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Transcript of Di erential Scanning Calorimetry - basvangestel.nl · Di erential Scanning Calorimetry (DSC) is an...
Differential Scanning
Calorimetry
Literature study Solid State Chemistry
Bas van Gestel
July 7, 2007 – December 18, 2007
Solid State Chemistry,
Institute for Molecules and Materials,
Radboud University Nijmegen
2
Contents
1 Introduction 5
2 Introduction to calorimetry 7
2.1 The Four Elements . . . . . . . . . . . . . . . . . . . . . . . . 7
2.2 Internal Energy and Heat . . . . . . . . . . . . . . . . . . . . 8
2.3 Temperature and temperature scales . . . . . . . . . . . . . . 10
2.3.1 Physiological temperature scale . . . . . . . . . . . . . 11
2.3.2 Liquid in glass . . . . . . . . . . . . . . . . . . . . . . . 11
2.3.3 Resistance Thermometers . . . . . . . . . . . . . . . . 13
2.3.4 Thermocouples . . . . . . . . . . . . . . . . . . . . . . 15
2.3.5 Thermodynamic temperature . . . . . . . . . . . . . . 16
2.4 Phase transitions . . . . . . . . . . . . . . . . . . . . . . . . . 17
2.5 History of calorimetry . . . . . . . . . . . . . . . . . . . . . . 18
3 Differential Scanning Calorimetry 21
3.1 Basics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21
3.1.1 Heat Capacity . . . . . . . . . . . . . . . . . . . . . . . 22
3.1.2 Melting and recrystallization . . . . . . . . . . . . . . . 23
3.1.3 Glass transition . . . . . . . . . . . . . . . . . . . . . . 24
3.1.4 Solid-solid transformations . . . . . . . . . . . . . . . . 25
3.2 Sample preparation . . . . . . . . . . . . . . . . . . . . . . . . 25
3.3 Transition points . . . . . . . . . . . . . . . . . . . . . . . . . 25
3.3.1 Melting point . . . . . . . . . . . . . . . . . . . . . . . 25
3
3.3.2 Transition enthalpy . . . . . . . . . . . . . . . . . . . . 26
3.3.3 Glass transition temperature . . . . . . . . . . . . . . . 27
4 Other TA techniques 29
4.1 Thermometry . . . . . . . . . . . . . . . . . . . . . . . . . . . 29
4.2 Differential Thermal Analysis (DTA) . . . . . . . . . . . . . . 29
4.3 Thermogravimetric Analysis (TGA) . . . . . . . . . . . . . . . 30
4.4 Dilatometry . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31
4.5 Thermomechanical Analysis (TMA) . . . . . . . . . . . . . . . 31
4.6 Thermo-optical Analysis (TOA) . . . . . . . . . . . . . . . . . 32
4.7 Evolved Gas Analysis (EGA) . . . . . . . . . . . . . . . . . . 33
5 Instrumentation 35
5.1 Setup . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 35
5.2 Temperature measurement . . . . . . . . . . . . . . . . . . . . 36
5.2.1 Classical heat flow sensor . . . . . . . . . . . . . . . . . 37
5.2.2 Improved classical heat flow sensor . . . . . . . . . . . 38
5.2.3 FRS5 and HSS7 heat flow sensors . . . . . . . . . . . . 38
5.3 Radboud University, Solid State Chemistry . . . . . . . . . . . 39
6 Artifacts 41
6.1 Different heating rates . . . . . . . . . . . . . . . . . . . . . . 41
6.2 Sample weight . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
6.3 Gas production . . . . . . . . . . . . . . . . . . . . . . . . . . 42
7 Applications 45
7.1 Phase diagrams . . . . . . . . . . . . . . . . . . . . . . . . . . 45
7.2 Polymorph detection . . . . . . . . . . . . . . . . . . . . . . . 46
7.3 Purity determination . . . . . . . . . . . . . . . . . . . . . . . 47
7.4 High temperature DSC . . . . . . . . . . . . . . . . . . . . . . 48
A Derivation formula 5.2 49
4
Chapter 1
Introduction
Differential Scanning Calorimetry (DSC) is an analytical technique in which
a sample and a reference are subjected to a temperature program and where
differences in heat capacity or heat of transitions are measured. Therefore, it
is part of the group of analytical techniques called Thermal Analysis (TA). [1]
This literature study starts with an introduction to calorimetry in chapter 2.
What properties do we measure with calorimetry? Why can we measure
these properties in this way? How do we measure temperature? What are
phase transitions? How did calorimetry start in the past?
