Starting from the star formation rate (SFR) per unit area, , determined for damped Lyα systems (DLAs) using the C II* method, we obtain the SFR per unit comoving volume, (z), at z ≈ 3. Pure warm neutral medium (WNM) solutions are ruled out since they generate more bolometric background radiation than observed, but the two-phase solutions dominated by the cold neutral medium (CNM) are consistent with the backgrounds. We find that (z) for DLAs agrees with the (z) for the Lyman break galaxies (LBGs). Although the mass of produced stars indicated by the SFRs is consistent with the current densities of known stellar populations, the mass of metals produced by z = 2.5 is 30 times larger than detected in absorption in DLAs. Of the three possible solutions to this "missing metals" problem, the most likely appears to be that star formation occurs in compact bulge regions. We search for evidence of feedback and find no correlations between and N(H I), but possible correlations between and low-ion velocity width and and metal abundance. We show that (1) the correlation between cooling rate and dust-to-gas ratio is positive evidence for grain photoelectric heating, (2) the cosmic microwave background (CMB) does not significantly populate the C II excited fine-structure states, and (3) the ratio of C II* to resonance-line optical depths is a sensitive probe of the multiphase structure of the DLA gas. We address recent arguments that DLAs are comprised only of WNM gas and show them to be inconclusive. Despite the rough agreement between (z) for DLAs and LBGs, current evidence indicates that these are distinct populations.