In f(R, G_{\mu\nu}T^{\mu\nu}) gravity, gravitational baryogenesis produces a baryon-to-entropy ratio compatible with observations, and chi-square fits to H(z) and \mu(z) data match \Lambda CDM performance.
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Cosmological Realization of Baryon Asymmetry in f(R, G_{\mu\nu}T^{\mu\nu}) Gravity
In f(R, G_{\mu\nu}T^{\mu\nu}) gravity, gravitational baryogenesis produces a baryon-to-entropy ratio compatible with observations, and chi-square fits to H(z) and \mu(z) data match \Lambda CDM performance.