In chapter 3 details about DSC measurement and specimen preparation will
be explained. How can we measure the heat capacity? How can we find
a melting point? What kind of additional information can we get from a
thermogram?
Other thermal analysis techniques will be explained in chapter 4. Chapter 5
is about the working of the DSC equipment that is used in scientific rereach
nowadays. In chapter 6 some common practical issues will be discussed and
in chapter 7 a few applications are mentioned.
5
6
Chapter 2
Introduction to calorimetry
In calorimetry your aim is to measure heat. Because there doesn’t exist
something like a ‘heat meter’, we have to measure the amount of heat in-
directly. This can be done in different ways: we can measure temperature
changes, look at phase transitions or use chemical, electric and mechanical
heat transfers. [2]
2.1 The Four Elements
Since 450 BC Greek philosophers divide the world into four elements: earth,
water, air and fire (see figure 2.1). Every material or force on earth is built
up from these four elements. And this classification is still used in modern
physics, but with different names. Earth, water and air are replaced by three
phases: solid, liquid and gas. Fire is replaced by heat (or energy in general),
which is the quantity we want to measure in calorimetry. [3]
7
Figure 2.1: The four elements.
2.2 Internal Energy and Heat
Before we can start measuring heat, we have to understand what ‘heat’ is.
Heat Q is an extensive property (depending on the amount of substance). It
is the amount of energy in a system as a result of a temperature difference
between the system and its surroundings. So one way to determine Q is to
cool the sample to the absolute zero of temperature (without changing it
physically or chemically) and then add energy until the original temperature
is reached. The sum of the added energy is the heat Q. [4–6]
Because this way of measuring heat is not doable practically, we try to de-
scribe heat first, in order to find easier ways in measuring it. The first step
in describing heat is to look at the internal energy of a system. The internal
energy of a system, which can only produce volume work (dW = −p dV ) is
described by the First Law of Thermodynamics as
dU = dQ + dW = dQ − pdV (2.1)
In this equation U is the internal energy of the system, Q is the amount of
energy transferred as heat to the system and W is the work done on the
8
system. p stands for pressure and V for volume. The SI-unit for the three
forms of energy (U , Q and W ) is the joule (J = m2 kg s−2). An old unit is
the calorie, which is equal to 4.184 J exactly.
When we write dU in exact differential notation, we get
dU =
(
∂U
∂T
)
V
dT +
(
∂U
∂V
)
T
dV (2.2)
Using equations (2.1) and (2.2), we can describe the heat Q in terms of the
variables of state T and V :
dQ = dU + p dV =
(
∂U
∂T
)
V
dT +
(
∂U
∂V
)
T
dV + p dV (2.3)
The heat capacity at constant volume is defined as
Cv ≡dQ
dT=
(
∂U
∂T
)
V
(2.4)
When we keep the volume constant (dV = 0) and fill in the definition of Cv
from equation (2.4), we can write equation (2.3) as
dQ|V =
(
∂U
∂T
)
V
dT = Cv dT (2.5)
So, if we use the variable of state T and keep the volume V constant, we can
measure the heat (Q) by integrating Cv dT over T :
Q|V =
∫
dQ|V =
∫ T=T1
T=T0
Cv dT = ∆U (2.6)
In most cases (read: in DSC) it is more convenient to use T and p as variables.
A comparable derivation can be done for that situation. In this case we don’t
look at the internal energy U , but consider the enthalpy H. Enthalpy has
9
the same unit as internal energy: joule (J) and is defined as
H ≡ U + pV (2.7)
When we, again, describe a system which can only produce volume work, we
get from equations (2.7), (2.1) and some mathematics (d(pV ) = p dV +V dp)
dH = dU + d(pV ) = dQ − p dV + p dV + V dp = dQ + V dp (2.8)
The heat capacity at constant pressure is defined as
Cp ≡dQ
dT=
(
∂H
∂T
)
p
(2.9)
When we write H in exact diffential notation, use equation (2.8) by constant
pressure and the definition from equation (2.9), we get
dQ|p =
(
∂H
∂T
)
p
dT = Cp dT (2.10)
So when we work at constant pressure, we can measure the heat Q by inte-
grating Cp d T over T :
Q|p =
∫
dQ|p =
∫ T=T1
T=T0
Cp dT = ∆H (2.11)
2.3 Temperature and temperature scales
In the derivation above we used temperature, without knowing the details
about it. Temperature T is the intensive parameter (independent of the
amount of substance) of heat. The standard unit of temperature nowadays
is kelvin, K. [5]
When we want to use numbers to indicate a temperature, we have to use a
10
scale. And during the last centuries many scales have been in use.
