Primordial non-Gaussianity in supersolid inflation

Journal of High Energy Physics

Rocco Rollo¹  Marco Celoria²  Denis Comelli³  Luigi Pilo⁴ 

[1] Gran Sasso Science Institute (GSSI), Viale Francesco Crispi 7, I-67100, L’Aquila, Italy;Centro Nazionale INFN di Studi Avanzati GGI, Largo Enrico Fermi 2, I-50125, Firenze, Italy;ICTP, International Centre for Theoretical Physics, Strada Costiera 11, 34151, Trieste, Italy;INFN Sezione di Ferrara, via Saragat 1, 44122, Ferrara, Italy;Laboratori Nazionali del Gran Sasso (LNGS), via Giovanni Acitelli, 2, 67100, L’Aquila, Italy;Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi dell’Aquila, I-67010, L’Aquila, Italy;

关键词: Effective Field Theories;    Spontaneous Symmetry Breaking;    Cosmology of Theories beyond the SM;   

DOI  :  10.1007/JHEP06(2021)147

来源: Springer

【 摘 要 】

We study primordial non-gaussianity in supersolid inflation. The dynamics of supersolid is formulated in terms of an effective field theory based on four scalar fields with a shift symmetric action minimally coupled with gravity. In the scalar sector, there are two phonon-like excitations with a kinetic mixing stemming from the completely spontaneous breaking of diffeomorphism. In a squeezed configuration, fNL of scalar perturbations is angle dependent and not proportional to slow-roll parameters showing a blunt violation of the Maldacena consistency relation. Contrary to solid inflation, the violation persists even after an angular average and generically the amount of non-gaussianity is significant. During inflation, non-gaussianity in the TSS and TTS sector is enhanced in the same region of the parameters space where the secondary production of gravitational waves is sizeable enough to enter in the sensitivity region of LISA, while the scalar fNL is still within the current experimental limits.

【 授权许可】

CC BY