We revisit the dynamic spin susceptibility, χ(q, ω), of one-dimensional interacting fermions. To second order in the interaction, backscattering results in a logarithmic correction to χ(q, ω) at q ≪ kF , even if the single-particle spectrum is linearized near the Fermi points. Consequently, the dynamic spin structure factor, Imχ(q, ω), is non-zero at frequencies above the single-particle continuum. In the boson language, this effect results from the marginally irrelevant backscattering operator of the sine-Gordon model. Away from the threshold, the high-frequency tail of Imχ(q, ω) due to backscattering is larger than that due to finite mass by a factor of kF /q. We derive the renormalization group equations for the coupling constants of the g-ology model at finite ω and q and find the corresponding expression for χ(q, ω), valid to all orders in the interaction but not in the immediate vicinity of the continuum boundary, where the finite-mass effects become dominant.Introduction Bosonization is the most common way to describe one-dimensional (1D) interacting fermions. 1 If the lattice effects are not essential, an exact correspondence between the fermion and fermion-hole (boson) operators maps the charge sector of the system onto a gas of free bosons [the Tomonaga-Luttinger liquid (TLL)]. The spin sector, however, is not free but maps onto the sine-Gordon model. The non-Gaussian (cosine) term of this model results from backscattering of fermions with opposite spins. If the interaction between the original fermions is repulsive, the backscattering term represents a marginally irrelevant operator and is renormalized down to zero at the fixed point, where the spin sector also becomes free. At intermediate energy scales, such marginally irrelevant operators lead to logarithmic renormalizations of the observables. 2 Since the original paper by Dzyaloshinskii and Larkin (DL), 3 it has been known that the backscattering operator gives rise to the logarithmic temperature (or external magnetic field) corrections to the static spin susceptibility. In Refs. 4 and 5, it was shown that the static spin susceptibility also depends logarithmically on the external momentum q at small q. In addition, both the spin-and charge susceptibilities at 2k F acquire multiplicative logarithmic renormalizations. 1,6 In this work, we focus on dynamics of the longwavelength part of the spin response. First, we need to outline the differences between the charge and spin sectors. As charge bosons are free at all energies, the dynamical charge structure factor (the imaginary part of the charge susceptibility at finite frequency, ω, and momentum, q) is a delta function centered at the boson dispersion, ω = v c q, which is represented by a straight line in Fig. 1A. This result differs from that for free fermions only in that the Fermi velocity, v F , is replaced by the renormalized charge velocity, v c . A non-zero width of the charge structure factor appears only if one goes beyond the TLL paradigm by taking into account finite curvature (inverse ...