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Paul Song

Publications and source records attributed to Paul Song.

3 recordsLinked to original sources

SteerDuplex: Steerable Duplex Speech Dialogue Models

Full-duplex spoken dialogue models support low-latency turn taking, interruption handling, and backchanneling, yet a key capability remains underexplored: steerability, the ability to reliably shift conversational behavior along attributes such as tone, persona, speaking rate, and voice style in response to user instructions. We introduce a taxonomy of text- and audio-based steerability that identifies substantial gaps in current full-duplex models. To address this gap, we introduce SteerDuplex, a Moshi-based full-duplex speech model fine-tuned on natural conversations and synthetic dialogues targeting instruction following, vocal delivery, reasoning, and duplex interaction. We further apply two-stage reinforcement learning (RL) with hybrid rewards, combining verifiable interaction checks and judge-based semantic feedback to improve timing and response continuity. To evaluate full-duplex spoken steerability, we introduce SteerBench, a benchmark with 390 spoken prompts and 1,067 human-authored binary audio and text rubrics spanning tone, persona, style/accent, and speed/length. On SteerBench, supervised training improves audio-steering average pass rate by 44.5 percentage points over the strongest evaluated open baseline. On Audio MultiChallenge, task average pass rate improves by 7 points over its strongest evaluated open baseline. RL further raises source-clean interruption response from 72.5% to 82.5% and reduces synthetic pause barge-in from 26.5% to 9%. Steering and aggregate task scores remain comparable or higher, while reward probes reveal reward hacking through incomplete responses. Our model and benchmark support systematic research on spoken steerability, with reward analysis showing why timing gains must be evaluated alongside response completeness.

cs.AI

Formation of the Supersonic Solar Wind: Parker's Theory Revisited

We examine and propose to fundamentally modify the classical theory of solar wind formation. To form a supersonic solar wind, the classical theory requires that a subsonic flow speed must start at a specific initial speed from the coronal base, called eigenspeed, go along a continuous eigenfunction, and reach the sonic point, which is where the flow speed equals the sonic speed, while the critical condition, which is where the effective driving force is zero, is satisfied. Any mismatch between the sonic point and critical condition distances results in either subsonic winds when the initial speed is below the eigenspeed, or no solar wind when the initial speed is above the eigenspeed. Because the critical condition is determined by the solar wind temperature profile, which depends on ionization process at the top of the chromosphere and the heating process around the coronal base but not by the processes at the sonic point, the required match between the two is generally not met and hence the momentum equation in the conventional theory encounters difficulty when the initial speed is above the eigenspeed. To resolve the difficulty, we propose a discontinuity between the sonic point and the critical condition to reach supersonic solar wind solutions. As a result, supersonic solar winds can be produced when the initial speed in the coronal base is greater than the eigenspeed. The critical solution or eigen function provided by the conventional solar wind model describes the condition that separates the supersonic solar winds from subsonic ones.

astro-ph.SR

Time-Dependent Two-Fluid Magnetohydrodynamic Model and Simulation of the Chromosphere

The sun's chromosphere is a highly dynamic, partially-ionized region where spicules (hot jets of plasma) form. Here we present a two-fluid MHD model to study the chromosphere, which includes ion-neutral interaction and frictional heating. Our simulation recovers a magnetic canopy shape that forms quickly, but is also quickly disrupted by the formation of a jet. Our simulation produces a shock self-consistently, where the jet is driven by the frictional heating, which is much greater than the ohmic heating. Thus, our simulation demonstrates that the jet could be driven purely by thermal effects due to ion-neutral collisions and not by magnetic reconnection. We plan to improve the model to include photo-chemical effects and radiation.

astro-ph.SR