papers

Publications (28)

astro-ph.HE2018

Probing the physics of newly born magnetars through observation of superluminous supernovae

Quan Cheng, Shuang-Nan Zhang, Yun-Wei Yu +1

The central engines of some superluminous supernovae (SLSNe) are generally suggested to be newly born fast rotating magnetars, which spin down mainly through magnetic dipole radiat…

cs.AI2026

Via Negativa for AI Alignment: Why Negative Constraints Are Structurally Superior to Positive Preferences

Quan Cheng

Recent empirical results have demonstrated that training large language models (LLMs) with negative-only feedback can match or exceed standard reinforcement learning from human fee…

cs.AR2026

PDAGENT-BENCH: Characterizing, Grounding, and Architecting LLM/VLM Agents for VLSI Physical Design

Qiufeng Li, Rongqian Chen, Quan Cheng +6

The paper presents PDAGENT-BENCH, a benchmark suite and workflow framework for evaluating large language model and vision‑language model agents on VLSI physical design tasks, cover…

#benchmarking#llm agents#vlsi physical design#eda workflow
astro-ph.HE2024

Constraints on the internal physics of neutron stars from the observational data of several young pulsars: the role of a power-law decaying dipole magnetic field

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng

The observational data (e.g., the timing data and magnetic tilt angles ) of young pulsars can be used to probe some critical issues about the internal physics of neutron stars…

cs.AI2026

Why the Valuable Capabilities of LLMs Are Precisely the Unexplainable Ones

Quan Cheng

This paper proposes and argues for a counterintuitive thesis: the truly valuable capabilities of large language models (LLMs) reside precisely in the part that cannot be fully capt…

astro-ph.HE2021

Constraining mechanism associated with fast radio burst and glitch from SGR J1935

Wei-Hua Wang, Heng Xu, Wei-Yang Wang +4

The discovery of fast radio burst (FRB) 200428 from galactic SGR J1935+2154 makes it possible to measure rotational changes accompanied by FRBs and to test several FRB models which…

cs.CV2026

Stable Routing for Mixture-of-Experts in Class-Incremental Learning

Zirui Guo, Quan Cheng, Da-Wei Zhou +1

Class-incremental learning (CIL) requires models to learn new classes sequentially while preserving prior knowledge. Recently, approaches that combine pre-trained models with mixtu…

astro-ph.HE2024

Investigating the neutron star physics through observations of several young pulsars in the dipole-field re-emergence scenario

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng

The observed timing data, magnetic tilt angle , and age of young pulsars could be used to probe some important issues about neutron star (NS) physics, e.g., the NS internal mag…

astro-ph.HE2026

Exploring Superfluid Angular Momentum Reservoir Effect on Pulsar Glitches and Forecasting Next Glitches of the Crab Pulsar

Pei-Xin Zhu, Xiao-Ping Zheng, Quan Cheng +2

Pulsar glitches are generally viewed as stochastic events driven by sudden angular momentum transfer from the neutron star's superfluid interior to its crust. Except two peculiar p…

astro-ph.HE2017

A possible origin of the Galactic Center magnetar SGR 1745-2900

Quan Cheng, Shuang-Nan Zhang, Xiao-Ping Zheng

Since a large population of massive O/B stars and putative neutron stars (NSs) located in the vicinity of the Galactic center (GC), intermediate-mass X-ray binaries (IMXBs) constit…

astro-ph.SR2015

Stochastic gravitational wave background from magnetic deformation of newly born magnetars

Quan Cheng, Yun-Wei Yu, Xiao-Ping Zheng

Newly born magnetars are promising sources for gravitational wave (GW) detection due to their ultra-strong magnetic fields and high spin frequencies. Within the scenario of a growi…

cs.CV2025

Continuous Subspace Optimization for Continual Learning

Quan Cheng, Yuanyu Wan, Lingyu Wu +2

Continual learning aims to learn multiple tasks sequentially while preserving prior knowledge, but faces the challenge of catastrophic forgetting when adapting to new tasks. Recent…

hep-ph2017

Bondi accretion of dark matter by neutron stars

Xi Huang, Jian-Feng Liu, Wei-Hua Wang +2

In this paper, we have compared two different accretion mechanisms of dark matter particles by a canonical neutron star with and , and shown the ef…

astro-ph.HE2025

Could the stochastic gravitational wave background from newborn magnetars be detected by the advanced LIGO and Einstein Telescope?

