Group “Fundamental Interactions”
The cosmology team includes researchers with expertise in Cosmology, General Relativity, Quantum Field Theory, and Particle Physics. They collaborate and share national and international grants with several groups of theorists, cosmologists, astronomers, astrophysicists, and particle physicists.
Over the past fifteen years, an avalanche of high-quality data has transformed cosmology into a field rich in results. It has become an ideal arena for testing and potentially falsifying predictions arising from several areas of fundamental physics. This abundance of information has recently enabled the discovery of unexpected phenomena such as the acceleration of the expansion of the universe and the detection of long-sought physical signals that had previously escaped observation, such as gravitational waves.
The core of our activities is organized around three main research directions:
| AGAPITO | Alessandro | Ph.D. | Contact | |
| BEL | Julien | Research teacher | +33.4.91.26.95.05 | Contact |
| BERA | Sayantani | Post Ph.D. | Contact | |
| CINTIA | Giordano | Post Ph.D. | Contact | |
| DE RENZIS | Viola | Post Ph.D. | Contact | |
| HU | Shiqian | Post Ph.D. | Contact | |
| KALBOUNEH | Basheer | Post Ph.D. | +33.4.91.26.97.88 | Contact |
| MANCARELLA | Michele | Research teacher | Contact | |
| MARINONI | Christian | Research teacher Team leader « Cosmology » | +33.4.91.26.95.35 | Contact |
| PEDROTTI | Alessandro | Ph.D. | Contact | |
| PIAZZA | Federico | Research teacher | +33.4.91.26.95.00 | Contact |
| RAMOS | Samuel | Ph.D. | Contact | |
| SANTIAGO | Jessica | Post Ph.D. | Contact | |
| SARMA | Maharshi | Ph.D. | Contact | |
| TAXIL | Pierre | Research teacher emeritus | +33.4.91.26.95.52 | Contact |
| VAREILLES | Simeon | Ph.D. | Contact | |
| VIREY | Jean-Marc | Research teacher | +33.4.91.26.95.48 | Contact |
| ZIANE | Mehdi-Bara | Ph.D. | +33.4.91.26.97.79 | Contact |
Torsion, an alternative to dark matter?
General Relativity and Gravitation, 2011, 43 (11), pp.2965-2978. (10.1007/s10714-011-1222-6)
The bimodality of the 10k zCOSMOS-bright galaxies up to z ~ 1: a new statistical and portable classification based on the optical galaxy properties
Astronomy & Astrophysics - A&A, 2011, 535, pp.10. (10.1051/0004-6361/201016130)
The nonlinear biasing of the 10k zCOSMOS galaxies up to z~1
The Astrophysical Journal, 2011, 731 (2), pp.102. (10.1088/0004-637X/731/2/102)
The zCOSMOS-Bright survey: the clustering of early and late galaxy morphological types since z≃ 1
Monthly Notices of the Royal Astronomical Society, 2011, 412 (2), pp.825. (10.1111/j.1365-2966.2010.17939.x)
Comparison of the VIMOS-VLT Deep Survey with the Munich semi-analytical model
Astronomy & Astrophysics - A&A, 2011, 525, pp.125. (10.1051/0004-6361/201015540)
A geometric measure of dark energy with pairs of galaxies
Nature, 2010, 468 (7323), (10.1038/nature09577)
K+a galaxies in the zCOSMOS Survey: Physical properties of systems in their post-starburst phase
Astronomy & Astrophysics - A&A, 2010, 509, pp.A42. (10.1051/0004-6361/200912802)
The density field of the 10k zCOSMOS galaxies
The Astrophysical Journal, 2010, 708 (1), pp.505. (10.1088/0004-637X/708/1/505)
zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift
Astronomy & Astrophysics - A&A, 2010, 523, pp.A13. (10.1051/0004-6361/200913020)
Tracking the impact of environment on the Galaxy Stellar Mass Function up to z~1 in the 10k zCOSMOS sample
Astronomy & Astrophysics - A&A, 2010, 524, pp.A76. (10.1051/0004-6361/200912801)