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Yu-Chung Chen

Publications and source records attributed to Yu-Chung Chen.

4 recordsLinked to original sources

A Modular and T-Gate Efficient Architecture for Quantum Leading-Zero/One Counter

The Quantum Leading-Zero/One Counter (QLZOC) is a fundamental component in quantum arithmetic, playing a critical role in normalization, floating-point units, dynamic range scaling, and logarithmic approximations. Conventional designs primarily rely on direct Boolean-to-quantum mapping, which results in inefficient resource utilization such as irregular gate growth and width-dependent resource overhead. In this work, we propose a scalable, modular, and resource efficient architecture for QLZOC by reformulating the counting process into a sequence of systematic conditional bit-flip operations. Moreover, our design achieves functional polymorphism so that the same design can be easily toggled between zero and one detection, while ensuring seamless scalability to any bit-width without manual re-tuning. We further introduce a Parallel QLZOC (PQLZOC) variant and a Fan-Out optimized (FO-PQLZOC) design. In this work, we evaluate resource efficiency based on the classic criteria about T gates, including the number of total T gates being used (T-count) and the number of sequential T gate layers (T-depth). By exploiting the properties of all-zero/one qubit blocks and a hierarchical merge strategy, the proposed FO-PQLZOC reduces the T-depth from O(m) to O(log m), where m is the input size. Comparative analysis demonstrates that our optimized architecture achieves a 40% reduction in T-count and a 60% reduction in T-depth over state-of-the-art designs, providing a high-performance, T-gate efficient solution for general-purpose quantum arithmetic processors.

quant-ph

Feasibility-Guided Planning over Multi-Specialized Locomotion Policies

Planning over unstructured terrain presents a significant challenge in the field of legged robotics. Although recent works in reinforcement learning have yielded various locomotion strategies, planning over multiple experts remains a complex issue. Existing approaches encounter several constraints: traditional planners are unable to integrate skill-specific policies, whereas hierarchical learning frameworks often lose interpretability and require retraining whenever new policies are added. In this paper, we propose a feasibility-guided planning framework that successfully incorporates multiple terrain-specific policies. Each policy is paired with a Feasibility-Net, which learned to predict feasibility tensors based on the local elevation maps and task vectors. This integration allows classical planning algorithms to derive optimal paths. Through both simulated and real-world experiments, we demonstrate that our method efficiently generates reliable plans across diverse and challenging terrains, while consistently aligning with the capabilities of the underlying policies.

cs.RO

The creation of radiation and the relic of inflaton potential

Recently, we have performed research on the subject of the cosmological constant problem. The scenario is based on two postulates for inflationary theory: one is that inflaton $ϕ$ can interact with radiation (relativistic particles); the other is that radiation will be created continuously during and after the epoch of inflation. According to these postulates and from a "macroscopic perspective", we discover that radiation can be viewed as a product of the interaction between $\dotϕ$ and some "effective kinetic frictional force" that exists in inflaton dynamics. Deducing and surmising from "effective friction", we obtain conclusions of two special types of expanding universe: A Type I universe will finally enter an expanding course after a special time $t_{*}$ with uniformly rolling $\dotϕ(t_{*})$ due to the balance between $V^{'}(ϕ(t))$, 3H(t)\dotϕ(t_{*}) and the "effective kinetic frictional force". In this result, the expanding course will see particles created continuously. Additionally, for a Type II universe, $ϕ$ will be at rest after $t_{r}$ inside a region named the "stagnant zone" that is formed by the "maximum effective static frictional force". Consistent with this, inflaton potential will survive as a relic $V(ϕ(t_{r}))$, playing the role of the effective cosmological constant $Λ$ .

gr-qc

The Cosmological Constant as a Ghost of Inflaton

The cosmological constant (term) is the simplest way, presently known, to illustrate the accelerating expansion of the universe. However, because of/despite its simple appearance, there is much confusion surrounding its essence. Theorists have been asking questions for years: Is there a mechanism to explain this term? Is it really a constant or a variable? Moreover, it seems that we have created a huge gulf separating the theories of inflation and accelerating expansion. Can we eliminate such an uncomfortable discontinuity? Abstract In this paper, we will journey to see the growth of the universe from the very beginning of inflation. To simplify our discussion, we will briefly "turn off" the effects of real and dark matter and shall use inflaton (a classical scalar field) dynamics with a time-varying inflaton potential V(phi,t) as the screen to watch this process. Relying on these conditions, we propose a non-traditional method of obtaining the solution of scale factor R(t), which is only dependent on phi'(t)^2, and discover that the term R"(t)/R(t) will be a constant after kinetic inflaton phi'(t) is at rest. This result can be regarded as the effective cosmological constant phenomenally. Moreover, we will also "rebuild" V(phi,t), realize its evolutionary process and then, according to the relationship between V(phi,t) and phi'(t)^2, it will be possible to smoothly describe the whole evolution of the universe from the epoch of inflation. Therefore, the implications of our findings will mean that the gulf between theories will disappear. Lastly, we will also see how the formula could provide a framework for solving the old and new cosmological constant problems as well as much more besides.

gr-qc