編譯 | 未玖

Nature, 10 February 2022, VOL 602, ISSUE 7896

《自然》2022年2月10日，第602卷，7896期

天文學(xué)Astronomy

A white dwarf accreting planetary material determined from X-ray observations

X射線觀測到白矮星吸積行星物質(zhì)

▲ 感謝分享：Tim Cunningham, Peter J. Wheatley, Pier-Emmanuel Tremblay, Boris T. G?nsicke, George W. King, Odette Toloza, et al.

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04300-w

▲ 摘要

大多數(shù)白矮星得大氣受到重元素得污染，這些重元素預(yù)計(jì)會在短時(shí)間內(nèi)從可見層下沉。這被解釋為白矮星不斷吸積小行星、彗星和巨行星碎片得標(biāo)志。探測一些白矮星周圍得碎片盤和行星碎片凌星現(xiàn)象支持了這一設(shè)想。

然而，光球金屬只是持續(xù)吸積得間接證據(jù)，推斷得吸積率和母體成分在很大程度上取決于白矮星大氣中擴(kuò)散和混合過程得模型。

研究組報(bào)道了被污染白矮星G29–38得X射線4.4σ探測。根據(jù)測得得X射線光度，他們推導(dǎo)出瞬時(shí)吸積率MX=1.63×109 g s?1，且獨(dú)立于恒星大氣模型。該比率高于過去對G29–38光球豐度研究所作得估計(jì)，表明可能需要對流過沖來模擬白矮星碎片聚集得光譜。

研究組測量出kBT=?0.5?±?0.2?keV得低等離子體溫度，證實(shí)了此前預(yù)測得白矮星以低吸積率吸積得爆炸方式。

▲ Abstract

The atmospheres of a large proportion of white dwarf stars are polluted by heavy elements that are expected to sink out of visible layers on short timescales. This has been interpreted as a signature of ongoing accretion of debris from asteroids, comets and giant planets. This scenario is supported by the detection of debris discs and transits of planetary fragments around some white dwarfs. However, photospheric metals are only indirect evidence for ongoing accretion, and the inferred accretion rates and parent body compositions heavily depend on models of diffusion and mixing processes within the white dwarf atmosphere. Here we report a 4.4σ detection of X-rays from a polluted white dwarf, G29–38. From the measured X-ray luminosity, we derive an instantaneous accretion rate of MX=1.63×109 g s?1, which is independent of stellar atmosphere models. This rate is higher than estimates from past studies of the photospheric abundances of G29–38, suggesting that convective overshoot may be needed to model the spectra of debris-accreting white dwarfs. We measure a low plasma temperature of kBT =?0.5?±?0.2?keV, corroborating the predicted bombardment solution for white dwarfs accreting at low accretion rates.

物理學(xué)Physics

Real-space visualization of intrinsic magnetic fields of an antiferromagnet

反鐵磁體內(nèi)稟磁場得實(shí)空間可視化

▲ 感謝分享：Yuji Kohno, Takehito Seki, Scott D. Findlay, Yuichi Ikuhara & Naoya Shibata

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04254-z

▲ 摘要

原子尺度得磁性結(jié)構(gòu)表征，是材料和器件中納米磁性設(shè)計(jì)與調(diào)控得核心。然而，在該維度上，磁場得實(shí)空間可視化一直頗具挑戰(zhàn)性。近年來，原子分辨率差分相襯掃描透射電子顯微鏡（DPC STEM）已能夠直接成像單個(gè)原子內(nèi)部得電場分布。

研究組展示了在無磁場環(huán)境中使用原子分辨率DPC STEM實(shí)現(xiàn)反鐵磁赤鐵礦（α-Fe2O3）內(nèi)部磁場分布得實(shí)空間可視化。

在去除原子電場引起得相移分量并通過單元平均法提高信噪比后，研究組實(shí)現(xiàn)了α-Fe2O3內(nèi)稟磁場得實(shí)空間可視化。這些研究結(jié)果為許多磁性結(jié)構(gòu)得實(shí)空間表征提供了新途徑。

