We present constraints on extensions of the minimal cosmological models dominated by dark matter and dark energy, CDM and CDM, by using a combined analysis of galaxy clustering and weak gravitational lensing from the first-year data of the Dark Energy Survey (DES Y1) in combination with external data. We consider four extensions of the minimal dark energy-dominated scenarios: 1) nonzero curvature , 2) number of relativistic species different from the standard value of 3.046, 3) time-varying equation-of-state of dark energy described by the parameters and (alternatively quoted by the values at the pivot redshift, , and ), and 4) modified gravity described by the parameters and that modify the metric potentials. We also consider external information from Planck CMB measurements; BAO measurements from SDSS, 6dF, and BOSS; RSD measurements from BOSS; and SNIa information from the Pantheon compilation. Constraints on curvature and the number of relativistic species are dominated by the external data; when these are combined with DES Y1, we find at the 68% confidence level, and $N_{\rm eff}<3.28, (3.55)$ at 68% (95%) confidence. For the time-varying equation-of-state, we find the pivot value $(w_p, w_a)=(-0.91^{+0.19}{-0.23}, -0.57^{+0.93}{-1.11})z_p=0.27(w_p, w_a)=(-1.01^{+0.04}{-0.04}, -0.28^{+0.37}{-0.48})z_p=0.20$ from DES Y1 combined with external data; in either case we find no evidence for the temporal variation of the equation of state. For modified gravity, we find the present-day value of the relevant parameters to be $\Sigma_0= 0.43^{+0.28}{-0.29}(\Sigma_0, \mu_0)=(0.06^{+0.08}{-0.07}, -0.11^{+0.42}_{-0.46})$ from DES Y1 combined with external data, consistent with predictions from GR.

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