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10x increase in atom array size boosts China’s quantum leap

Chinese researchers unveil 10x larger atom array for next-gen quantum processors.


Scientists in China have achieved a significant breakthrough in advancing quantum physics.

A team of researchers has developed the largest array of atoms for quantum computing.

The key component for a quantum computer is reportedly capable of creating arrays 10 times larger than previous systems.

Building energy model offers cities decarbonization roadmap

A new software tool developed by Cornell researchers can model a small city’s building energy use within minutes on a standard laptop, then run simulations to help policymakers prioritize the most cost-effective approaches to decarbonization.

Using the City of Ithaca, New York, as a , the urban building energy model quickly mapped more than 5,000 residential and and their baseline energy use. Simulated investments in weatherization, electric heat pumps and rooftop solar panels, while also factoring in financial incentives, generated insights that are informing city efforts to achieve carbon neutrality by 2030.

The tool’s automated workflow, accessibility and accuracy—without advanced computing power—could be particularly valuable for smaller cities that lack resources and expertise dedicated to decarbonization, the researchers said. But they said the new model—now also supporting the county that surrounds Ithaca—could be further scaled up to serve big cities or an entire state.

View a PDF of the paper titled Characterizing Deep Research: A Benchmark and Formal Definition, by Abhinav Java and 8 other authors

Information tasks such as writing surveys or analytical reports require complex search and reasoning, and have recently been grouped under the umbrella of \textit{deep research} — a term also adopted by recent models targeting these capabilities. Despite growing interest, the scope of the deep research task remains underdefined and its distinction from other reasoning-intensive problems is poorly understood. In this paper, we propose a formal characterization of the deep research (DR) task and introduce a benchmark to evaluate the performance of DR systems. We argue that the core defining feature of deep research is not the production of lengthy report-style outputs, but rather the high fan-out over concepts required during the search process, i.e., broad and reasoning-intensive exploration. To enable objective evaluation, we define DR using an intermediate output representation that encodes key claims uncovered during search-separating the reasoning challenge from surface-level report generation. Based on this formulation, we propose a diverse, challenging benchmark LiveDRBench with 100 challenging tasks over scientific topics (e.g., datasets, materials discovery, prior art search) and public interest events (e.g., flight incidents, movie awards). Across state-of-the-art DR systems, F1 score ranges between 0.02 and 0.72 for any sub-category. OpenAI’s model performs the best with an overall F1 score of 0.55. Analysis of reasoning traces reveals the distribution over the number of referenced sources, branching, and backtracking events executed by current DR systems, motivating future directions for improving their search mechanisms and grounding capabilities. The benchmark is available at https://github.com/microsoft/LiveDRBench.

Wow! We Finally Have Evidence of a Planet in the Nearby Alpha Centauri

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Hello and welcome! My name is Anton and in this video, we will talk about new evidence for a large planet in the Alpha Centauri system near us.
Links:

NASA’s Webb Finds New Evidence for Planet Around Closest Solar Twin


https://arxiv.org/pdf/2508.03814
https://arxiv.org/pdf/2508.03812
https://iopscience.iop.org/article/10.3847/2515-5172/add880/meta.
Other videos:



#alphacentauri #planet #jameswebbspacetelescope.

0:00 Alpha centauri surprise!
0:40 What we know about the star system so far.
2:57 Potential detection in 2019
3:35 Why JWST is so good at this but there were still challenges.
4:55 Methods used to observe this star.
5:30 Surprise results and the initial analysis.
8:00 Non detection at later dates was important! Orbits worked out.
9:15 What we know about the planet so far.
11:30 Could this be rings?
12:30 What this implies and conclusions.
13:30 What’s next?

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