Work

Euclid preparation. The shape of halo profiles in $Λ$CDM and non-standard cosmologies

Year: 2026
Type: preprint
Abstract: We study the shape of three-dimensional and projected dark-matter halo profiles extracted from cosmological $N$-body simulations in $Λ$CDM and non-standard cosmologies, using the \texttt{DUSTGRAIN-PF} and \texttt{DEMNUni} suites. The models considered include massive neutrinos, $f(\mathcal{R})$ gravity, and dynamical dark energy. By comparing density, mass, velocity-dispersion, and excess-surface-density profiles up to $5\,r_{500{\rm c}}$, we quantify the differential imprint of non-standard physics on halo structure in view of \textit{Euclid} cluster WL studies. Our main analysis is performed at $z=1.1$, a high-redshift regime where the weak-lensing signal-to-noise starts to degrade, providing a conservative stress test for detectability; for \texttt{DUSTGRAIN-PF} we additionally analyse $z=0.5$ and $z=0.3$ snapshots. In low-mass haloes ($M_{\rm 200c}<7\times10^{13}\,M_\odot$), $f(\mathcal{R})$ gravity produces deviations of order $10\,\%$ in projected and three-dimensional profiles, especially in the outskirts where screening is less efficient. Massive neutrinos partially reduce this signal, reflecting the competition between free streaming and fifth-force-enhanced growth. Dynamical dark energy and massive-neutrino cosmologies generally induce smaller, few-percent deviations, with the largest effects again found in low-mass haloes and at large radii. Under simplified assumptions for \Euclid WL, detecting such profile differences at $z=1.1$ requires stacks of $\sim10^5$ haloes, while a few thousands haloes may be sufficient at $z\lesssim0.5$. This further calls for the need of integrating such precise modelling of non-standard effects -- along with other observational effects -- in any likelihood involving \textit{Euclid} WL masses to avoid non-negligible systematic biases. Concentration--mass relations show weaker cosmology dependence, typically at the $\sim5\,\%$ level. [...]
Authors: Euclid Collaboration, Pizzuti, L., Ferron, G. Y., Ragagnin, A., Brun, A. M. C. Le, Corasaniti, P. -S., Gayoux, T., Rácz, G., Altamura, E., Sakr, Z., Carbone, C., Baldi, M., Giocoli, C., Castro, T., Pace, F., Taylor, J. E., Borgani, S., Luongo, O., Mpetha, C. T., Angulo, R. E., Altieri, B., Andreon, S., Auricchio, N., Baccigalupi, C., Bardelli, S., Battaglia, P., Biviano, A., Branchini, E., Brescia, M., Camera, S., Capobianco, V., Cardone, V. F., Carretero, J., Castellano, M., Castignani, G., Cavuoti, S., Chambers, K. C., Cimatti, A., Colodro-Conde, C., Congedo, G., Conversi, L., Copin, Y., Courbin, F., Courtois, H. M., Cropper, M., Degaudenzi, H., De