2.3.1 Physiological temperature scale
When people are born, they already are able to recognize temperatures
around body temperature by using thermoreceptors: ‘cold’ means ‘colder
than body temperature’, ‘hot’ means ‘hotter than body temperature’. [7]
Temperatures further away from body temperature can be recognized through
the degree of pain. Colder and warmer increases the amount of pain. You get
a temperature scale from ‘ice cold’, via ‘cold’, ‘lukewarm’, ‘warm’ and ‘hot’
towards ‘red hot’. But it is difficult to use numbers to describe a temperature
measured with a thermoreceptor or an amount of pain. These scales only
give qualitative information. [2]
2.3.2 Liquid in glass
In the 17th century liquid-in-glass Florentine thermometers are developed.
This kind of thermometer is based on the difference in expansion coefficient
of a liquid and the glass. The scale can be chosen in different ways: almost
every pair of setpoints is usable. Between those setpoints a linear scale is
used. Consequently, these scales are empirical. The temperature t is linear
dependent of the length ` of the liquid column. [2]
t = a + b ` (2.12)
In the next century four scales became standards. All of them are based
on the linear expansion of a liquid in glass containers. These scales are
summarized in table 2.1. Remarkable is that the Celsius scale was first used
in a reversed way: freezing water was labeled 100 ◦C, and boiling water 0 ◦C.
But also this kind of thermometers has disadvantages. The main sources of
11
errors are time and immersion effects.
• Over years the glass of the thermometer will contract, introducing an
error of about 1–2 ◦C.
• To measure a temperature, you have to wait until the bulb containing
the liquid and the environment have come to equilibrium, but as heat
flow decreases in time when getting closer to equilibrium this can take
a considerable period of time (1–2 seconds to reach half the initial
temperature difference).
• Hysteresis effects slow down the measurements. These processes take
minutes on heating, but hours on cooling, with an error of about 1–2◦C per 100 ◦C.
• Pressure excerted on the glass bulb can also influence the reliability.
• The largest deviation is caused by partial immersion of the thermometer
(see figure 2.2), but for this error corrections are possible.
Figure 2.2: Partial immersion of a thermometer.
The error in temperature Terror caused by partial immersion can be calculated
by
Terror = kn(t − θ) (2.13)
12
In this equation k is the differential glass-mercury expansion coefficient (ap-
prox. 1.6 · 104), n is the mercury column length outside the bath (in degrees
of scale), t is the temperature the thermometer shows and θ is the temper-
ature of the stem, i.e. the glass column outside the bath (mostly at room
temperature). Using this equation the corrected temperature Tcorrected is
Tcorrected = T + Terror = t + kn(t − θ) = (1 + kn) · t − kn · θ (2.14)
Table 2.1: Temperature scales (liquid in glass)Year Person Description Value1701 Newton freezing water 0 ◦
body temperature 12 ◦
1714 Fahrenheit NaCl-ice-water 0 ◦
body temperature 96 ◦
later Fahrenheit freezing water 32 ◦
boiling water 212 ◦
1730 Reaumur ice point water/ethanol (80:20) 0 ◦
steam point water/ethanol (80:20) 80 ◦
1742 Celsius freezing water 0 ◦Cboiling water 100 ◦C
2.3.3 Resistance Thermometers
An other way of determining temperature is by measuring the electrical re-
sistance of a metal or semiconductor. [2, 8–10] Resistance is temperature
dependent and can be used as a measure for temperature. This effect is de-
scribed in an equation found by Hugh Longbourne Callendar, and refined by
Van Dusen:
RT = R0(1 + AT + BT 2 − C(T − 100)T 3) (2.15)
13
In this equation RT is the specific electrical resistance at temperature T . R0
is the resistance at 0 ◦C. T stands for the temperature in degrees Celsius (!)
