J-PAS: forecasts for dark matter-dark energy elastic couplings

被引:16
|
作者
Figueruelo, David [1 ,2 ]
Aparicio Resco, Miguel [3 ,4 ]
Teppa Pannia, Florencia A. [1 ,2 ]
Beltran Jimenez, Jose [1 ,2 ]
Bettoni, Dario [1 ,2 ]
Maroto, Antonio L. [3 ,4 ]
Abramo, L. Raul [5 ]
Alcaniz, Jailson [6 ]
Benitez, Narciso [7 ,12 ]
Bonoli, Silvia [8 ,9 ,10 ]
Carneiro, Saulo [11 ]
Cenarro, Javier [8 ]
Cristobal-Hornillos, David [8 ]
Dupke, Renato A. [6 ,13 ,14 ]
Ederoclite, Alessandro [15 ]
Lopez-Sanjuan, Carlos [8 ]
Marin-Franch, Antonio [8 ]
Marra, Valerio [16 ,17 ,18 ,19 ]
de Oliveira, Claudia Mendes [15 ]
Moles, Mariano [7 ,8 ]
Sodre, Laerte, Jr. [15 ]
Taylor, Keith [20 ]
Varela, Jesus [8 ]
Vazquez Ramio, Hector [8 ]
机构
[1] Univ Salamanca, Dept Fis Fundamental, E-37008 Salamanca, Spain
[2] Univ Salamanca, IUFFyM, E-37008 Salamanca, Spain
[3] Univ Complutense Madrid, Dept Fis Teor, Madrid 28040, Spain
[4] Univ Complutense Madrid, Inst Fis Particulas & Cosmos IPARCOS, Madrid 28040, Spain
[5] Univ Sao Paulo, Inst Fis, Rua Matao 1371, BR-05508090 Sao Paulo, Brazil
[6] Observ Nacl, Rua Gen Jose Cristino 77, BR-20921400 Rio De Janeiro, Brazil
[7] CSIC, Inst Astrofis Andalucia, Apdo 3004, E-18080 Granada, Spain
[8] CSIC, Unidad Asociada, Ctr Estudios Fis Cosmos Aragon CEFCA, Plaza San Juan 1, E-44001 Teruel, Spain
[9] Donostia Int Phys Ctr DIPC, Manuel Lardizabal Ibilbidea 4, San Sebastian, Spain
[10] Basque Fdn Sci, Ikerbasque, E-48013 Bilbao, Spain
[11] Univ Fed Bahia, Inst Fis, BR-40210340 Salvador, BA, Brazil
[12] Abante Asesores, Plaza Independencia 6, Madrid 28001, Spain
[13] Univ Michigan, Dept Astron, 311West Hall,1085 South Univ Ave, Ann Arbor, MI 48109 USA
[14] Univ Alabama, Dept Phys & Astron, Box870324, Tuscaloosa, AL 35487 USA
[15] Univ Sao Paulo, Dept Astron, Inst Astron, Geofisicae Ciencias Atmosfer, Sao Paulo, Brazil
[16] Univ Fed Espirito Santo, Nucleo Astrofis & Cosmol, BR-29075910 Vitoria, ES, Brazil
[17] Univ Fed Espirito Santo, Dept Fis, BR-29075910 Vitoria, ES, Brazil
[18] INAF Osservatorio Astron Trieste, Via Tiepolo 11, I-34131 Trieste, Italy
[19] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34151 Trieste, Italy
[20] Instruments4, 4121 Pembury Pl, La Canada Flintridge, CA 91011 USA
基金
巴西圣保罗研究基金会;
关键词
dark energy theory; dark matter theory; BARYON ACOUSTIC-OSCILLATIONS; MOMENTUM EXCHANGE; REDSHIFT;
D O I
10.1088/1475-7516/2021/07/022
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider a cosmological model where dark matter and dark energy feature a coupling that only affects their momentum transfer in the corresponding Euler equations. We perform a fit to cosmological observables and confirm previous findings within these scenarios that favour the presence of a coupling at more than 3a. This improvement is mainly driven by cluster counts from Planck Sunyaev-Zeldovich data that we include as a certain prior. We subsequently perform a forecast for future J-PAS data and find that clustering measurements will permit to clearly discern the presence of an interaction within a few percent level with the uncoupled case at more than 10o(-) when the complete survey, covering 8500 sq. deg., is considered. We found that the inclusion of weak lensing measurements will not help to further constrain the coupling parameter. For completeness, we compare to forecasts for DESI and Euclid, which provide similar discriminating power.
引用
收藏
页数:35
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