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Michael J. Yuan

Publications and source records attributed to Michael J. Yuan.

4 recordsLinked to original sources

The Economics of AI Decoding Chips: Rebalancing Compute, Capacity, and Bandwidth for Efficient LLM Inference

Every mainstream GPU is built compute-heavy and capacity-light: it pairs enormous arithmetic throughput with too little memory to hold a modern model. In contrast, large language model decoding requires little compute and a large amount of memory: a GPU's floating-point units run at single-digit-percent utilization during decoding, and the memory the workload does need is sold only bundled with yet more compute. The compute is recovered only at hyperscale, where Mixture-of-Experts (MoE) models are spread across 96--320-GPU expert-parallel clusters serving thousands of concurrent users, a scale available to a handful of operators. We formalize the inefficiency with two fixed per-chip constants. F/B, the roofline ridge point, determines whether the compute can be utilized; F/S, the compute bundled with each GB of memory, determines how much compute must be bought. We then argue for a rebalanced decode accelerator: less compute, far more commodity memory, and a deliberately lower and cheaper bandwidth. The Skymizer HTX-301, a purpose-built 28nm PCIe accelerator using commodity DDR5, occupies that design point. Its entry cost is low. A single eight-chip card holds DeepSeek-R1 671B for about \$19,000, and a 4U server of four four-chip cards serves two users at a deterministic 20.3 tokens per second each for about \$28,000. Either costs less than a single H100, while the minimum GPU deployment for the model is an eight-GPU node near \$350,000. Concurrency then scales out by adding hardware: eight 4U servers carry sixteen users for about \$224,000, two-thirds of the node's price, with the cost per token unchanged at about \$12 per million against the node's \$21. The HTX-301's decisive advantage is a supply chain free of every rationed input: it uses no high-bandwidth memory, no CoWoS, and no leading-edge logic.

cs.AR↗

Trust, but verify

Decentralized AI agent networks, such as Gaia, allows individuals to run customized LLMs on their own computers and then provide services to the public. However, in order to maintain service quality, the network must verify that individual nodes are running their designated LLMs. In this paper, we demonstrate that in a cluster of mostly honest nodes, we can detect nodes that run unauthorized or incorrect LLM through social consensus of its peers. We will discuss the algorithm and experimental data from the Gaia network. We will also discuss the intersubjective validation system, implemented as an EigenLayer AVS to introduce financial incentives and penalties to encourage honest behavior from LLM nodes.

cs.AI↗

The Physics of Blazar Optical Emission Regions I: Alignment of Optical Polarization and the VLBI Jet

We collected optical and near IR linear polarization data obtained over 20--30 years for a sample of 51 blazars. For each object, we calculated the probability that the distribution of position angles was isotropic. The distribution of these probabilities was sharply peaked, with 27 blazars showing a probability < 15% of an isotropic distribution of position angles. For these 27 objects we defined a preferred position angle. For those 17 out of 27 blazars showing a well-defined radio structure angle (jet position angle) on VLBI scales (1--3mas), we looked at the distribution of angle differences -- the optical polarization relative to the radio position angles. This distribution is sharply peaked, especially for the BL Lac objects, with alignment better than 15 degrees for half the sample. Those blazars with preferred optical position angles were much less likely to have bent jets on 1--20mas scales. These results support a shock-in-jet hypothesis for the jet optical emission regions.

astro-ph↗

The Physics of Blazar Optical Emission Regions II: Magnetic Field Orientation, Viewing Angle and Beaming

For a sample of 51 blazars with extensive optical polarization data, we used circular statistics to calculate the scatter among the polarization position angles for each object. We found that this scatter is correlated with the radio core dominance. We compared this relationship with the predictions of a simple transverse shock model. The result suggests that blazar jets are likely to cover a wide range of speeds consistent with those derived from observations of superluminal motion.

astro-ph↗