and A, B and C are the Callendar-Van Dusen constants. For temperatures
above 0 ◦C C is equal to zero and the equation can be simplified to
RT = R0(1 + AT + BT 2) (2.16)
As this equation is kwadratic in T , it can be solved to an analytical expression
for T as a function of RT :
T (RT ) =−R0A +
√
R20A
2 − 4R0B(R0 − RT )
2R0B(2.17)
The Callendar-Van Dusen constants A, B and C for a standard sensor are
stated in IEC 751 by the International Electrotechnical Commission. For dif-
ferent sensors (or higher accuracy) it is possible to determine these constants
by measuring resistances at four temperatures:
• Measure R0 at t0 = 0 ◦C (freezing point of water)
• Measure R100 at t100 = 100 ◦C (boiling point of water)
• Measure Rh at th = a high temperature (e.g. Tfus zink, 419.53 ◦C)
• Measure Rl at tl = a low temperature (e.g. Tvap oxygen, −182.96 ◦C)
From these resistances α, δ and β are calculated:
α =R100 − R0
100 · R0
(2.18)
δ =th −
Rh−R0
R0·α(
th100
− 1) (
th100
) (2.19)
β =tl −
[
Rl−R0
R0·α+ δ
(
tl100
− 1) (
tl100
)
]
(
tl100
− 1) (
tl100
)3(2.20)
14
And α, δ and β can be converted into A, B and C by
A = α +α · δ
100(2.21)
B = −α · δ
1002(2.22)
C = −α · β
1004(2.23)
2.3.4 Thermocouples
The last way of thermometry (discussed in this literature study) is by us-
ing thermocouples. [2] When two connections of different metals are placed
at different temperatures (see figure 2.3), a net thermal electromotive force
occurs. This phenomenon is called the Seebeck effect, discovered in 1821 by
Thomas Seebeck.
Figure 2.3: A thermocouple.
In this way the potential difference is a measure for the temperature differ-
ence, described by the equation
EAB(t, t0) = a + bt + ct2 (2.24)
In this equation one of the connections is placed at t0 = 0 ◦C, the ice point
of water. EAB is the potential difference and t is the temperature in degrees
Celsius. a, b and c are calibration constants, depending on the materials
used.
15
It is possible to place just one or both connections at the reference temper-
ature. In the first case, the potentiometer is placed in the wiring of metal
A or B. In the second case copper wires are used to connect the two ends of
the thermocouples with the potentiometer, as depicted in figure 2.4.
Figure 2.4: Two setups for thermocouples.
In table 2.2 several combinations of metals are listed. The electromotive
forces at different temperatures are in microvolts per degree Celsius.
Table 2.2: Electromotive forces (in µV/◦C) of several combinations of metalscombination −190◦C 0◦C 500◦C 1000◦C 1500◦CCopper-Constantan 17 38.4 – – –Iron-Constantan 26 50.1 56 – –Chromel-Alumel 23 40.0 43 39 –Pt-Pt/10%Rh – 5.5 10 12 15
Nowadays there is an alternative for placing one connection at the ice point
of water. After calibration (with one connection at the ice point of water)
it is possible to use a compensator to measure the (room) temperature and
correct for the actual temperature of the reference.
2.3.5 Thermodynamic temperature
When scientists discovered that there is a minimum energy and consequently
a minimum temperature, they used this temperature as an absolute setpoint
16
for the temperature scale: 0 K. In earlier temperature scales the two setpoints
were chosen arbitrarily. This was the first scale with one arbitrary and one
absolute setpoint. [2, 4]
The other setpoint of this scale is the triple point of water, at 273.16 K. This
number is chosen so that the units of this scale are equal in size as the units
of the scale chosen by Celsius: one Kelvin temperature difference is equal to
a temperature difference of one degree Celsius.
2.4 Phase transitions
Besides temperature, you can also look at phase transitions when performing
calorimetric experiments. A liquid sample can be made gaseous by adding
energy. Adding energy increases the temperature of the sample, until it
begins to boil. Then, the temperature remains constant. When the sample
is evaporated completely, its temperature increases again. The opposite is
also possible: by removing energy, its temperature decreases and the sample
starts freezing. These are both examples of phase transitions.
In a phase transition the chemical composition of the sample doesn’t change.
Only its phase changes by adding or removing energy. Phase changes are
possible between all the three phases and as well as between two solid phases,
as summarized in table 2.3. The temperature at which the phase transition
occurs, is called the transition temperature Ttrs, where the subscript indicates
the kind of transition. [4]
Table 2.3: Names of phase transitions (IUPAC abbreviations)� Solid Liquid Gas
Solid S-S Transformation (trs) Fusion (fus) Sublimation (sub)Liquid Freezing – Vaporization (vap)Gas Deposition Condensation –
17
2.5 History of calorimetry
The first calorimetric experiments were done in the 18th century. In 1760
J. Black placed a hot object in a cavity in a block of ice and used the amount
of molten ice as a measure for the amount of heat (see figure 2.5). [2]
Figure 2.5: First setup of heat measurement.