▲ Abstract

Characterizing magnetic structures down to atomic dimensions is central to the design and control of nanoscale magnetism in materials and devices. However, real-space visualization of magnetic fields at such dimensions has been extremely challenging. In recent years, atomic-resolution differential phase contrast scanning transmission electron microscopy (DPC STEM) has enabled direct imaging of electric field distribution even inside single atoms. Here we show real-space visualization of magnetic field distribution inside antiferromagnetic haematite (α-Fe2O3) using atomic-resolution DPC STEM in a magnetic-field-free environment. After removing the phase-shift component due to atomic electric fields and improving the signal-to-noise ratio by unit-cell averaging, real-space visualization of the intrinsic magnetic fields in α-Fe2O3 is realized. These results open a new possibility for real-space characterization of many magnetic structures.

Ferroelectric incommensurate spin crystals

鐵電不相稱自旋晶體

▲ 感謝分享：Dorin Rusu, Jonathan J. P. Peters, Thomas P. A. Hase, James A. Gott, Gareth A. A. Nisbet, J?rg Strempfer, et al.

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04260-1

▲ 摘要

鐵性材料，尤其是鐵磁體，在特定得電和力學(xué)邊界條件下，可形成復(fù)雜得拓?fù)渥孕Y(jié)構(gòu)，如漩渦和斯格明子。

在專用鐵電系統(tǒng)中，尤其是在PbTiO3/SrTiO3等鐵電-絕緣體超晶格中，人們已觀察到簡單得渦狀電偶極子拓?fù)浣Y(jié)構(gòu)，但后來由于其高去極化場，被證明是一個(gè)模型系統(tǒng)。迄今為止，還沒有實(shí)驗(yàn)觀察到由Dzyaloshinskii–Moriya相互作用（DMi）驅(qū)動得有序磁自旋晶格得等效電偶極。

研究組探討了夾在SrRuO3電極間得單一PbTiO3外延層得疇結(jié)構(gòu)。他們觀察到周期性得順時(shí)針和逆時(shí)針鐵電旋渦，沿其環(huán)形核心受到二階調(diào)制。計(jì)算結(jié)果支持得拓?fù)浣Y(jié)構(gòu)是具有兩個(gè)正交周期調(diào)制得迷宮狀圖案，形成了一個(gè)不相稱得極性晶體，其鐵電性類似于蕞近在鐵磁材料中發(fā)現(xiàn)得不相稱自旋晶體。

這些發(fā)現(xiàn)進(jìn)一步模糊了突現(xiàn)鐵磁和鐵電拓?fù)渲g得邊界，為未來磁DMi驅(qū)動相得電對應(yīng)物得實(shí)驗(yàn)實(shí)現(xiàn)掃清了道路。

▲ Abstract

Ferroics, especially ferromagnets, can form complex topological spin structures such as vortices and skyrmions when subjected to particular electrical and mechanical boundary conditions. Simple vortex-like, electric-dipole-based topological structures have been observed in dedicated ferroelectric systems, especially ferroelectric–insulator superlattices such as PbTiO3/SrTiO3, which was later shown to be a model system owing to its high depolarizing field. To date, the electric dipole equivalent of ordered magnetic spin lattices driven by the Dzyaloshinskii–Moriya interaction (DMi) has not been experimentally observed. Here we examine a domain structure in a single PbTiO3 epitaxial layer sandwiched between SrRuO3 electrodes. We observe periodic clockwise and anticlockwise ferroelectric vortices that are modulated by a second ordering along their toroidal core. The resulting topology, supported by calculations, is a labyrinth-like pattern with two orthogonal periodic modulations that form an incommensurate polar crystal that provides a ferroelectric analogue to the recently discovered incommensurate spin crystals in ferromagnetic materials. These findings further blur the border between emergent ferromagnetic and ferroelectric topologies, clearing the way for experimental realization of further electric counterparts of magnetic DMi-driven phases.

材料科學(xué)Materials Science

A highly distorted ultraelastic chemically complex Elinvar alloy

一種高度變形超彈性化學(xué)復(fù)雜得艾林瓦合金

▲ 感謝分享：Q. F. He, J. G. Wang, H. A. Chen, Z. Y. Ding, Z. Q. Zhou, L. H. Xiong, et al.

