Composite dark energy and the cosmological tensions

被引:2
作者
Gomez-Valent, Adria [1 ]
Peracaula, Joan Sola [1 ]
机构
[1] Univ Barcelona, Inst Cosmos Sci, Dept Fis Quant & Astrofis, Av Diagonal 647, E-08028 Barcelona, Catalonia, Spain
关键词
LUMINOUS RED GALAXIES; GROWTH-RATE; COSMIC STRUCTURE; POWER SPECTRUM; CONSTRAINTS; CONSTANT; DYNAMICS; MODELS; VACUUM; BOSS;
D O I
10.1016/j.physletb.2025.139391
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The standard cosmological model currently in force, aka Lambda CDM, has been plagued with a variety of phenomenological glitches or tensions in the last decade or so, which puts it against the wall. At the core of the Lambda CDM we have a rigid cosmological term, Lambda, for the entire cosmic history. This feature is unnatural and even inconsistent in the context of fundamental physics. Recently, the results from the DESI collaboration suggested the possibility that dark energy (DE) should be dynamical rather than just a cosmological constant. Using a generic w0wgCDM parameterization, DESI reported signs of quintessence behavior at 2.5-3.96 c.l. by combining their BAO data with CMB and different SNIa samples. However, to alleviate the tensions the DE needs more features. In the proposed wXCDM model [45], the DE is actually a composite cosmic fluid with two components (X, Y) acting sequentially: first X (above a transition redshift zt) and second Y (below zt). Fitting the model to the data, we find that the late component Y behaves as quintessence, like DESI. However, to cure the H0 and growth tensions, X must behave as 'phantom matter' (PM), which in contrast to phantom DE provides positive pressure at the expense of negative energy density. The PM behavior actually appears in stringy versions of the running vacuum model (RVM). Using the SNIa (considering separately Pantheon+ and DESY5), cosmic chronometers, transversal BAO, LSS data, and the full CMB likelihood from Planck 2018, we find that both tensions can be completely cut down. We also compare the wXCDM with our own results using the standard wCDM and w0wgCDM parameterizations of the DE. In all cases, model wXCDM performs much better. Finally, we have repeated our analysis with BAO 3D data (replacing BAO 2D), and we still find that the main dynamical DE models (including composite ones) provide a much better fit quality compared to Lambda CDM. The growth tension is alleviated again, but in contrast, the H0-tension remains significant, which is most likely reminiscent of the internal conflict in the BAO sector.
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页数:13
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共 123 条
[1]   The Dark Energy Survey: Cosmology Results with ∼1500 New High-redshift Type Ia Supernovae Using the Full 5 yr Data Set [J].
Abbott, T. M. C. ;
Acevedo, M. ;
Aguena, M. ;
Alarcon, A. ;
Allam, S. ;
Alves, O. ;
Amon, A. ;
Andrade-Oliveira, F. ;
Annis, J. ;
Armstrong, P. ;
Asorey, J. ;
Avila, S. ;
Bacon, D. ;
Bassett, B. A. ;
Bechtol, K. ;
Bernardinelli, P. H. ;
Bernstein, G. M. ;
Bertin, E. ;
Blazek, J. ;
Bocquet, S. ;
Brooks, D. ;
Brout, D. ;
Buckley-Geer, E. ;
Burke, D. L. ;
Camacho, H. ;
Camilleri, R. ;
Campos, A. ;
Rosell, A. Carnero ;
Carollo, D. ;
Carr, A. ;
Carretero, J. ;
Castander, F. J. ;
Cawthon, R. ;
Chang, C. ;
Chen, R. ;
Choi, A. ;
Conselice, C. ;
Costanzi, M. ;
da Costa, L. N. ;
Crocce, M. ;
Davis, T. M. ;
DePoy, D. L. ;
Desai, S. ;
Diehl, H. T. ;
Dixon, M. ;
Dodelson, S. ;
Doel, P. ;
Doux, C. ;
Drlica-Wagner, A. ;
Elvin-Poole, J. .
ASTROPHYSICAL JOURNAL LETTERS, 2024, 973 (01)
[2]   Cosmology intertwined: A review of the particle physics, astrophysics, and cosmology associated with the cosmological tensions and anomalies [J].
