2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/210907We investigate the noncommutative effect on the non-Gaussianities of primordial cosmological perturbation. In the lowest order of string length and slow-roll parameter, we find that in the models with small speed of sound the noncommutative modifications could be observable if assuming a relatively low string scale. In particular, the dominant modification of non-Gaussianity estimator f_{NL} could reach O(1) in DBI inflation and K-inflation. The corrections are sensitive to the speed of sound and the choice of string length scale. Moreover the shapes of the corrected non-Gaussianities are distinct from that of ordinary ones.26 pages, 3 figures Added references, changed contentAstrophysicsHigh Energy Physics - TheoryNon-commutative Geometry Modified Non-Gaussianities of Cosmological Perturbationtext