Name: how heat changes atomic spectra
Uploaded: 2024-12-05T18:32:14.000Z
Duration: 1 min 27 s
Channel: JoVE

Ricordiamo che l'atomizzazione, o la scomposizione di campioni liquidi in atomi in fase gassosa, è cruciale nella spettroscopia atomica.
L'efficienza di atomizzazione aumenta con la temperatura. Inoltre, la temperatura influisce sulla proporzione di atomi in stato eccitato o ionizzato, influenzando la potenza del segnale.
L'entità dell'effetto della temperatura è stimata dall'espressione di Maxwell-Boltzmann, che descrive le popolazioni relative degli stati fondamentali ed eccitati all'equilibrio termico.
A 2500 K, quasi lo 0,017% degli atomi di sodio sono eccitati. Con un aumento della temperatura di 100 K, la popolazione dello stato eccitato relativo aumenta del 45%, ma diminuisce la popolazione dello stato fondamentale in modo trascurabile.
Poiché il processo di rilassamento dello stato eccitato provoca l'emissione di luce, il controllo della temperatura è fondamentale nell'AES per un'intensità di emissione costante.
Al contrario, le intensità di AAS e AFS dipendono dalle popolazioni dello stato fondamentale.
Tuttavia, le variazioni di temperatura influenzano la popolazione totale nel suo complesso e l'alta temperatura provoca interferenze di ionizzazione, entrambe le quali influenzano l'intensità spettrale.
Inoltre, tutta la spettroscopia atomica ad alta temperatura mostra un effetto Doppler più pronunciato, con allargamento della linea spettrale e riduzione dell'altezza del picco.

spettroscopia atomica: effetti della temperatura

Atomic Spectroscopy: Effects of Temperature

L'atomizzazione, ovvero la conversione dei campioni in atomi e ioni in fase gassosa, è essenziale per la spettroscopia atomica. La temperatura della fiamma richiesta per l'atomizzazione influisce sull'efficienza dei metodi di spettroscopia atomica aumentando l'efficienza di atomizzazione e la popolazione relativa degli stati eccitati e fondamentali.

All'equilibrio termico, le popolazioni relative degli atomi eccitati e fondamentali, possono essere stimate utilizzando la distribuzione di Maxwell-Boltzmann. Per esempio, un aumento della temperatura da 2500 K a 2600 K può far aumentare la popolazione degli atomi di sodio allo stato eccitato del 45%, mentre la diminuzione della popolazione allo stato fondamentale è trascurabile. Siccome la spettroscopia di emissione atomica (AES) si basa sull'emissione di fotoni da questi stati eccitati, è altamente dipendente dalla temperatura. Al contrario, la spettroscopia di assorbimento atomico (AAS) e la spettroscopia di fluorescenza atomica (AFS) dipendono principalmente dalla popolazione dello stato fondamentale e hanno una dipendenza dalla temperatura meno significativa. Tuttavia, per gli elementi facilmente ionizzabili, un aumento della temperatura della fiamma provoca una perdita di atomi per ionizzazione, influenzando negativamente l'assorbimento e l'intensità spettrale della fluorescenza.

Inoltre, nella spettroscopia atomica in generale, una temperatura più elevata aumenta la velocità degli atomi, rendendo l'effetto Doppler più pronunciato. Questo determina l'ampliamento delle linee spettrali atomiche e la diminuzione dell'altezza del picco.

Spettroscopia atomica: effetti della temperatura

L'atomizzazione, che converte i campioni in atomi e ioni in fase gassosa, è essenziale per la spettroscopia atomica. La temperatura della fiamma richiesta per l'atomizzazione ...

atomic-spectroscopy-effects-of-temperature

Education

Didattica

JoVE Core

Analytical Chemistry

Chimica Analitica

Unit 1

Unità 1

Atomic Spectroscopy

Spettroscopia atomica

KEY TERMS AND CONCEPTS

TERMINI E CONCETTI CHIAVE

how heat changes atomic spectra

Heat changes atomic spectra by affecting atomization, excitation, ionization, and line shape. In atomic spectroscopy, atomization means converting a sample into gas-phase atoms and ions. The flame temperature needed for this step changes how efficiently the method works and shifts the balance between excited and ground-state atoms.

At thermal equilibrium, the relative numbers of excited and ground-state atoms can be estimated with the Maxwell-Boltzmann distribution. A small temperature rise can make a big difference. For example, increasing the temperature from 2500 K to 2600 K can raise the number of excited-state sodium atoms by 45%, while the decrease in ground-state atoms is negligible.

This temperature effect matters most for atomic emission spectroscopy, or AES, because it depends on photons emitted from excited atoms. Atomic absorption spectroscopy, or AAS, and atomic fluorescence spectroscopy, or AFS, mainly depend on ground-state atoms, so their temperature dependence is less significant. However, for easily ionizable elements, higher flame temperature can remove atoms by ionization and reduce absorption and fluorescence signal intensity.