Lucia, G., Dole, H., Dubath, F., Dupac, X., Dusini, S., Escoffier, S., Farina, M., Faustini, F., Ferriol, S., Finelli, F., Fosalba, P., Fotopoulou, S., Frailis, M., Franceschi, E., Fumana, M., Gabarra, L., Galeotta, S., George, K., Gillis, B., Gracia-Carpio, J., Grazian, A., Grupp, F., Haugan, S. V. H., Hemmati, S., Holmes, W., Hormuth, F., Hornstrup, A., Jahnke, K., Jhabvala, M., Joachimi, B., Kermiche, S., Kiessling, A., Kubik, B., Kuijken, K., Kunz, M., Kurki-Suonio, H., Ligori, S., Lilje, P. B., Lindholm, V., Lloro, I., Magliocchetti, M., Mainetti, G., Mansutti, O., Marggraf, O., Martinelli, M., Martinet, N., Marulli, F., Massey, R. J., Mauri, N., Maurogordato, S., Medinaceli, E., Mei, S., Meneghetti, M., Merlin, E., Meylan, G., Monaco, P., Mora, A., Moresco, M., Moretti, C., Moscardini, L., Munari, E., Neissner, C., Nightingale, J. W., Padilla, C., Paltani, S., Pasian, F., Pettorino, V., Pezzotta, A., Pires, S., Polenta, G., Poncet, M., Popa, L. A., Raison, F., Renzi, A., Rhodes, J., Riccio, G., Risso, I., Romelli, E., Roncarelli, M., Saglia, R., Sapone, D., Sartoris, B., Schneider, P., Schrabback, T., Secroun, A., Sefusatti, E., Sihvola, E., Simon, P., Sirignano, C., Sirri, G., Stanco, L., Starck, J. -L., Tallada-Crespí, P., Taylor, A. N., Tereno, I., Tessore, N., Toft, S., Toledo-Moreo, R., Torradeflot, F., Tutusaus, I., Valentijn, E. A., Valiviita, J., Vassallo, T., Wang, Y., Weller, J., Zacchei, A., Zamorani, G., Zerbi, F. M., Zucca, E., Ballardini, M., Bergamini, P., Boucaud, A., Bozzo, E., Burigana, C., Cabanac, R., Calabrese, M., Cappi, A., Caro, F., Vigo, J. A. Escartin, García-Bellido, J., Gasparetto, T., Macias-Perez, J., Maoli, R., Metcalf, R. B., Pöntinen, M., Sarpa, E., Scottez, V., Sereno, M., Tenti, M., Tucci, M., Viel, M., Wiesmann, M., Barroso, J. A. Acevedo, Akrami, Y., Andika, I. T., Anselmi, S., Archidiacono, M., Aricò, G., Atrio-Barandela, F., Baes, M., Bazzanini, L., Bertacca, D., Bethermin, M., Beutler, F., Blanchard, A., Blot, L., Böhringer, H., Brown, M. L., Bruton, S., Calabro, A., Quevedo, B. Camacho, Carvalho, C. S., Cogato, F., Collett, T. E., Conseil, S., Cooray, A. R., Corcho-Caballero, P., Costanzi, M., Csizi, B., Cucciati, O., de Boer, T., De Paolis, F., Desprez, G., Díaz-Sánchez, A., Di Domizio, S., Diego, J. M., Duret, V., Fang, Y., Farina, A., Finoguenov, A., Fontanot, F., Franco, A., Fu, Y., Ganga, K., Gavazzi, R., Gaztanaga, E., Ghaffari, Z., Giacomini, F., Gianotti, F., Gonzalez, E. J., Gozaliasl, G., Gruppuso, A., Guidi, M., Gutierrez, C. M., Hall, A., Hatch, N. A., Hernández-Monteagudo, C., Hildebrandt, H., Hjorth, J., Kajava, J. J. E., Kang, Y., Kansal, V., Karagiannis, D., Kim, J., Kirkpatrick, C. C., Kovács, A., Kova{č}i{ć}, I., Koyama, K., Kruk, S., Lam, M. C., Lattanzi, M., Legrand, L., Lembo, M., Leroy, G., Lesci, G. F., Lesgourgues, J., Linke, L., Manjón-García, A., Mannucci, F., Marleau, F. R., Martins, C. J. A. P., Migliaccio, M., Miluzio, M., Morgante, G., Nadathur, S., Naidoo, K., Navarro-Alsina, A., Nesseris, S., Oppizzi, F., Paoletti, D., Passalacqua, F., Paterson, K., Patrizii, L., Pattison, C., Paviot, R., Pisani, A., Potter, D., Pratt, G. W., Quai, S., Radovich, M., Rodighiero, G., Roster, W., Sacquegna, S., Sahlén, M., Sanders, D. B., Schneider, A., Sciotti, D., Sellentin, E., Serjeant, S., Shankar, F., Smith, L. C., Sorce, J. G., Szapudi, I., Tanidis, K., Tao, C., Tarsitano, F., Testera, G., Teyssier, R., Tosi, S., Troja, A., Uhlemann, C., Valieri, C., Venhola, A., Vergani, D., Verza, G., Vielzeuf, P., Vinciguerra, S., von Wietersheim-Kramsta, M., Wang, L., Wright, A. H., Yeung, H. W.
