Journal of Physics: Conference Series OPEN ACCESS Related content - Condensate fraction of asymmetric three- Fermionic condensation in ultracold atoms, component Fermi gas Du Jia-Jia, Liang Jun-Jun and Liang Jiu- nuclear matter and neutron stars Qing - S-Wave Scattering Properties for Na—K Cold Collisions To cite this article: Luca Salasnich 2014 J. Phys.: Conf. Ser. 497 012026 Zhang Ji-Cai, Zhu Zun-Lue, Sun Jin-Feng et al. - Landau damping in a dipolar Bose–Fermi mixture in the Bose–Einstein condensation (BEC) limit View the article online for updates and enhancements. S M Moniri, H Yavari and E Darsheshdar This content was downloaded from IP address 170.106.40.139 on 26/09/2021 at 20:46 22nd International Laser Physics Worksop (LPHYS 13) IOP Publishing Journal of Physics: Conference Series 497 (2014) 012026 doi:10.1088/1742-6596/497/1/012026 Fermionic condensation in ultracold atoms, nuclear matter and neutron stars Luca Salasnich Dipartimento di Fisica e Astronomia “Galileo Galilei” and CNISM, Universit`a di Padova, Via Marzolo 8, 35131 Padova, Italy E-mail:
[email protected] Abstract. We investigate the Bose-Einstein condensation of fermionic pairs in three different superfluid systems: ultracold and dilute atomic gases, bulk neutron matter, and neutron stars. In the case of dilute gases made of fermionic atoms the average distance between atoms is much larger than the effective radius of the inter-atomic potential. Here the condensation of fermionic pairs is analyzed as a function of the s-wave scattering length, which can be tuned in experiments by using the technique of Feshbach resonances from a small and negative value (corresponding to the Bardeen-Cooper-Schrieffer (BCS) regime of Cooper Fermi pairs) to a small and positive value (corresponding to the regime of the Bose-Einstein condensate (BEC) of molecular dimers), crossing the unitarity regime where the scattering length diverges.