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Tutorial#gpu📝 BlogAnalyzed: Dec 28, 2025 15:31

Monitoring Windows GPU with New Relic

Published:Dec 28, 2025 15:01
1 min read
Qiita AI

Analysis

This article discusses monitoring Windows GPUs using New Relic, a popular observability platform. The author highlights the increasing use of local LLMs on Windows GPUs and the importance of monitoring to prevent hardware failure. The article likely provides a practical guide or tutorial on configuring New Relic to collect and visualize GPU metrics. It addresses a relevant and timely issue, given the growing trend of running AI workloads on local machines. The value lies in its practical approach to ensuring the stability and performance of GPU-intensive applications on Windows. The article caters to developers and system administrators who need to monitor GPU usage and prevent overheating or other issues.
Reference

最近は、Windows の GPU でローカル LLM なんていうこともやることが多くなってきていると思うので、GPU が燃え尽きないように監視も大切ということで、監視させてみたいと思います。

Analysis

This paper proposes a classically scale-invariant extension of the Zee-Babu model, a model for neutrino masses, incorporating a U(1)B-L gauge symmetry and a Z2 symmetry to provide a dark matter candidate. The key feature is radiative symmetry breaking, where the breaking scale is linked to neutrino mass generation, lepton flavor violation, and dark matter phenomenology. The paper's significance lies in its potential to be tested through gravitational wave detection, offering a concrete way to probe classical scale invariance and its connection to fundamental particle physics.
Reference

The scenario can simultaneously accommodate the observed neutrino masses and mixings, an appropriately low lepton flavour violation and the observed dark matter relic density for 10 TeV ≲ vBL ≲ 55 TeV. In addition, the very radiative nature of the set-up signals a strong first order phase transition in the presence of a non-zero temperature.

Analysis

This paper proposes a novel method to detect primordial black hole (PBH) relics, which are remnants of evaporating PBHs, using induced gravitational waves. The study focuses on PBHs that evaporated before Big Bang nucleosynthesis but left behind remnants that could constitute dark matter. The key idea is that the peak positions and amplitudes of the induced gravitational waves can reveal information about the number density and initial abundance of these relics, potentially detectable by future gravitational wave experiments. This offers a new avenue for probing dark matter and the early universe.
Reference

The peak frequency scales as $f_{ ext {relic }}^{1 / 3}$ where $f_{ ext {relic }}$ is the fraction of the PBH relics in the total DM density.

Research#llm📝 BlogAnalyzed: Dec 27, 2025 00:31

New Relic, LiteLLM Proxy, and OpenTelemetry

Published:Dec 26, 2025 09:06
1 min read
Qiita LLM

Analysis

This article, part of the "New Relic Advent Calendar 2025" series, likely discusses the integration of New Relic with LiteLLM Proxy and OpenTelemetry. Given the title and the introductory sentence, the article probably explores how these technologies can be used together for monitoring, tracing, and observability of LLM-powered applications. It's likely a technical piece aimed at developers and engineers who are working with large language models and want to gain better insights into their performance and behavior. The author's mention of "sword and magic and academic society" seems unrelated and is probably just a personal introduction.
Reference

「New Relic Advent Calendar 2025 」シリーズ4・25日目の記事になります。