In 1781 Laplace was the first to make an apparatus for this measurement,
based on the same technique, but with much better isolation (see figure 2.6).
He placed a sample of higher temperature T1 in basket LM (at the bottom
of figure 2.6), which he inserted into the calorimeter cavity ff. He placed the
lid HG (second part from the bottom of figure 2.6) on top of the basket LM.
Afterwards he placed the lid FF (at the top of figure 2.6) on the apparatus.
The heat flow from the sample made the measuring ice in volume HGbbd
melting, until equilibrium was reached. For larger samples this might take
even 12 hours. The whole calorimeter was kept adiabatic by a second, insu-
lating layer of ice in FFaaaa. After the experiment, the molten measuring ice
(water) was drawn through the stopcock y and weighed. [2, 11] The average
heat capacity was then given by
cp =mwater ∆Hfus
msample (T1 − T0)(2.25)
18
In this equation mwater is the mass of the molten measuring ice. msample is
the mass of the sample and ∆Hfus is the heat of fusion of one unit mass of
ice (unit: J g−1). T1 is the initial temperature of the sample and T0 is the
melting temperature of the measuring ice (0◦C).
Modern adiabatic calorimetry experiments are based on the Nernst calorime-
ter. This type of calorimeter is decreased in size, automated and computer-
ized. It is still the best tool to measure heat capacities from 10 K to room
temperature. [12] The heat capacity of the sample is in this case calculated
from the heater input ∆Q, determined electrically by resistance heating, and
the temperature increase ∆T . In this formula C ′ is the heat capacity of the
empty calorimeter, its ‘water value’. [5]
cp =∆Qcorrected − C ′∆Tcorrected
∆Tcorrected msample
(2.26)
The next step in the developement of calorimetry was Differential Scanning
Calorimetry (DSC), with a larger temperature range: 200 to 1000 K. The
main advantage of the DSC is that the correction procedure (needed when
using earlier calorimeters) is simplified.
19
Figure 2.6: The first ‘calorimeter’, by Laplace.
20
Chapter 3
Differential Scanning
Calorimetry
Around 1900 it became possible to measure temperature continuously using
thermocouples. This was the start of the development of Differential Thermal
Analysis. In 1904 Kurnakov and Saladin were the first to make the classical
DTA set-up: photographic T − ∆T − t-recording, reference temperature for
thermocouples and a DTA-furnace.
3.1 Basics
In a Differential Scanning Calorimetry (DSC) experiment the aim is to keep
the sample and a reference (at constant pressure) at the same temperature
throughout a temperature programme. During the experiment the heat flow
(heat transferred to or from the sample and the reference) is measured. The
term ‘Differential’ refers to the fact that the sample data are compared to
the reference data. In such an experiment one is ‘Scanning’ through a tem-
perature programme. [4, 13, 14]
21
3.1.1 Heat Capacity
Heating the sample costs more energy than heating the reference, because
one has to increase the temperature of the sample holder and the sample
itself. From the difference heat flow dQ
dt, needed to heat a sample minus the
reference, and the heating rate dTdt
one can calculate the heat capacity at
constant pressure Cp.
Cp =
(
dQ
dT
)
p
=
(
dQ
dt
dt
dT
)
p
=
(
dQ/dt
dT/dt
)
p
=
(
heat flow
heating rate
)
p
(3.1)
When using a constant heating rate (dTdt
= a), the heat flow at constant
pressure is proportional to the Cp.
(
dQ
dT
)
p
= Cp ·
(
dT
dt
)
p
= Cp · a (3.2)
In a plot of heat flow against temperature the Cp is visible (multiplied with
the (constant) heating rate). In figure 3.1 a constant heating rate is measured.
Figure 3.1: Measuring the heat capacity.
22
3.1.2 Melting and recrystallization
When you continue heating, eventually the sample will begin to melt. But
to keep the temperature of the sample and reference the same, more heat
is needed for the sample. In a plot of heat flow against temperature an
endothermal peak (increase of heat flow) will become visible. An exothermal
peak (decrease of heat flow) will appear when solidification occurs.
Figure 3.2: Measuring an (endothermal) melting peak.
In theory the Cp of melting and solidification is infinitely large. Because it
takes time to transport the heat through the sample, the peak is not infinitely
high and small, but broadened, with the same peak area as decribed in section
3.3.2.