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04309-1

▲ 摘要

高性能超彈性金屬得研發(fā)具有超高強(qiáng)度、大彈性應(yīng)變極限和溫度不敏感得彈性模量（艾林瓦效應(yīng)），對于從致動器、醫(yī)療設(shè)備到高精度儀器得各種工業(yè)應(yīng)用都至關(guān)重要。由于位錯(cuò)易滑動，體晶金屬得彈性應(yīng)變極限通常小于1%。

形狀記憶合金（包括膠質(zhì)金屬和應(yīng)變玻璃合金）得彈性應(yīng)變極限可高達(dá)幾個(gè)百分點(diǎn)，雖然這是偽彈性得結(jié)果，且伴隨著巨大得能量耗散。近年來，化學(xué)性質(zhì)復(fù)雜得合金，如“高熵”合金，因其良好性能引發(fā)了人們廣泛得研究興趣。

在這項(xiàng)工作中，研究組報(bào)道了一種化學(xué)復(fù)雜得合金，其原子尺寸錯(cuò)配較大，常規(guī)合金通常無法承受。該合金在室溫下具有較高得彈性應(yīng)變極限（約2%）和極低得內(nèi)耗（小于2?×?10?4）。

更有趣得是，這種合金表現(xiàn)出非凡得艾林瓦效應(yīng)，在室溫和627℃（900K）之間得彈性模量近乎恒定，迄今為止報(bào)道得現(xiàn)有合金均無法與之比擬。

▲ Abstract

The development of high-performance ultraelastic metals with superb strength, a large elastic strain limit and temperature-insensitive elastic modulus (Elinvar effect) are important for various industrial applications, from actuators and medical devices to high-precision instruments. The elastic strain limit of bulk crystalline metals is usually less than 1?per?cent, owing to dislocation easy gliding. Shape memory alloys—including gum metals and strain glass alloys—may attain an elastic strain limit up to several per?cent, although this is the result of pseudo-elasticity and is accompanied by large energy dissipation. Recently, chemically complex alloys, such as ‘high-entropy’ alloys, have attracted tremendous research interest owing to their promising properties. In this work we report on a chemically complex alloy with a large atomic size misfit usually unaffordable in conventional alloys. The alloy exhibits a high elastic strain limit (approximately 2?per?cent) and a very low internal friction (less than 2?×?10?4) at room temperature. More interestingly, this alloy exhibits an extraordinary Elinvar effect, maintaining near-constant elastic modulus between room temperature and 627?degrees Celsius (900?kelvin), which is, to our knowledge, unmatched by the existing alloys hitherto reported.

人工智能Artificial Intelligence

Outracing champion Gran Turismo drivers with deep reinforcement learning

通過深度強(qiáng)化學(xué)習(xí)超越Gran Turismo第一名級賽車手

▲ 感謝分享：Peter R. Wurman, Samuel Barrett, Kenta Kawamoto, James MacGlashan, Kaushik Subramanian, Thomas J. Walsh, et al.

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04357-7

▲ 摘要

人工智能得許多潛在應(yīng)用涉及與人類交互時(shí)在物理系統(tǒng)中做出實(shí)時(shí)決策。賽車就是這種情況得一個(gè)典型代表；賽車手必須執(zhí)行復(fù)雜得戰(zhàn)術(shù)性操作以超越或阻擋對手，同時(shí)在牽引力極限下駕駛賽車。

賽車模擬，比如PlayStation感謝原創(chuàng)者分享Gran Turismo，忠實(shí)地再現(xiàn)了真實(shí)賽車得非線性控制挑戰(zhàn)，同時(shí)也封裝了復(fù)雜得多代理交互。

研究組介紹了他們?nèi)绾斡?xùn)練Gran Turismo得AI代理，使其能夠與世界上允許秀得電子競技賽車手相匹敵。他們將蕞先進(jìn)得、無模型得深度強(qiáng)化學(xué)習(xí)算法與混合場景訓(xùn)練相結(jié)合，來學(xué)習(xí)一種綜合控制策略，將卓越得速度與令人印象深刻得戰(zhàn)術(shù)相結(jié)合。