Institutions: University of Milano-Bicocca, Trieste Astronomical Observatory, Centre National de la Recherche Scientifique, Université Paris Sciences et Lettres, Observatoire de Paris, Sorbonne Université, Laboratoire d'Étude de l'Univers et des Phénomènes Extrêmes, Institut d'Astrophysique de Paris, Université Paris Cité, University of Helsinki, University of Cambridge, University of Manchester, Consejo Superior de Investigaciones Científicas, Saint Joseph University, Instituto de Física Teórica, Institut de Recherche en Astrophysique et Planétologie, National Institute for Astrophysics, Istituto Nazionale di Fisica Nucleare, Sezione di Bologna, Osservatorio di Astrofisica e Scienza dello Spazio, University of Bologna, Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, Institute for Fundamental Physics of the Universe, Fondazione ICSC Centro Nazionale di Ricerca in High Performance Computing, Big Data e Quantum Computing, University of Lisbon, Institute of Astrophysics and Space Sciences, Istituto Nazionale di Fisica Nucleare, Sezione di Torino, Osservatorio Astrofisico di Torino, University of Turin, University of Waterloo, University of Trieste, Brera Astronomical Observatory, Goddard Space Flight Center, Ikerbasque, Donostia International Physics Center, European Space Astronomy Centre, Scuola Internazionale Superiore di Studi Avanzati, Istituto Nazionale di Fisica Nucleare, Sezione di Genova, University of Genoa, Astronomical Observatory of Capodimonte, University of Naples Federico II, Astronomical Observatory of Rome, Istituto Nazionale di Fisica Nucleare, Sezione di Roma I, Port d'Informació Científica, Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli, University of Hawaiʻi at Mānoa, University of Hawaii System, Instituto de Astrofísica de Canarias, Royal Observatory, University of Edinburgh, European Space Agency, European Space Research Institute, Lyon 1 Université, Institut National de Physique Nucléaire et de Physique des Particules, Institut de Physique des 2 Infinis de Lyon, Institució Catalana de Recerca i Estudis Avançats, Institute of Space Sciences, Institut de Ciències del Cosmos, University College London, University of Geneva, Université Paris-Saclay, Institut d'Astrophysique Spatiale, Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Aix-Marseille Université, Centre de physique des particules de Marseille, Institute for Space Astrophysics and Planetology, Institut d'Estudis Espacials de Catalunya, University of Bristol, University of Oxford, Ludwig-Maximilians-Universität München, Max Planck Institute for Extraterrestrial Physics, Osservatorio Astronomico di Padova, University of Oslo, California Institute of Technology, Infrared Processing and Analysis Center, Jet Propulsion Laboratory, Technical University of Denmark, Max Planck Institute for Astronomy, Leiden University, Leiden Observatory, Helsinki Institute of Physics, SKA Observatory, Centre de Calcul de l’Institut National de Physique Nucléaire et de Physique des Particules, University of Bonn, Durham University, Université Côte d'Azur, Lagrange Laboratory, Observatoire de la Côte d’Azur, Centre Pierre Binétruy, University of California, Berkeley, École Polytechnique Fédérale de Lausanne, Institute for High Energy Physics, Newcastle University, European Space Research and Technology Centre, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Astrophysique, Instrumentation et Modélisation, Agenzia Spaziale Italiana, Centre National d'Études Spatiales, Institute of Space Science - INFLPR Subsidiary, University of Padua, University of Chile, Universität Innsbruck, University of Copenhagen, European Union, Universidad Politécnica de Cartagena, University of Groningen, University of Ferrara, Istituto Nazionale di Fisica Nucleare, Sezione di Ferrara, Istituto di Radioastronomia di Bologna, Osservatorio Astronomico della Regione Autonoma Valle d'Aosta, Regione Autonoma Valle d'Aosta, Institut polytechnique de Grenoble, Sapienza University of Rome, Université Catholique de Lille, JUNIA, Case Western Reserve University, Laboratoire Univers et Théories, University of Milan, Istituto Nazionale di Fisica Nucleare, Sezione di Milano, Universidad de Salamanca, Ghent University, Observatoire astronomique de Strasbourg, Université de Strasbourg, Kavli Institute for the Physics and Mathematics of the Universe, Max Planck Institute for Physics, University of Portsmouth, University of California, Irvine, University of Salento, Istituto Nazionale di Fisica Nucleare, Sezione di Lecce, Instituto de Física de Cantabria, Instituto de Astronomía Teórica y Experimental, Aalto University, Universidad de La Laguna, University of Nottingham, Ruhr University Bochum, University of Turku, ARC Centre of Excellence for Dark Matter Particle Physics, Swinburne University of Technology, University of the Western Cape, Konkoly Observatory, HUN-REN Research Centre for Astronomy and Earth Sciences, Centro Brasileiro de Pesquisas Físicas, Arcetri Astrophysical Observatory, Universidade do Porto, Centro de Astrofísica da Universidade do Porto, University of Rome Tor Vergata, University of Zurich, Collurania Teramo Observatory, Uppsala University, The Open University, University of Southampton, Université de Lille, Centre de Recherche en Informatique, Signal et Automatique de Lille, Centrale Lille Institut, University of Nova Gorica, ETH Zurich, Institute for Particle Physics and Astrophysics, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Princeton University, Bielefeld University, University of Oulu, The Abdus Salam International Centre for Theoretical Physics (ICTP), Flatiron Institute, Space Research Organisation Netherlands
Language: English
Open Access status: green
OpenAlex ID: W7208765418
Cites: 4
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Related to: 10