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Yossathorn Tawabutr

Publications and source records attributed to Yossathorn Tawabutr.

20 records · Page 2Linked to original sources

Helicity at Small $x$: Oscillations Generated by Bringing Back the Quarks

We construct a numerical solution of the recently-derived large-$N_c \& N_f$ small-$x$ helicity evolution equations with the aim to establish the small-$x$ asymptotics of the quark helicity distribution beyond the large-$N_c$ limit explored previously in the same framework. (Here $N_c$ and $N_f$ are the numbers of quark colors and flavors.) While the large-$N_c$ helicity evolution involves gluons only, the large-$N_c \& N_f$ evolution includes contributions from quarks as well. We find that adding quarks to the evolution makes quark helicity distribution oscillate as a function of $x$. Our numerical results in the large-$N_c \& N_f$ limit lead to the $x$-dependence of the flavor-singlet quark helicity distribution which is well-approximated by \begin{align} ΔΣ(x, Q^2)\bigg|_{\mbox{large-}N_c \& N_f} \sim \left( \frac{1}{x} \right)^{α_h^q} \, \cos \left[ ω_q \, \ln \left( \frac{1}{x} \right) + φ_q \right]. \end{align} The power $α_h^q$ exhibits a weak $N_f$-dependence, and, for all $N_f$ values considered, remains very close to $α_h^q (N_f=0) = (4/\sqrt{3}) \sqrt{α_s N_c/(2 π)}$ obtained earlier in the large-$N_c$ limit. The novel oscillation frequency $ω_q$ and phase shift $φ_q$ depend more strongly on the number of flavors $N_f$ (with $ω_q =0$ in the pure-glue large-$N_c$ limit). The typical period of oscillations for $ΔΣ$ is rather long, spanning many units of rapidity. We speculate whether the oscillations we find are related to the sign variation with $x$ seen in the strange quark helicity distribution extracted from the data.

hep-ph↗

Emergent spacetime & Quantum Entanglement in Matrix theory

In the context of the Bank-Fishler-Shenker-Susskind Matrix theory, we analyze a spherical membrane in light-cone M theory along with two asymptotically distant probes. In the appropriate energy regime, we find that the membrane behaves like a smeared Matrix black hole; and the spacetime geometry seen by the probes can become non-commutative even far away from regions of Planckian curvature. This arises from non-linear Matrix interactions where fast matrix modes lift a flat direction in the potential -- akin to the Paul trap phenomenon in atomic physics. In the regime where we do have a notion of emergent spacetime, we show that there is non-zero entanglement entropy between supergravity modes on the membrane and the probes. The computation can easily be generalized to other settings, and this can help develop a dictionary between entanglement entropy and local geometry -- similar to Ryu-Takayanagi but instead for asymptotically flat backgrounds.

hep-th↗