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The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

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Page 1: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

The flames of Romance

Candlelight and Chemistry

Molecular spectroscopy and reaction dynamics

Arnar HafliðasonApril 10th 2015

Page 2: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

The beauty of science

• Lets begin with Richard Feynman

• The story about the flower and his artist friend

Page 3: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

You, light up my life

• What is a candle made of..?

• What is needed for it to burn..?

• What is, “to burn”..?

• Why is fire, yellow.. Why is fire, blue?

• Let’s gaze into the flames and see what’s cookin’?

Page 4: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

What is candle made of?

• Paraffin wax C31H64 • Or actually a mixture of long hydro-

carbon molecules, i.e. CnH2n+2, ranging from n=25-40.

• Paraffin wax is a white or colorless soft solid derivable from petroleum

• Candle wick, a braided cotton that holds the flame of a candle

Page 5: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

What is needed for it to burn? • Prerequisite is OXYGEN

• Oxygen around is usually enough, though you might want to add more oxygen to spice things up

• You need the “spark” for the chemistry to happen

• The process needs to be exothermic to sustain itself

• The rate of the chemical reactions needs to be fast enough to keep the process going

• Some source of hydrocarbons (gas, wax) for the oxygen to react with

Page 6: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

What is, “to burn”?

• When the hydrocarbons start “to burn”, a chemical reaction occurs. The light that we see emitted is caused by the reaction of hydrocarbons with oxygen, a rapid oxidation process, also know as combustion:

+ Energy

Exothermic Reaction Energy

Page 7: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Energy from exothermic reaction

Divided into 2 main groups

1. Kinetic Energy (Vibration, Rotation, translation)• Ekin = nkBT (Increase in temperature => more energy)HEAT

2. Radiation Energy (emission following e- transfer)• E = h n = h(c/ )l (shorter wavelength => more energy)LIGHT

Page 8: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

What is, “to burn”?

• When the hydrocarbons start “to burn”, a chemical reaction occurs. The light that we see emitted is caused by the reaction of hydrocarbons with oxygen, a rapid oxidation process, usually called combustion:

+ Energy

Exothermic Reaction

→(…+𝑪𝑯+𝑶𝑯+𝑪𝟐+…)→?????

Could this explain the different colors in the fire??

Energy

Reactive radicals are formed

Page 9: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Why is fire, yellow.. Why is fire, blue?

… it depends on what you’re burning … and what the heat is when it’s burning

Page 10: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

1) Just gas, no extra oxygen (candle)

2) Gas, and little bit of oxygen

3) Gas, and oxygen

4) Gas, and a lot of oxygen

Lets connect a gas-burner: propane gas cylinder and oxygen cylinder

Page 11: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Heat from steps 1) – 4) estimated around 1000 K – 3000 K.

1) Yellow because of incomplete com-bustion caused by lack of oxygen. What we see as yellow/white is soot (Cn(s)) that is glowing

Less combustion – Less heat – less blue

Propane/Oxygen

4) Blue because of “complete” combustion caused by abundance of oxygen. Notice the flame is almost clear above the blue inner core

More combustion – More heat – more blue

Page 12: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Gaze into the flames and see what’s cookin’

• Monochromator• separates light

into wavelengths

Page 13: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Experimental setup

/Mono-chromator /

gas burner

/PMT/inlet slit

Page 14: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Diffraction grating Source about 4 cm from slit

Opening is 5x5 mm

Slit settings: 10, 30 and 50 μm

Page 15: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Measured emission spectra

Page 16: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Radicals and radiation

• C2 and OH radicals• Emission at 516 nm, the C2 radical is in

excited electronic state, it relaxes to a lower energy state, d3Π → a3Π, giving of radiation equal to that energy-difference

• Emission at 308.6 nm, the OH radical is in excited state and is relaxed to the ground state, A2Σ+ → X2Π, giving of radiation equal to that energy-difference

Page 17: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Radicals and radiation

