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We study a model of Symmetric Teleparallel gravity that is able to accountfor the current accelerated expansion of the universe without the need for darkenergy component. We investigate this model by making use of dynamical systemanalysis techniques to identify the regions of the parameter space with viablecosmologies and constrain it using type Ia supernova (SnIa), cosmic microwavebackground (CMB) data and make forecasts using standard siren (SS) events. Weconclude that this model is disfavored with respect to $\Lambda$CDM andforthcoming standard siren events can be decisive in testing the viability ofthe model.

Testing $\Lambda$-Free f(Q) Cosmology