Metastable solids can melt twice. After the first melting a metastable liquid
is formed, which recrystallizes at higher temperatures into a different crystal
structure. In this process energy will be released and an exothermic peak can
be expected. Shortly after recrystallization, the sample will melt again, with
an endothermic peak. This phenomenon was observed for bismuth germanate
by using in-situ optical microscopy. [15]
23
Figure 3.3: Measuring a recrystallization.
3.1.3 Glass transition
Glass transitions of polymers can also be determined by DSC. Below the glass
transition temperature Tg the sample is amorphous. At higher temperatures
the molecules have enough energy to become crystalline. The Cp increases
when you go from below to above the Tg. In a plot of heat flow against
temperature (with constant heating rate) this is visible as an increase in the
baseline (see also section: 3.1.1).
Figure 3.4: Measuring a glass transition.
24
3.1.4 Solid-solid transformations
Phase transitions in the solid phase can be made visible too. The integral over
the peak indicates the enthalpy change involved with transition: endothermal
or exothermal. Many different peak shapes can occur.
3.2 Sample preparation
The standard procedure for sample preparation starts with grinding the sam-
ple using a mortar and pestle to reach homogeneity. This is essential, as
samples of well-grinded and single crystals can give very different results, as
described in [16]. Between 0.5 and 20 mg of the powder is transferred into
an aluminium sample pan. A lid is pressed onto the pan. Sometimes the lid
is pierced, to maintain constant pressure (see section 6.3). [1, 14]
Using the aluminium pans above 500 ◦C will result in destruction of the
DSC sample holder. So for temperatures above 500 ◦C (or for samples which
react with the aluminium pans), gold, graphite or glass pans are available.
During the measurement, the sample is continuously flushed with an inert
gas (mostly nitrogen, between 20 and 80 cm3 min−1), to prevent oxidation of
the sample. The reference is an empty pan of the same kind.
3.3 Transition points
3.3.1 Melting point
A first order transition is characterized by its baseline and the peak. In such
a curve there are a couple of characteristic temperatures: the beginning of
melting, the peak temperature and the return to the baseline. And none of
these is the same as the melting point. To determine the melting point, one
25
has to extrapolate the baseline and the left tangent of the temperature peak
as shown in figure 3.5. [2]
Figure 3.5: Melting point determination.
3.3.2 Transition enthalpy
Using equation (2.11) we can state that the peak area A (the area between
the peak and an interpolation of the baseline) is proportional to the amount
of energy absorbed/released by the transition ∆Htrs:
A ∝ ∆Htrs (3.3)
26
3.3.3 Glass transition temperature
An amorphous sample that is heated from below to above the glass transition
temperature will become more crystalline. This transition takes time, so in
a plot of heat flow against temperature (with constant heating rate) the
increase of the baseline is spread over a temperature range. For the glass
transition temperature the middle of the incline is chosen, as depicted in
figure 3.6. [13]
Figure 3.6: The glass transition temperature.
27
28
Chapter 4
Other TA techniques
4.1 Thermometry
Thermometry is the oldest thermal analysis technique. It involves measure-
ment of temperature, usually as a function of time. When a constant heat
input is used and temperature is measured in time, a heating curve can be
created from this data. The slope of such a curve gives information about the
sample’s heat capacity and phase transition. When the temperature stays
constant, while heating up the sample, the sample must be melting (possibly
eutectic) or vaporizing. [2]
4.2 Differential Thermal Analysis (DTA)
Differential Thermal Analysis can be done in the same setup as DSC. The
difference between these techniques is the paramater that is kept constant.
By DSC the temperatures of the sample and reference are equal, by using
different heat flows Qsample and Qreference. By DTA the amount of heat Q
supplied to sample and reference is the same. Phase transitions will cause
29
the temperature of the sample Tsample to be lower (endothermic) or higher
(exothermic) than that of the reference Treference.
Figure 4.1: Differences between reference temperature and sample tempera-ture at constant heat flow.
4.3 Thermogravimetric Analysis (TGA)
In Thermogravimetric Analysis the sample is subjected to a temperature
program, while the mass of the sample is measured by a highly sensitive
electronic balance. Usually the experiment is performed under an inert at-
mosphere (nitrogen), but an oxidative one (air or oxygen) is also possible.
To compensate for gas flow effects, a blank curve is substracted. [14]
The first part of a TGA curve provides information about volatile components
(1), such as solvents or water. At higher temperatures water of crystallization
can come free (2). Eventually the sample will evaporate or decompose (3). [1]
This technique is often used in combination with a mass spectrometer or a gas
chromatograph, to analyse the volatile compounds. See also section 4.7. [2]
30
Figure 4.2: Schematic view of a TGA curve.