• CH radicals• Emission at 430.7 nm, the CH radical is in

excited electronic state and relaxes to the ground state, A2Δ → X2Π, giving of radiation equal to that energy-difference

• Emission at 389.1 nm, transition: B2Σ- → X2Π• Emission at 314.7 nm, transition: C2Σ+ → X2Π

Page 18: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

A = 430.7 nm

What do I mean by “energy-difference”?

h = 430.7 nm

𝐸=h𝜈=h𝑐𝜆

h: Planck constantc: speed of light constant: wavelength of light

CH

Potential curves for the CH molecule

B = 389.1 nm

C = 314.7 nm

= 389.1 nm = 314.7 nm

Page 19: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Radicals and radiation

• Emission observed is found at: 314.7, 389.1 and 430.7 nm for CH, 308.6 for OH and 516 nm for C2

Human color vision

Page 20: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Measured emission spectra

Page 21: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Vibrational and rotational structure

v’’

01

23

4

01

23

v’A2Δ

X2Π

Measurement

Page 22: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Location of vibrational bands

nm

Measured Calculated

Total

v’=3v’’=3

v’=2v’’=2

v’=0v’’=0

v’=1v’’=1

Page 23: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Rotational structure for v’=0v’’=0 transition.

4 68

10

14J’=20

Measurement

Page 24: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Spectral simulation at T=3000K

Simulation with PGOPHER

MeasurementSimulation

Lambda doubling

e-

Page 25: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Simulation on A2Δ → X2Π for v‘=0 → v‘‘=0

• B’’=14.17• A’’=29.75• D’’=0.00142

• B’=14.56• A’=-1.1• D’=0.00152

• B’’=14.19• A’’=27.95• D’’=0.00148

• B’=14.57• A’=-1.1• D’=0.00146

Calculated Constants from NISTMinimal adjustment of constants from NIST (National Institute of Standards and Technology).

B: Rotational constantD: Centrifugal distortionA: Spin-orbit coupling

cm-1

X2Π

A2Δ

Page 26: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Few measurements under different circumstances

1. Different quantity of oxygen burned with propane gas, 5 different settings

2. 6 different height settings of the slit from the source of the flame

Page 27: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

3 cm3 mm

Slit

Page 28: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

2x O2

1900 K

4x O2

3000 K3x O2

2200 K

Difference in rotational distribution. More heat is observed with increase in use of oxygen.

Simulations:

Page 29: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Comparing population distribution. Experiment vs. Boltzmann distribution

J=7

J=6

T = 2200 K Jmax = 6.74

Page 30: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

3x O2

0 mm

50 mm

15 mm

Page 31: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

3x O2

0 mm

50 mm

15 mm

Page 32: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015
Page 33: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Thank you all for coming

Page 34: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Some equations

𝐽𝑚𝑎𝑥=12 √ 2𝑘𝑇

h𝐵 𝑐−

12

𝑛 𝐽

𝑁=(2 𝐽+1)𝑒

(−𝐵𝐽 ( 𝐽 +1)h𝑐𝑘𝑇 )

Boltzmann distributionHönl-London factors

Page 35: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Frank-Condon factors. Can calculate transition probability between vibrational states v’ and v’’

v’’

v’

0

01

12

23

34

4

Page 36: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

Voltage and slit

• Intensity for different settings was measured

10 15 20 25 30

0.4

0.5

0.6

0.7

0.8

0.9

1

micrometer

Inte

nsity

Change of slit opening

y = 0.033*x + 0.0033

Slit change

Fitting

900 920 940 960 980 1000

0.4

0.5

0.6

0.7

0.8

0.9

1Voltage change

Voltage

Inte

nsity

y = 0.0064*x - 5.4

Change in voltage

linear fitting

Slit settings: 10, 30 and 50 μm

Voltage settings: 900 and 1000 V

Page 37: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015

156 cm-1

Page 38: The flames of Romance The flames of Romance Candlelight and Chemistry Molecular spectroscopy and reaction dynamics Arnar Hafliðason April 10 th 2015