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相关概念视频

Infrared (IR) Spectroscopy: Overview01:09

Infrared (IR) Spectroscopy: Overview

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When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
6.8K
IR Spectrum01:19

IR Spectrum

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When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0%...
3.3K
IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

5.8K
When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
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IR Spectrometers01:25

IR Spectrometers

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There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
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IR Absorption Frequency: Delocalization01:04

IR Absorption Frequency: Delocalization

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Electron delocalization refers to the distribution of electrons across multiple atoms within a molecule rather than being confined to a single atom or bond. This phenomenon is common in systems with conjugated bonds—structures where alternating single and double bonds allow π-electrons to move freely across the network. The movement of electrons stabilizes the molecule and can affect various chemical properties, including vibrational frequencies observed in IR spectroscopy.
In IR...
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IR Frequency Region: Fingerprint Region01:03

IR Frequency Region: Fingerprint Region

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IR spectra are divided into two main regions: the diagnostic region and the fingerprint region. The diagnostic region of the spectrum lies above 1500 cm−1. The absorptions resulting from single-bond vibrations of the N–H, C–H, and O–H stretch at higher wavenumbers and appear on the left side of the spectrum. The stretching absorptions of the C≡C and C≡N occur between 2100–2300 cm−1. In contrast, those arising from stretching absorptions of the...
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相关实验视频

Updated: May 5, 2026

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks
10:31

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks

Published on: May 8, 2015

13.1K

在银河系中心区域的红外扩散星际波段.

T R Geballe1, F Najarro, D F Figer

  • 1Gemini Observatory, 670 N. A'ohoku Place, Hilo, Hawaii 96720, USA. tgeballe@gemini.edu

Nature
|November 4, 2011
PubMed
概括

研究人员在银河系中心发现了13个新的分散星际波段 (DIB). 这些宇宙吸收特征,可能是基于碳的分子,出现在比以前观察到的DIB更恶劣的环境中.

科学领域:

  • 天文学 天文学
  • 天体物理学 天体物理学
  • 频谱学是一种光谱学.

背景情况:

  • 分散星际带 (DIBs) 是由于星际物质而在恒星光谱中观察到的吸收特征.
  • 已知有500多个DIB,主要是在可见和近红外波长.
  • 怀疑DIBs的载体是多原子含碳分子,但没有一个被确定的.

研究的目的:

  • 在更长的红外波长 (1.5-1.8微米) 中寻找和描述新的DIB.
  • 调查这些新发现的DIBs的起源和环境.
  • 将银河系中心的DIB属性与其他扩散云的DIB属性进行比较.

主要方法:

  • 高分辨率的光谱观测恒星的高灭绝向银河系中心.
  • 在1.5-1.8微米波长区间分析光谱.
  • 将DIB强度与星际灭绝值进行比较.

主要成果:

  • 在1.5-1.8微米范围内发现了13个新的扩散星际带.
  • 这些DIB主要观察到银河系中心,这表明它们起源于该地区.
  • 这些DIB的相对强度与星际灭绝相关,类似于以前已知的DIB.

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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

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Last Updated: May 5, 2026

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks
10:31

Diffuse Reflectance Infrared Spectroscopic Identification of Dispersant/Particle Bonding Mechanisms in Functional Inks

Published on: May 8, 2015

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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies
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Characterizing Far-infrared Laser Emissions and the Measurement of Their Frequencies

Published on: December 18, 2015

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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F&#8722;
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Photoelectron Imaging of Anions Illustrated by 310 Nm Detachment of F−

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结论:

  • 银河系中心拥有以前未知的分散星际波段,起源于一个更温暖,更恶劣的环境.
  • 这些新的DIB的载体可能与已知DIB的载体相似,可能是多原子碳分子.
  • DIB强度通常随着分散的星际物质的数量而变大,无论具体的环境如何.