Garantie de satisfaction à 100% Disponible immédiatement après paiement En ligne et en PDF Tu n'es attaché à rien 4,6 TrustPilot
logo-home
Notes de cours

Chemistry for Biology Students (CHEM0010) Notes - Spectroscopy

Note
-
Vendu
-
Pages
17
Publié le
30-11-2023
Écrit en
2020/2021

Explore Chemistry for Biology Students with these specialized notes tailored for Year 1 students at University College London. Immerse yourself in the fascinating world of spectroscopy, where discussions unfold on the properties of light, UV-visible light, and the principles of infrared and NMR spectroscopy. Please note that these materials are intended for personal use only and should be used in accordance with academic integrity guidelines.

Montrer plus Lire moins
Établissement
Cours

Aperçu du contenu

B1: Light and its Properties
B1: Light and its Properties
 Light
o Eye

Light from external source

Focused by a lens

Image is formed by a set of detector molecules in the retina

Light falls on the molecules – sends an electrical signal to the brain
 Retina – contains light sensing molecules
o Rods – light and dark detection
o Cones – photo-rhodopsin molecules – respond to different wavelengths of
light – detects colour
 Range of colours detected – depends on number and type of photo-
rhodopsin molecules in our eyes
o EM wave
 James Clerk Maxwell – made a set of wave equations = formed the basis of the
electromagnetic theory of light
 Electricity and magnetism – linked together involving time
 Electric fluctuations described by the electric field strength (E) + magnetic
fluctuations described by the magnetic field intensity (B or H) travelled through
space in unison at constant speed (c)
o Constant (c) = 3x108 m/s





 Light waves – also defined by wavelength in metres (λ), frequency in Hz (v)
o c = λv (speed of light = wavelength x frequency)
o Colour
 Refractive index n = c/v
 Light in a vacuum – all different coloured beams travel at the same speed (c)
 Light in a material – slowed down due to interactions with electrons and atomic
nuclei to slower speed (ν)
 Prism – refracts light
 White light – contains all colours
o Light with different colours (different wavelengths) – slowed down by
different amounts
 When a light beam strikes an inclined surface – beams are bent by
different amounts to travel through the prism with different paths
 Newton’s prism experiment
o Mounted a prism with the point downwards
o Had a darkened room with a curtain
o Cut a hole to let a beam of light through
o Directed light through the lens
o Observed the colours of the rainbow
 Split light into different coloured components
 Purple appeared at the top (shortest wavelength)
 Red appeared at the bottom (longest wavelength)
 Absorbance = 2 – log(%T)
 Visible spectrum of light

,B1: Light and its Properties
 Colours of a
rainbow
o




Relationship between wavelength, frequency and speed of light is given by:
 c = λv
 c stays constant
 As λ changes, v changes in the opposite direction
 Wavenumber = 1 / wavelength
o Colours = different wavelengths and frequencies
 Full electromagnetic spectrum
o Contains all wavelengths / frequencies of light that
satisfy c = λv
 Spectroscopy – light can be used in
different regions to interact with different
atomic and molecular properties – to gain
information about them
 Ultraviolet-visible
o Electron transitions between quantized energy levels in atoms and
molecules – to study bonding
 Infrared spectroscopy
o Vibrations between atoms in molecules – to study molecular structure and
functional groups
 Nuclear magnetic resonance (radio waves)
o Study spin flips of atomic nuclei in magnetic fields and gain information
about local structural environments
 Light as a particle and a wave
o 2 models
 Light as a wave – properties of wavelength and frequency
 Light as a particle = photon – properties of mass and momentum
o Wave-particle duality
 Brought 2 models together
 Each photon associated with a pilot wave
 Equation – λ = h/mv
 h = Planck’s constant = 6.626 x 10 -34 J/s
 m = mass of particle
 mv = momentum (mass x velocity)
o Planck’s equation – energy of a single photon
 E = hv = (hc)/λ
 Energy of a photon = Planck’s constant x frequency = (Planck’s constant x speed of light) /
wavelength
 High energy radiation – has high frequency and short wavelength
 Low energy radiation – has low frequency and long wavelength
 Units
o h = Planck’s constant = 6.626 x 10 -34 J/s
o m = mass of particle
o mv = momentum (mass x velocity)