Higher temperature also makes atoms move faster. This increases the Doppler effect, which broadens atomic spectral lines and lowers peak height. As a result, temperature can shape both the strength and the width of atomic signals.

How Heat Changes Atomic Spectra

atomic spectroscopy: absorption, emission, and fluorescence

atomic-spectroscopy-absorption-emission-and-fluorescence

Element Analysis with Atomic Light Spectra

Atomic spectroscopy is used to identify and measure elements by their light signals. It supports both qualitative analysis, which tells what is present, and quantitative analysis, which tells how much is present. The optical methods in this group are atomic absorption spectroscopy, atomic emission spectroscopy, and atomic fluorescence spectroscopy. These methods begin with atomization. In this step, a solid, liquid, or solution sample is changed into gas-phase atoms and ions. Once the sample...

atomic spectroscopy: effects of temperature

Heat changes atomic spectra by affecting atomization, excitation, ionization, and line shape. In atomic spectroscopy, atomization means converting a sample into gas-phase atoms and ions. The flame temperature needed for this step changes how efficiently the method works and shifts the balance between excited and ground-state atoms. At thermal equilibrium, the relative numbers of excited and ground-state atoms can be estimated with the Maxwell-Boltzmann distribution. A small temperature rise...

atomic absorption spectroscopy: overview

Atomic Absorption Spectroscopy for Trace Metals

Atomic absorption spectroscopy (AAS) measures trace metals by tracking how atoms absorb electromagnetic radiation (EMR). The absorbed light makes atoms move to a higher-energy orbit. In AAS, the key step is atomization, which converts the sample into gas-phase atoms. A flame or a furnace is typically used for this step. Inside the flame, some atoms become thermally excited. Most stay in the ground state, which is the lowest-energy state. These ground-state gas-phase atoms absorb EMR only when...

atomic absorption spectroscopy: instrumentation

atomic-absorption-spectroscopy-instrumentation

Atomic Absorption Spectroscopy: Key Parts

Atomic absorption spectrophotometry uses a set of key parts to measure light absorbed by atoms. The main components are a radiation source, an atomizer, a monochromator, and a detector. Each part has a specific job in the instrument. The radiation source is usually a hollow-cathode lamp, or HCL, or an electrodeless-discharge lamp, or EDL. Both produce a narrow emission line at the needed wavelength. Some instruments instead use continuum sources with high-resolution monochromators to narrow...

atomic absorption spectroscopy: radiation and light sources

atomic-absorption-spectroscopy-radiation-and-light-sources

Choosing Light Sources for AAS Measurements

Atomic absorption spectroscopy (AAS) uses a light source that emits a very narrow range of wavelengths. This is needed because the source must match the absorption behavior of the analyte atom. The choice of source also depends on giving a precise, intense emission at the right wavelength for accurate detection. Two common line sources in AAS are hollow-cathode lamps (HCLs) and electrodeless-discharge lamps (EDLs). These lamps are selected based on the element being analyzed and the level of...

atomic absorption spectroscopy: atomization methods

atomic-absorption-spectroscopy-atomization-methods

Atomic Absorption Spectroscopy: Sample Atomization

Atomic absorption spectroscopy uses sample atomization to turn a liquid specimen into free atoms for analysis. The two main approaches are flame atomization and electrothermal atomization. Both methods prepare the sample so its atoms can be measured by the instrument. Flame atomization uses a nebulizer and spray chamber to mix the sample with a fuel-oxidant mixture. This creates a fine aerosol mist that enters the burner. The fuel and oxidant are usually close to a stoichiometric ratio, but a...

atomic absorption spectroscopy: interference

atomic-absorption-spectroscopy-interference

Correcting Errors in Atomic Absorption Spectroscopy

Atomic absorption spectroscopy interference can create systematic error by making the analytical signal or the background look stronger or weaker than it should be. In atomic absorption measurements, these errors are usually grouped as spectral interference, chemical interference, and physical interference. Spectral interference happens when signals from other elements or molecules overlap with the analyte signal, the substance being measured. This overlap can falsely raise or hide the analyte...

atomic absorption spectroscopy: lab

AAS Sample Prep and Calibration

Atomic absorption spectroscopy (AAS) depends on careful sample preparation and calibration. Samples must be turned into clear solutions before measurement. That often means extra treatment to dissolve materials such as soils, animal tissues, and minerals. Common sample prep methods include hot mineral acids, wet ashing, combustion in closed containers, high-temperature ashing, and fusion with reagents. These steps help make the sample suitable for AAS analysis. Solutions that contain organic...

