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相关论文: The SiC problem: astronomical and meteoritic evide…

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We present new multielement NanoSIMS isotopic measurements (C, N, Si, Mg-Al, Ti, and Ni) for four putative nova SiC grains and 79 AB SiC grains from the Murchison meteorite to reassess their stellar origins. High-resolution imaging and a…

太阳与恒星天体物理 · 物理学 2026-05-20 Jordi José , Nan Liu , Conel M. O'D. Alexander , Jianhua Wang

The Visible-Infrared Mapping Spectrometer (VIR) on board the Dawn spacecraft revealed that aqueous secondary minerals -- Mg-phyllosilicates, NH4-bearing phases, and Mg/Ca carbonates -- are ubiquitous on Ceres. Ceres' low reflectance…

地球与行星天体物理 · 物理学 2020-11-03 H. Kurokawa , B. L. Ehlmann , M. C. De Sanctis , M. G. A. Lapôtre , T. Usui , N. T. Stein , T. H. Prettyman , A. Raponi , M. Ciarniello

The Cosmic Infrared Background (CIB) traces the emission of star-forming galaxies throughout all cosmic epochs. Breaking down the contribution from galaxies at different redshifts to the observed CIB maps would allow us to probe the history…

星系天体物理 · 物理学 2023-02-01 Baptiste Jego , Jaime Ruiz-Zapatero , Carlos García-García , Nick Koukoufilippas , David Alonso

The mysterious 21mu emission feature seen in 12 proto-planetary nebulae (PPNe) remains unidentified since its first detection in 1989. Over a dozen of candidate materials have been proposed within the past decade, but none of them has…

天体物理学 · 物理学 2009-11-13 B. W. Jiang , Ke Zhang , Aigen Li

Titanium carbide (TiC) nanocrystals were recently proposed as the carrier of the mysterious 21$\mum$ emission feature observed in post-asymptotic giant branch stars, based on their close spectral match and the presolar nature of meteoritic…

天体物理学 · 物理学 2009-11-10 Aigen Li

We report on the microscopic surface structure of carbon-fiber-reinforced silicon carbide (C/SiC) composite mirrors that have been improved for the Space Infrared Telescope for Cosmology and Astrophysics (SPICA) and other cooled telescopes.…

天体物理学 · 物理学 2009-06-23 Keigo Enya , Takao Nakagawa , Hidehiro Kaneda , Takashi Onaka , Tuyoshi Ozaki , Masami Kume

Textured silicon surface structures, in particular black silicon (b-Si), open up possibilities for Si-based solar cells and photodetectors to be extremely thin and highly sensitive owing to perfect light-trapping and anti-reflection…

The unique quantum properties of the nitrogen-vacancy (NV) center in diamond have motivated efforts to find defects with similar properties in silicon carbide (SiC), which can extend the functionality of such systems not available to the…

The outstanding demonstration of quantum confinement in Si nanocrystals (Si NC) in a SiC matrix requires the fabrication of Si NC with a narrow size distribution. It is understood without controversy that this fabrication is a difficult…

应用物理 · 物理学 2020-05-18 C. Weiss , M. Schnabel , A. Reichert , P. Löper , S. Janz

Gravitational lensing deflects the paths of cosmic infrared background (CIB) photons, leaving a measurable imprint on CIB maps. The resulting statistical anisotropy can be used to reconstruct the matter distribution out to the redshifts of…

宇宙学与河外天体物理 · 物理学 2018-07-04 Emmanuel Schaan , Simone Ferraro , David N. Spergel

A new classification system for carbon-rich stars is presented based on an analysis of 51 AGB carbon stars through the most relevant classifying indices available. The extension incorporated, that also represents the major advantage of this…

Infra-red maps and profiles with high spatial resolution were obtained for two single crystal diamonds with pronounced CO2 IR absorption peaks. Detailed examination allows unambiguous assignment of the spectral features to solid CO2-I…

材料科学 · 物理学 2021-02-16 Evgenii P. Barannik , Andrey A. Shiryaev , Thomas Hainschwang

The dependence of stellar molecular bands on the metallicity is studied using infrared L-band spectra of AGB stars (both carbon-rich and oxygen-rich) and M-type supergiants in the Large and Small Magellanic Clouds (LMC and SMC) and in the…

The cosmic infrared background (CIB) traces star-forming galaxies throughout cosmic history, with emission peaking at $z\sim1-2$. CIB anisotropies are present at the far-infrared frequencies observed by cosmic microwave background (CMB)…

宇宙学与河外天体物理 · 物理学 2024-05-24 Fiona McCarthy

Meteorite matrices from primitive chondrites are an interplay of ingredients at the sub-micron scale, which requires analytical techniques with the nanometer spatial resolution to decipher the composition of individual components in their…

地球与行星天体物理 · 物理学 2022-06-22 Van T. H. Phan , Rolando Rebois , Pierre Beck , Eric Quirico , Lydie Bonal , Takaaki Noguchi

Using a full analytical computation of the bispectrum based on the halo model together with the halo occupation number, we derive the bispectrum of the cos- mic infrared background (CIB) anisotropies that trace the clustering of dusty-star-…

宇宙学与河外天体物理 · 物理学 2014-03-05 Aurélie Pénin , Fabien Lacasa , Nabila Aghanim

Peculiarities of formation of inclusions of amorphous Si (a-Si) phase in Si-rich Si oxynitride films grown by plasma-enhanced chemical vapor deposition (PECVD) are studied by combined Raman scattering and infrared (IR) absorption…

材料科学 · 物理学 2026-01-21 M. V. Voitovych , A. Sarikov , V. O. Yukhymchuk , V. V. Voitovych , M. O. Semenenko

The naturally occurring radioisotope $^{32}$Si represents a potentially limiting background in future dark matter direct-detection experiments. We investigate sources of $^{32}$Si and the vectors by which it comes to reside in silicon…

仪器与探测器 · 物理学 2018-02-20 J. L. Orrell , I. J. Arnquist , M. Bliss , R. Bunker , Z. S. Finch

Laboratory analyses on fine-grained diamond residues from primitive meteorites have shown that nano-diamonds represent the most abundant form of presolar dust preserved in meteoritic samples. The presolar diamonds carry isotopic anomalies…

天体物理学 · 物理学 2007-05-23 A. C. Andersen , U. G. Jorgensen , F. M. Nicolaisen , P. G. Sorensen , K. Glejbol

We present the design, fabrication, and characterization of high quality factor and small mode volume planar photonic crystal cavities from cubic (3C) thin films (thickness ~ 200 nm) of silicon carbide (SiC) grown epitaxially on a silicon…