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng +1

Newborn magnetars are important gravitational wave sources due to their ultra-strong magnetic fields and fast spins, and the entire population in the Universe may significantly con…

astro-ph.HE2025

Physics of Strong Magnetism with eXTP

Mingyu Ge, Long Ji, Roberto Taverna +47

In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission, in its new configuration, for studies of strongly magnetized compact obj…

astro-ph.HE2026

Superfluid Angular Momentum Reservoir Effect in Pulsar Glitches and Crab Pulsar Glitch Time Prediction

Pei-Xin Zhu, Xiao-Ping Zheng, Quan Cheng +2

Pulsar glitches are usually regarded as stochastic, independent events triggered by sudden angular momentum transfer from the neutron star's superfluid interior to its crust. Howev…

astro-ph.HE2019

What can PSR J1640-4631 tell us about the internal physics of this neutron star?

Quan Cheng, Shuang-Nan Zhang, Xiao-Ping Zheng +1

Gravitational wave emissions (GWEs) of pulsars could not only make them promising targets for continuous gravitational wave searches but also leave imprints in their timing data. W…

astro-ph.HE2014

How can newly born rapidly rotating neutron stars become magnetars?

Quan Cheng, Yun-Wei Yu

In a newly born (high-temperature and Keplerian rotating) neutron star, r-mode instability can lead to stellar differential rotation, which winds the seed poloidal magnetic field (…

astro-ph.SR2013

Could strange stars be in the color-flavor-locked phase: Tested by their thermal evolutions

Quan Cheng, Yun-Wei Yu, Xiao-Ping Zheng

The thermal evolution of strange stars in both normal and color-flavor-locked (CFL) phases are investigated together with the evolutions of the stellar rotation and the r-mode inst…

astro-ph.HE2024

On the initial spin periods of magnetars born in weak supernova explosions and their gravitational wave radiation

Yu-Long Yan, Quan Cheng, Xiao-Ping Zheng +1

The initial spin periods of newborn magnetars are \textbf{strongly associated with the origin of their strong magnetic fields, both of which can affect the electromagnetic radiatio…

astro-ph.HE2025

Dense Matter in Neutron Stars with eXTP

Ang Li, Anna L. Watts, Guobao Zhang +82

In this White Paper, we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission to constrain the equation of state of dense matter in neutron stars, explo…

cs.AR2025

Efficient Calibration for RRAM-based In-Memory Computing using DoRA

Weirong Dong, Kai Zhou, Zhen Kong +5

Resistive In-Memory Computing (RIMC) offers ultra-efficient computation for edge AI but faces accuracy degradation due to RRAM conductance drift over time. Traditional retraining m…

astro-ph.HE2017

Stochastic gravitational wave background from newly born massive magnetars: The role of a dense matter equation of state

Quan Cheng, Shuang-Nan Zhang, Xiao-Ping Zheng

Newly born massive magnetars are generally considered to be produced by binary neutron star (NS) mergers, which could give rise to short gamma-ray bursts (SGRBs). The strong magnet…

astro-ph.HE2025

Revealing the internal magnetic field configuration of magnetars via their associated periodic signals

Jie Shu, Quan Cheng, Xiao-Ping Zheng

The magnetic deformation of magnetars is affected by their internal magnetic fields, which are generally difficult to be measured directly through observations. In this work, the p…

cs.AR2026

Heterogeneity-Aware Microscaling for Efficient Low-Bit LLM Inference

Junyi Luo, Xinting Jiang, Tai-Hao Wen +9

Microscaling (MX) is now the standard for low-bit large language model (LLM) inference. Its 4-bit form MXFP4 still loses substantial accuracy, because existing MX formats fix eithe…

astro-ph.HE2026

Studies on the spin and magnetic inclination evolution of magnetars Swift J1834.9-0846 under wind braking

Biaopeng Li, Zhifu Gao, Wenqi Ma +3

The magnetar Swift J1834.9-0846 presents a significant challenge to neutron star spin-down models. It exhibits two key anomalies: an insufficient rotational energy loss rate to pow…

cs.AR2026

VeRA+: Vector-Based Lightweight Digital Compensation for Drift-Resilient RRAM In-Memory Computing

Weirong Dong, Kai Zhou, Zhen Kong +8

RRAM-based in-memory computing (IMC) offers high energy efficiency but suffers from conductance drift that severely degrades long-term accuracy. Existing approaches including retra…

cs.HC2023

STAGER checklist: Standardized Testing and Assessment Guidelines for Evaluating Generative AI Reliability

Jinghong Chen, Lingxuan Zhu, Weiming Mou +5

Generative Artificial Intelligence (AI) holds immense potential in medical applications. Numerous studies have explored the efficacy of various generative AI models within healthca…