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In the first part, I will focus on probing the small scales via CMB distortions, scalar induced secondary GWs and line intensity mapping. In the second part, I will discuss probing light bosons (even if they are subdominant part of dark matter) in a range of masses from e-26 to e-23 eV via pulsar timing arrays, e-21 to e-17eV via SMBH superradiance and e-12 to e21 eV via light black hole superradiance.