atomic emission spectroscopy: overview

Atomic Emission Spectroscopy for Element Analysis

Atomic emission spectroscopy is used to identify the elements in a sample by measuring the light they emit. Atoms are first excited to higher energy levels by thermal energy from hot sources such as plasma, arcs, or sparks. When they fall back to lower energy levels, they give off light at specific wavelengths. Each element produces its own set of lines, so the emission spectrum can show both what is present and how much is there. AES instruments are similar to atomic absorption spectrometers,...

atomic emission spectroscopy: instrumentation

atomic-emission-spectroscopy-instrumentation

AES Sample Handling and Detection

Atomic emission spectrometry (AES) uses sample handling, atomization, and detection parts to measure emitted light from atoms and ions. The sample must first be changed into a gas-phase form so it can produce a measurable signal. AES uses two main atomizer types. Continuous atomizers, such as flames and plasmas, feed the sample in a steady stream. Discrete atomizers add one sample at a time with syringes or autosamplers. The electrothermal atomizer is the most common discrete type. Many...

atomic emission spectroscopy: interference

atomic-emission-spectroscopy-interference

Reducing Interference in AES Signals

Atomic emission spectroscopy (AES) can produce interfering signals when atoms and molecules in a flame or plasma emit overlapping light. High-temperature atomizers excite many species at once, including oxides, hydroxides, and flame combustion products. These extra emissions can make the analyte signal harder to read. Spectral interference happens when emission lines or bands overlap. One way to reduce it is to improve instrument resolution. Another is to choose a different emission line for...

inductively coupled plasma atomic emission spectroscopy: principle

inductively-coupled-plasma-atomic-emission-spectroscopy-principle

ICP-AES Torch and Sample Analysis

Inductively coupled plasma atomic emission spectroscopy uses a plasma torch to analyze elements in a sample. This method is also called inductively coupled plasma optical emission spectroscopy, or ICP-OES. It is widely used because the plasma creates a strong environment for elemental analysis. The ICP source, or torch, contains three concentric quartz tubes. Argon gas flows through the tubes. A spark from a Tesla coil starts the ionization of argon and creates a high-temperature plasma. The...

inductively coupled plasma atomic emission spectroscopy: instrumentation

inductively-coupled-plasma-atomic-emission-spectroscopy

ICP-AES Instrument Types and Detection

Inductively coupled plasma atomic emission spectroscopy, or ICP-AES, uses an inductively coupled plasma to detect and analyze elements in a sample. The method measures the light given off by atoms, which helps identify and compare different elements. It is a common approach in atomic emission spectroscopy. ICP-AES instruments are built in three main forms: sequential, simultaneous multichannel, and Fourier transform instruments. Fourier transform designs are less commonly used, but they are...

atomic emission spectroscopy: lab

Plasma Sources in Atomic Emission Spectroscopy

Atomic emission spectroscopy uses plasma sources to identify elements by their light. The method creates abundant spectra with characteristic emission lines. Inductively coupled plasma, or ICP, is especially useful because it gives strong quantitative data. It works well under stable conditions, with low noise, low background, and few interferences. Newer air-operated microwave sources are also being studied. These sources may be more cost-effective than conventional ICP systems. Atomic...

atomic fluorescence spectroscopy

Measuring Elements by Atomic Fluorescence

Atomic fluorescence spectroscopy measures elements by detecting the light atoms give off after they are excited by electromagnetic radiation. The atoms are first placed in a flame, furnace, or plasma. They absorb energy, become excited, and then release that energy as they return to their original state. The emitted light is called fluorescence. The fluorescence is observed at a right angle to the incoming beam. This setup helps separate the emitted light from the light used to excite the...

flame photometry: overview

Flame Emission Spectrometry Basics

Flame emission spectrometry uses a flame to excite elements in a sample so their light can be measured. It is also called flame photometry. The method can be used for both qualitative and quantitative analysis of elements. The idea became established in the early 1860s when Kirchhoff and Bunsen showed that specific elements give off characteristic radiation in a flame. The first instrument for this purpose measured sodium in plant ash with a Bunsen flame. A major problem was how to add the...

flame photometry: lab

Flame Photometry and Metal Detection

Flame photometry is a method for detecting metals by measuring the light they emit in a flame. A solution such as potassium chloride is aspirated into the flame. The solvent evaporates first. The remaining salt becomes dehydrated and then dissociates into free gaseous atoms in the ground state. Some of these atoms absorb energy from the flame and move to an excited state. When they return to the ground state, they emit photons at characteristic wavelengths. These emissions are very narrow...

key terms and concepts

Learn how flame temperature affects atomization, excited and ground-state atoms, ionization, and Doppler broadening in atomic spectroscopy.

How Heat Changes Atomic Spectra | JoVE K12

analytical chemistry

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How Heat Changes Atomic Spectra

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