4.4 Dilatometry
In Dilatometry length and/or volume of a sample is measured, while being
subjected to a temperature program. This technique gives information about
linear expansion coefficients, glass transitions, polymorphic transformations
that cause volume changes of solids and shrinkage or expansion of fibers or
films.
4.5 Thermomechanical Analysis (TMA)
The aim of Thermomechanical Analysis (TMA) is roughly the same as that
of Dilatometry. The difference is that the measurements are performed
under tension or load. So the aim of this technique is measuring dimen-
sional changes of a sample under a constant, well defined load. If a period-
31
ically changing load is applied, the technique is called dynamic load TMA
(DLTMA). In dilatometric measurements the load on the sample is low or
negligable. The TMA signal represents the change in length measured with
a high resolution displacement sensor. TMA provides information on soft-
ening temperatures, dimensional stability on heating and viscoelastic behav-
ior. [1, 2]
Figure 4.3: Schematic view of a TMA curve.
4.6 Thermo-optical Analysis (TOA)
In Thermo-optical Analysis the sample is subjected to a temperature pro-
gram, while measuring the optical transmission or reflection of the sample.
Automatic melting point and dropping point instruments use this technique.
For example, a solid sample is melted, with an increase of transmittance.
Irregularities during the melting can be caused by crystals moving through
the light beam. [1]
32
Figure 4.4: Schematic view of a TOA curve.
4.7 Evolved Gas Analysis (EGA)
The name Evolved Gas Analysis is used when volatile components of a sample
are investigated, while performing thermal analysis, for example by a mass
spectrometer or an infrared spectrometer. A common combination is TGA
with a mass spectrometer. In figure 4.5 the temperature of the sample is
measured, while a mass spectrometer measured the intensity of molecules
with mass-to-charge ratio (m/q) 18 (water) and 44 (CO2). In step 1 and 2
surface water and water of crystallization is removed. In step 3 decomposition
of the organic sample takes place, by releasing water and CO2. [1]
33
Figure 4.5: Schematic view of a EGA curve.
34
Chapter 5
Instrumentation
5.1 Setup
In figure 5.1 a schematic view of a DSC is shown. [17] The main parts of the
device take care of temperature control: heater and cooler. The numbers
1 and 3 to 5 show the different parts of the furnace, the numbers 6 to 9
the parts of the cooler. Number 10 shows the cabel that conducts the raw
signal to the amplifier and number 11 and 12 show the dry and purge gas
inlets. The sample and reference are shown by number 2 and are placed on a
temperature sensor, the most important part of the device (see section 5.2).
Sometimes a sample robot can be used to change samples. When using it, a
DSC can work 24 hours a day, without assistance of a researcher. For oxygen-
sensitive or hygroscopic samples there is a possiblity to let the robot remove
a protective cap from the sampleholders immediately before measurement.
35
Figure 5.1: Schematic view of a DSC. 1) Furnace lid 2) Sample and referenceon the DSC sensor 3) Silver furnace 4) PT100 of furnace 5) Flat heaterbetween two electrically insulating disks 6) Thermal resistance for cooler 7)Cooling flange 8) Compression spring construction 9) Cooling flange PT10010) DSC raw signal for amplifier 11) Dry gas inlet 12) Purge gas inlet.
5.2 Temperature measurement
In DSC three different kinds of temperature sensors are used, as described
in [18]: the classical heat flow sensor, the improved classical heat flow sensor
(based on single T0 temperature measurement) and the FRS5 and HSS7 heat
flow sensors (based on multiple T0 temperature measurement) introduced by
the Mettler-Toledo company.
36
5.2.1 Classical heat flow sensor
Figure 5.2: Classical heat flow sensor.
The classical heat flow sensor measures the temperature of the sample and
the reference each with one thermocouple (see section 2.3.4). The effective
heat flow can be calculated with the simplified formula, mentioned in [18].
dq
dt=
1
R∆T (5.1)
In this equation R stands for the thermal resistance of the sensor and ∆T
stands for the temperature difference between the sample and the reference.dq
dtis the difference in heat flow between sample and reference and is the heat
used for warming up or transforming the specimen material.
This formula can only be used under the assumption that the thermal resis-
tances and the heat capacities on the sample and the reference sides are the
same (R = RS = RR and CR = CS) and the temperature difference between
the sample and the reference is approximately zero ( d∆Tdt
≈ 0).
