the research grant no: CRG/2020/004347. BRD would like to acknowledge IISER Kolkata, for the financial support through the postdoctoral fellowship.
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
About this article
Cite this article
Dinda, B.R., Hossain, M.W. & Sen, A.A. 21-cm power spectrum in interacting cubic Galileon model. J Astrophys Astron 44, 85 (2023). https://doi.org/10.1007/s12036-023-09976-2
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s12036-023-09976-2