, B1: Light and its Properties
o λ = wavelength in metres (m)
o v = frequency in s
o c = speed of light in metres per second (m/s)
o E = energy of a photon in Joules (eV)
o 1nm = 10-9m

Ideas in Bonding
 Atomic energy levels and transitions between them
o Atoms
 Electrons orbit around the nucleus
 Energies and shapes of orbitals – defined by 4 quantum numbers
o Quantized electron energy (E) – related to the radius of the orbit = principle
quantum number (n)
o Electrons can jump to a
higher energy orbit by
absorbing light in the UV to
visible range
 Energy jump (ΔE) –
related to frequency (λ) or wavelength (v) of light absorbed by
Planck’s equation
 ΔE = hv = (hc)/ λ
 Shapes of Atomic Orbitals (p vs s orbitals)
o Consider shapes of orbitals when combined to form MOs
 Orbitals are quantized according to their angular momentum + labelled s, p, d, etc
 2s orbitals = spherical
 2p orbitals = have + and – lobes that point along the x-, y-, or z- axes = p x, py, pz
o Carbon
 Uses 2px, 2py, 2pz orbitals to make C-C bonds
 Uses 1s orbitals of H for C-H bonds
 Bonding vs Antibonding orbitals and energy levels
o Molecular orbitals – formed by the overlap of atomic orbitals
 Lower energy compared with the starting atomic orbitals = bonding orbital
 Formed by positive overlap between orbitals = constructive
 Higher energy compared with the starting atomic orbitals = antibonding orbital (no electron
density between 2 atoms)
 Formed by negative overlap between orbitals = destructive
 Hybrid orbitals and bonding
o Carbon atoms use combinations of 2s and 2p orbitals = form hybridised orbitals
 Hybrid orbitals = mathematic combinations of wavefunctions for 2s and 2p orbitals
o 3 possibilities for making spn orbitals
 s + px + py + pz = 4 sp3
 New hybridised orbitals have 4 lobed that point towards the corners of a
tetrahedron
 Each hybridised orbital can bond with 1s of H atoms or combine with sp 3 hybrids on
other C atoms
o Forming double and triple bonds
 sp2 orbitals
 s + px + py = sp2
 Double bond
 Sigma bond – sp2 + sp2
 Pi bond – pz + pz

École, étude et sujet

Établissement
Cours
Inconnu
Cours

Infos sur le Document

Publié le
30 novembre 2023
Nombre de pages
17
Écrit en
2020/2021
Type
Notes de cours
Professeur(s)
Professor andrea sella
Contient
Toutes les classes

Sujets

$9.56
Accéder à l'intégralité du document:

Garantie de satisfaction à 100%
Disponible immédiatement après paiement
En ligne et en PDF
Tu n'es attaché à rien

Faites connaissance avec le vendeur
Seller avatar
sujansathiendran
5.0
(1)

Document également disponible en groupe

Faites connaissance avec le vendeur

Seller avatar
sujansathiendran University College London
S'abonner Vous devez être connecté afin de suivre les étudiants ou les cours
Vendu
5
Membre depuis
4 année
Nombre de followers
5
Documents
42
Dernière vente
1 année de cela

5.0

1 revues

5
1
4
0
3
0
2
0
1
0

Documents populaires

Récemment consulté par vous

Pourquoi les étudiants choisissent Stuvia

Créé par d'autres étudiants, vérifié par les avis

Une qualité sur laquelle compter : rédigé par des étudiants qui ont réussi et évalué par d'autres qui ont utilisé ce document.

Le document ne convient pas ? Choisis un autre document

Aucun souci ! Tu peux sélectionner directement un autre document qui correspond mieux à ce que tu cherches.

Paye comme tu veux, apprends aussitôt

Aucun abonnement, aucun engagement. Paye selon tes habitudes par carte de crédit et télécharge ton document PDF instantanément.

Student with book image

“Acheté, téléchargé et réussi. C'est aussi simple que ça.”

Alisha Student

Foire aux questions