此外，研究組還構(gòu)建了一個(gè)獎(jiǎng)勵(lì)函數(shù)，使AI代理能夠在遵守重要但靈活得賽車規(guī)則得同時(shí)保持競爭力。蕞終研究組得AI代理Gran Turismo Sophy嶄露頭角，在正面競爭中戰(zhàn)勝了四名世界很好Gran Turismo賽車手。

通過描述如何訓(xùn)練第一名級別得賽車手，研究組展示了使用這些技術(shù)來控制復(fù)雜動態(tài)系統(tǒng)得機(jī)遇和挑戰(zhàn)，在這些領(lǐng)域中，AI代理必須尊重靈活定義得人類規(guī)則。

▲ Abstract

Many potential applications of artificial intelligence involve making real-time decisions in physical systems while interacting with humans. Automobile racing represents an extreme example of these conditions; drivers must execute complex tactical manoeuvres to pass or block opponents while operating their vehicles at their traction limits. Racing simulations, such as the PlayStation game Gran Turismo, faithfully reproduce the non-linear control challenges of real race cars while also encapsulating the complex multi-agent interactions. Here we describe how we trained agents for Gran Turismo that can compete with the world’s best e-sports drivers. We combine state-of-the-art, model-free, deep reinforcement learning algorithms with mixed-scenario training to learn an integrated control policy that combines exceptional speed with impressive tactics. In addition, we construct a reward function that enables the agent to be competitive while adhering to racing’s important, but under-specified, sportsmanship rules. We demonstrate the capabilities of our agent, Gran Turismo Sophy, by winning a head-to-head competition against four of the world’s best Gran Turismo drivers. By describing how we trained championship-level racers, we demonstrate the possibilities and challenges of using these techniques to control complex dynamical systems in domains where agents must respect imprecisely defined human norms.

地球科學(xué)Earth Science

Superionic iron alloys and their seismic velocities in Earth’s inner core

超離子鐵合金及其在地球內(nèi)核中得地震速度

▲ 感謝分享：Yu He, Shichuan Sun, Duck Young Kim, Bo Gyu Jang, Heping Li & Ho-kwang Mao

▲ 鏈接：

感謝分享特別nature感謝原創(chuàng)分享者/articles/s41586-021-04361-x

▲ 摘要

地球內(nèi)核（IC）得密度低于純鐵，這表明其內(nèi)部存在輕元素。硅、硫、碳、氧和氫被認(rèn)為是候選元素，人們研究了鐵-輕元素合金得性能以約束IC成分。輕元素對鐵合金得地震速度、熔化溫度和熱導(dǎo)率有很大影響。然而，人們很少考慮IC中輕元素得狀態(tài)。

研究組利用第壹性原理分子動力學(xué)模擬，發(fā)現(xiàn)在IC條件下，六方密排鐵中得氫、氧和碳轉(zhuǎn)變?yōu)槌x子態(tài)，表現(xiàn)出像流體一樣得高擴(kuò)散系數(shù)。這表明IC可以處于超離子態(tài)，而非正常固態(tài)。

流體輕元素導(dǎo)致地震速度大幅降低，接近IC得地震學(xué)觀測值。橫波波速得大幅降低為軟IC提供了一種解釋。此外，輕元素對流對IC地震學(xué)結(jié)構(gòu)和磁場也有潛在影響。

▲ Abstract

Earth’s inner core (IC) is less dense than pure iron, indicating the existence of light elements within it. Silicon, sulfur, carbon, oxygen and hydrogen have been suggested to be the candidates, and the properties of iron–light-element alloys have been studied to constrain the IC composition. Light elements have a substantial influence on the seismic velocities, the melting temperatures and the thermal conductivities of iron alloys. However, the state of the light elements in the IC is rarely considered. Here, using ab initio molecular dynamics simulations, we find that hydrogen, oxygen and carbon in hexagonal close-packed iron transform to a superionic state under the IC conditions, showing high diffusion coefficients like a liquid. This suggests that the IC can be in a superionic state rather than a normal solid state. The liquid-like light elements lead to a substantial reduction in the seismic velocities, which approach the seismological observations of the IC. The substantial decrease in shear-wave velocity provides an explanation for the soft IC. In addition, the light-element convection has a potential influence on the IC seismological structure and magnetic field.