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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Professor Pedro Ferreira

Professor of Astrophysics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Astrophysics

Research groups

  • Beecroft Institute for Particle Astrophysics and Cosmology
pedro.ferreira@physics.ox.ac.uk
Telephone: 01865 (2)73366
Denys Wilkinson Building, room 757
  • About
  • Publications

Cosmological constraints on Galileon dark energy with broken shift symmetry

Physical Review D American Physical Society (APS) 113:2 (2026) 23551

Authors:

William J Wolf, Pedro G Ferreira, Carlos García-García

Abstract:

Current cosmological data seem to show that dark energy is evolving in time and that it possibly crossed the phantom divide in the past. So far the only theories that lead to such a behavior involve a nontrivial coupling between dark energy, in the form of a scalar field, and the gravitational or matter sector. We show that there is another possibility involving both a nontrivial kinetic sector in a cubic Galileon theory and a scalar field potential that breaks the Galileon shift symmetry, which can lead to a similar phenomenology on large scales. We perform a full Bayesian analysis using the latest cosmological data, including DESI DR2 baryonic acoustic oscillation measurements, type Ia SNe measurements from DESY5, Union3, and Pantheon+, and cosmic microwave background data from Planck and ACT. We find that it is statistically strongly favored over a universe dominated by a cosmological constant (with a Bayes factor of <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"> <mi>log</mi> <mi>B</mi> <mo>≃</mo> <mn>6.5</mn> </math> ). Yet, as with other nonminimally coupled theories, it has severe ancillary gravitational effects. These can be mitigated to some extent, but as with other viable theories, the penalty is ever more elaborate scalar field models of dark energy.

Euclid Quick Data Release (Q1). LEMON -- Lens Modelling with Neural networks. Automated and fast modelling of Euclid gravitational lenses with a singular isothermal ellipsoid mass profile

(2026)

Authors:

Euclid Collaboration, V Busillo, C Tortora, RB Metcalf, JW Nightingale, M Meneghetti, F Gentile, R Gavazzi, F Zhong, R Li, B Clément, G Covone, NR Napolitano, F Courbin, M Walmsley, E Jullo, J Pearson, D Scott, AMC Le Brun, L Leuzzi, N Aghanim, B Altieri, A Amara, S Andreon, H Aussel, C Baccigalupi, M Baldi, S Bardelli, P Battaglia, A Biviano, E Branchini, M Brescia, J Brinchmann, S Camera, G Cañas-Herrera, V Capobianco, C Carbone, VF Cardone, J Carretero, S Casas, M Castellano, G Castignani, S Cavuoti, KC Chambers, A Cimatti, C Colodro-Conde, G Congedo, CJ Conselice, L Conversi, Y Copin, HM Courtois, M Cropper, A Da Silva, H Degaudenzi, S de la Torre, G De Lucia, AM Di Giorgio, J Dinis, H Dole, F Dubath, X Dupac, S Dusini, S Escoffier, M Farina, R Farinelli, F Faustini, S Ferriol, F Finelli, S Fotopoulou, M Frailis, E Franceschi, S Galeotta, K George, W Gillard, B Gillis, C Giocoli, J Gracia-Carpio, BR Granett, A Grazian, F Grupp, SVH Haugan, W Holmes, I Hook, F Hormuth, A Hornstrup, P Hudelot, K Jahnke, M Jhabvala, B Joachimi, E Keihänen, S Kermiche, A Kiessling, B Kubik, M Kümmel, M Kunz, H Kurki-Suonio, Q Le Boulc'h, S Ligori, PB Lilje, V Lindholm, I Lloro, G Mainetti, D Maino, E Maiorano, O Mansutti, O Marggraf, K Markovic, M Martinelli, N Martinet, F Marulli, R Massey, S Maurogordato, E Medinaceli, S Mei, Y Mellier, E Merlin, G Meylan, A Mora, M Moresco, L Moscardini, R Nakajima, C Neissner, S-M Niemi, C Padilla, S Paltani, F Pasian, K Pedersen, V Pettorino, S Pires, G Polenta, M Poncet, LA Popa, L Pozzetti, F Raison, R Rebolo, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, R Saglia, Z Sakr, AG Sánchez, D Sapone, B Sartoris, JA Schewtschenko, M Schirmer, P Schneider, T Schrabback, A Secroun, E Sefusatti, G Seidel, M Seiffert, S Serrano, P Simon, C Sirignano, G Sirri, G Smadja, L Stanco, J Steinwagner, P Tallada-Crespí, AN Taylor, I Tereno, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, L Valenziano, J Valiviita, T Vassallo, A Veropalumbo, Y Wang, J Weller, G Zamorani, E Zucca, V Allevato, M Ballardini, M Bolzonella, E Bozzo, C Burigana, R Cabanac, M Calabrese, D Di Ferdinando, JA Escartin Vigo, L Gabarra, M Huertas-Company, S Matthew, N Mauri, AA Nucita, A Pezzotta, M Pöntinen, C Porciani, V Scottez, M Tenti, M Viel, M Wiesmann, Y Akrami, S Alvi, IT Andika, S Anselmi, M Archidiacono, F Atrio-Barandela, D Bertacca, M Bethermin, A Blanchard, L Blot, S Borgani, ML Brown, S Bruton, A Calabro, B Camacho Quevedo, A Cappi, F Caro, CS Carvalho, T Castro, F Cogato, S Conseil, S Contarini, AR Cooray, O Cucciati, F De Paolis, G Desprez, A Díaz-Sánchez, S Di Domizio, JM Diego, P Dimauro, A Enia, Y Fang, AG Ferrari, PG Ferreira, A Finoguenov, A Franco, K Ganga, J García-Bellido, T Gasparetto, V Gautard, E Gaztanaga, F Giacomini, F Gianotti, G Gozaliasl, M Guidi, CM Gutierrez, A Hall, WG Hartley, S Hemmati, C Hernández-Monteagudo, H Hildebrandt, J Hjorth, JJE Kajava, Y Kang, V Kansal, D Karagiannis, K Kiiveri, CC Kirkpatrick, S Kruk, M Lattanzi, J Le Graet, L Legrand, M Lembo, F Lepori, G Leroy, J Lesgourgues, TI Liaudat, SJ Liu, A Loureiro, J Macias-Perez, G Maggio, M Magliocchetti, F Mannucci, R Maoli, J Martín-Fleitas, CJAP Martins, L Maurin, M Miluzio, P Monaco, C Moretti, G Morgante, S Nadathur, K Naidoo, P Natoli, A Navarro-Alsina, S Nesseris, F Passalacqua, K Paterson, L Patrizii, A Pisani, D Potter, S Quai, M Radovich, I Risso, P-F Rocci, S Sacquegna, M Sahlén, E Sarpa, A Schneider, M Schultheis, D Sciotti, E Sellentin, M Sereno, LC Smith, J Stadel, K Tanidis, C Tao, G Testera, R Teyssier, S Tosi, A Troja, M Tucci, C Valieri, A Venhola, D Vergani, G Vernardos, G Verza, P Vielzeuf, NA Walton

Cosmological constraints on Galileon dark energy with broken shift symmetry

(2026)

Authors:

William J Wolf, Pedro G Ferreira, Carlos García-García

Symbolically regressing dark matter halo profiles using weak lensing

(2026)

Authors:

Alicia Martín, Tariq Yasin, Deaglan J Bartlett, Harry Desmond, Pedro G Ferreira

Euclid preparation. LXXXV. Toward a DR1 application of higher-order weak lensing statistics

(2026)

Authors:

Euclid Collaboration, S Vinciguerra, F Bouchè, N Martinet, L Castiblanco, C Uhlemann, S Pires, J Harnois-Déraps, C Giocoli, M Baldi, VF Cardone, A Vadalà, N Dagoneau, L Linke, E Sellentin, PL Taylor, JC Broxterman, S Heydenreich, V Tinnaneri Sreekanth, N Porqueres, L Porth, M Gatti, D Grandón, A Barthelemy, F Bernardeau, A Tersenov, H Hoekstra, J-L Starck, S Cheng, PA Burger, I Tereno, R Scaramella, B Altieri, S Andreon, N Auricchio, C Baccigalupi, S Bardelli, A Biviano, E Branchini, M Brescia, S Camera, G Cañas-Herrera, V Capobianco, C Carbone, J Carretero, M Castellano, G Castignani, S Cavuoti, KC Chambers, A Cimatti, C Colodro-Conde, G Congedo, L Conversi, Y Copin, F Courbin, HM Courtois, M Cropper, A Da Silva, H Degaudenzi, S de la Torre, G De Lucia, H Dole, F Dubath, X Dupac, S Dusini, S Escoffier, M Farina, R Farinelli, S Farrens, F Faustini, S Ferriol, F Finelli, M Frailis, E Franceschi, M Fumana, S Galeotta, K George, B Gillis, J Gracia-Carpio, A Grazian, F Grupp, SVH Haugan, W Holmes, F Hormuth, A Hornstrup, P Hudelot, K Jahnke, M Jhabvala, B Joachimi, E Keihänen, S Kermiche, A Kiessling, M Kilbinger, B Kubik, M Kunz, H Kurki-Suonio, AMC Le Brun, S Ligori, PB Lilje, V Lindholm, I Lloro, G Mainetti, D Maino, O Mansutti, O Marggraf, M Martinelli, F Marulli, RJ Massey, E Medinaceli, S Mei, M Melchior, Y Mellier, M Meneghetti, G Meylan, A Mora, M Moresco, L Moscardini, C Neissner, S-M Niemi, C Padilla, S Paltani, F Pasian, K Pedersen, V Pettorino, G Polenta, M Poncet, LA Popa, F Raison, A Renzi, J Rhodes, G Riccio, E Romelli, M Roncarelli, R Saglia, Z Sakr, AG Sánchez, D Sapone, B Sartoris, P Schneider, T Schrabback, A Secroun, G Seidel, S Serrano, C Sirignano, G Sirri, A Spurio Mancini, L Stanco, J Steinwagner, P Tallada-Crespí, AN Taylor, N Tessore, S Toft, R Toledo-Moreo, F Torradeflot, I Tutusaus, J Valiviita, T Vassallo, Y Wang, J Weller, A Zacchei, G Zamorani, FM Zerbi, E Zucca, M Ballardini, M Bolzonella, A Boucaud, E Bozzo, C Burigana, R Cabanac, M Calabrese, A Cappi, JA Escartin Vigo, L Gabarra, WG Hartley, R Maoli, J Martín-Fleitas, S Matthew, N Mauri, RB Metcalf, A Pezzotta, M Pöntinen, I Risso, V Scottez, M Sereno, M Tenti, M Viel, M Wiesmann, Y Akrami, IT Andika, RE Angulo, S Anselmi, M Archidiacono, F Atrio-Barandela, E Aubourg, D Bertacca, M Bethermin, A Blanchard, L Blot, M Bonici, S Borgani, ML Brown, S Bruton, A Calabro, B Camacho Quevedo, F Caro, CS Carvalho, T Castro, F Cogato, S Conseil, AR Cooray, G Desprez, A Díaz-Sánchez, JJ Diaz, S Di Domizio, JM Diego, MY Elkhashab, Y Fang, PG Ferreira, A Finoguenov, A Franco, K Ganga, J García-Bellido, T Gasparetto, V Gautard, R Gavazzi, E Gaztanaga, F Giacomini, F Gianotti, G Gozaliasl, M Guidi, CM Gutierrez, A Hall, S Hemmati, H Hildebrandt, J Hjorth, JJE Kajava, Y Kang, D Karagiannis, K Kiiveri, J Kim, CC Kirkpatrick, S Kruk, L Legrand, M Lembo, F Lepori, G Leroy, GF Lesci, J Lesgourgues, TI Liaudat, J Macias-Perez, M Magliocchetti, F Mannucci, CJAP Martins, L Maurin, M Miluzio, P Monaco, C Moretti, G Morgante, S Nadathur, K Naidoo, A Navarro-Alsina, S Nesseris, D Paoletti, F Passalacqua, K Paterson, L Patrizii, A Pisani, D Potter, S Quai, M Radovich, S Sacquegna, M Sahlén, DB Sanders, E Sarpa, A Schneider, D Sciotti, LC Smith, K Tanidis, C Tao, G Testera, R Teyssier, S Tosi, A Troja, M Tucci, D Vergani, G Verza, NA Walton

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