Abdalla, Elcio ;
Abellan, Guillermo Franco ;
Aboubrahim, Amin ;
Agnello, Adriano ;
Akarsu, Ozgur ;
Akrami, Yashar ;
Alestas, George ;
Aloni, Daniel ;
Amendola, Luca ;
Anchordoqui, Luis A. ;
Anderson, Richard I. ;
Arendse, Nikki ;
Asgari, Marika ;
Ballardini, Mario ;
Bargerx, Vernon ;
Basilakos, Spyros ;
Batista, Ronaldo C. ;
Battistelli, Elia S. ;
Battye, Richard ;
Benetti, Micol ;
Benisty, David ;
Berlin, Asher ;
de Bernardis, Paolo ;
Berti, Emanuele ;
Bidenko, Bohdan ;
Birrer, Simon ;
Blakeslee, John P. ;
Boddy, Kimberly K. ;
Bom, Clecio R. ;
Bonilla, Alexander ;
Borghi, Nicola ;
Bouchet, Francois R. ;
Braglia, Matteo ;
Buchert, Thomas ;
Buckley-Geer, Elizabeth ;
Calabrese, Erminia ;
Caldwell, Robert R. ;
Camarena, David ;
Capozziello, Salvatore ;
Casertano, Stefano ;
Chen, Angela ;
Chen, Geoff C-F ;
Chen, Hsin-Yu ;
Chluba, Jens ;
Chudaykin, Anton ;
Cicoli, Michele ;
Copi, Craig J. ;
Courbin, Fred ;
Cyr-Racine, Francis-Yan ;
Czerny, Bozena .
JOURNAL OF HIGH ENERGY ASTROPHYSICS, 2022, 34 :49-211
[3]  
Adame AG, 2025, J COSMOL ASTROPART P, DOI [10.1088/1475-7516/2025/02/021, 10.1088/1475-7516/2025/02/021]
[4]  
Adame A.G., 2024, arXiv
[5]   Dark energy in light of the early JWST observations: case for a negative cosmological constant? [J].
Adil, Shahnawaz A. ;
Mukhopadhyay, Upala ;
Sen, Anjan A. ;
Vagnozzi, Sunny .
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2023, (10)
[6]   Planck 2018 results: VI. Cosmological parameters [J].
Aghanim, N. ;
Akrami, Y. ;
Ashdown, M. ;
Aumont, J. ;
Baccigalupi, C. ;
Ballardini, M. ;
Banday, A. J. ;
Barreiro, R. B. ;
Bartolo, N. ;
Basak, S. ;
Battye, R. ;
Benabed, K. ;
Bernard, J. -P. ;
Bersanelli, M. ;
Bielewicz, P. ;
Bock, J. J. ;
Bond, J. R. ;
Borrill, J. ;
Bouchet, F. R. ;
Boulanger, F. ;
Bucher, M. ;
Burigana, C. ;
Butler, R. C. ;
Calabrese, E. ;
Cardoso, J. -F. ;
Carron, J. ;
Challinor, A. ;
Chiang, H. C. ;
Chluba, J. ;
Colombo, L. P. L. ;
Combet, C. ;
Contreras, D. ;
Crill, B. P. ;
Cuttaia, F. ;
de Bernardis, P. ;
de Zotti, G. ;
Delabrouille, J. ;
Delouis, J. -M. ;
Di Valentino, E. ;
Diego, J. M. ;
Dore, O. ;
Douspis, M. ;
Ducout, A. ;
Dupac, X. ;
Dusini, S. ;
Efstathiou, G. ;
Elsner, F. ;
Ensslin, T. A. ;
Eriksen, H. K. ;
Fantaye, Y. .
ASTRONOMY & ASTROPHYSICS, 2020, 641
[7]   NEW LOOK AT STATISTICAL-MODEL IDENTIFICATION [J].
AKAIKE, H .
IEEE TRANSACTIONS ON AUTOMATIC CONTROL, 1974, AC19 (06) :716-723
[8]  
Akarsu Ö, 2023, Arxiv, DOI arXiv:2307.10899
[9]   Relaxing cosmological tensions with a sign switching cosmological constant [J].
Akarsu, Ozgur ;
Kumar, Suresh ;
Ozulker, Emre ;
Alberto Vazquez, J. .
PHYSICAL REVIEW D, 2021, 104 (12)
[10]  
Alcaniz JS, 2017, FUND THEOR PHYS, V187, P11, DOI 10.1007/978-3-319-51700-1_2