Jordi Miralda Escudé

Jordi Miralda Escudé

Universitat de Barcelona

Experimental Sciences & Mathematics

I learned physics at the Autonomous University of Barcelona, and astronomy on my own and through some amateur associations in Catalonia. I did my PhD in astrophysics at Princeton University, graduating in 1991 with a thesis on gravitational lensing by clusters of galaxies and large-scale structure. I was a postdoc at the Institute of Astronomy in Cambridge, and a Long-Term Member at the Institute for Advanced Study. I joined the University of Pennsylvania as a professor of astrophysics in 1996, and then moved to The Ohio State University in 2000. I have been back to Catalonia with an ICREA position since 2005, and I am at present doing research on astrophysics, cosmology and axion detection experiments at the Institut de Ciències del Cosmos in the University of Barcelona.

Research interests

I enjoy searching for physical explanations of what we observe in the Universe. My interests range over the formation of galaxies and their large-scale distribution, gravitational lensing and dark matter in the Universe, the intergalactic medium, and black holes in galactic nuclei. For many years I have focused on the large-scale distribution of intergalactic gas probed by absorption spectra in quasar spectroscopic surveys, which reveals crucial clues on both the initial conditions of the Universe and the formation of galaxies. At present I am looking at various techniques to inquire on the nature of dark matter, among them the observation of extremely magnified high-redshift stars close to the critical curves of clusters of galaxies acting as gravitational lenses, the study of tidal streams of stars left by stellar systems orbiting the Milky Way galaxy, and several techniques to detect axion waves as a highly promising dark matter candidate.

Selected publications

- Ahyoune, S et al. 2025, 'RADES axion search results with a high-temperature superconducting cavity in an 11.7 T magnet', Journal of high energy physics, vol. 4(2025), pp 113.
- Müller CV & Miralda-Escudé J 2025, 'Limits on Dark Matter Compact Objects Implied by Supermagnified Stars in Lensing Clusters', Monthly Notices of the Royal Astronomical Society, vol. 536, no. 2, pp 1579-1585.
- IAXO Collaboration, Ahyoune S et al. 2025, 'An accurate solar axions ray-tracing response of BabyIAXO', Journal of high energy physics, vol 2(2025), pp 159.
- Ubach H, Gieles M & Miralda-Escudé J, 2025, 'Constraining the Environment of Compact Binary Mergers with Self-lensing Signatures', Physical Review D, vol. 112, no. 8, pp 083026.

Selected research activities

As a member of the RADES Collaboration to detect axions as dark matter in haloscopes (or resonance cavities in a strong magnetic field), I have participated in analysing data obtained at the CERN SM18 magnet, contributing to the methodology for obtaining an upper limit to the axion signal at a frequency near 8.84 GHz, with postdocs S. Arguedas and S. Ahyoune.
I have also been active in RADES to develop single photon detection with a transmon qubit in these haloscopes, instead of the classical linear amplification method that is limited by the standard quantum limit.
In the IAXO Collaboration, and with technicians Saiyd Ahyoune and Eduardo Picatoste, we have continued testing the electronics for the Data Acquisition System of the BabyIAXO Micromegas detector, which will detect solar axions converting to X-rays in the BabyIAXO helioscope.
I have also started research on lensing effects in gravitational wave events with student Helena Ubach, in collaboration with Mark Gieles.