The main problem with this sensor is the assumption that the sample tem-
perature is uniform.
37
5.2.2 Improved classical heat flow sensor
In the improved classical heat flow sensor the sensor temperature is addition-
ally measured at one place (single T0 measurement). With this information
the thermal resistances and the heat capacities can be measured as well.
The heat flow can be calculated using the formula mentioned in [18], with-
out derivation. A possible derivation, with some remarks about mistakes in
the equation, can be found in appendix A).
dq
dt= −
∆T
RR
+ ∆TS0
(
1
RS
+1
RR
)
+ (CR − CS)dTS
dt− CR
d∆T
dt(5.2)
In this equation ∆T stands for the temperature difference between the sample
and the reference: TS − TR. RS and RR are thermal resistances and CS and
CR are heat capacities of the sample and the reference.
Figure 5.3: Improved classical heat flow sensor.
5.2.3 FRS5 and HSS7 heat flow sensors
The FRS5 and HSS7 sensors introduced by the Mettler-Toledo company
measure heat flows seperately on the sample and reference sides, by using two
rings of thermocouples. In the inner ring the sample or reference temperature
is measured, in the outer one the temperature of the sensor. In this case the
voltage outputs of the thermocouples are added, giving
38
Figure 5.4: FRS5 and HSS7 heat flow sensor.
dq
dt=
1
R
(
N∑
i=1
(∆TS0)i −N∑
i=1
(∆TR0)i
)
(5.3)
In this equation ∆TS0 and ∆TR0 stand for the temperature differences be-
tween sample and sensor and between reference and sensor.
In the FRS5 sensor 56 thermocouples are used (N = 14). In the HSS7 sensor
120 themocouples are used (N = 30). A picture of such a sensor can be
seen in figure 5.5. The sensor temperature is measured multiple times so we
speak of multiple T0 measurement. This largely improves the accuracy of the
heat flow measurement as compared to the classical heat flow sensor. When
compared with the FRS5, the HSS7 is 5 (at −64.6 ◦C) to 10 (at 135.2 ◦C)
times more sensitive.
5.3 Radboud University, Solid State Chemistry
The department of Solid State Chemistry possesses two DSC’s, one from
Mettler Toledo, one from Setaram.
39
Figure 5.5: HSS7 temperature sensor with 120 thermocouples.
• Mettler Toledo dsc822e with the Mettler Toledo TSO 801RO Sample
Robot and Julabo FT900 cooler.
• Setaram Calvet Calorimeter C80 with control device Setaram C32.
40
Chapter 6
Artifacts
6.1 Different heating rates
When scanning through a temperature profile, a heating rate needs to be set.
Depending on the type of DSC one is using, this can be set between 0.1 and
10 ◦C min−1. At different heating rates different heating curves are obtained.
At higher heating rates the peaks will get broader and the maximum (peak
value) shifts toward higher temperature. The melting point doesn’t change
(at least not as much as the maximum does), if read out in the correct way
as described in section 3.3.1.
In figure 7.1 this is shown. Remark: the areas under the different peaks must
be equal, because that is a measure for the amount of heat needed for a phase
transition. In this figure apparently different scales have been used for the
three peaks. [1]
Higher heating rate causes peak broadening while the surface area remains
constant. Moreover, less peaks will be visible, because the sample has no
time for phase transition. So a slow heating rate gives the most details. . .
until the signal-to-noise ratio becomes such low that the signal disappears
41
in the noise. For a very low heating rate a measurement takes a long time.
The heat flow to the sample will be approximately equal the heat flow to
the reference, because the transitions in the sample are spread out over long
times.
6.2 Sample weight
The mass of a sample should be kept as small as possible, to achieve re-
producibility if neccesary. Bigger samples give various problems. The tem-
perature of the sample can become non-uniform, because heat needs time
to transfer through the sample. Through temperature differences chemical
reactions can occur. And small sample masses also protect the apparatus in
the event of explosion, deflagration or corrosion. [14]
6.3 Gas production
When the sample is heated, the sample can partially evaporate. If the lid
is placed on the pan, the pressure in the pan can increase, while the mea-
surement has to be performed at constant pressure by equation (2.11). To
maintain constant pressure, the lid can be pierced.
42
Figure 6.1: Melting point independence of heating rate.
43
44
Chapter 7
Applications
7.1 Phase diagrams
DSC is often used in the determination of phase diagrams, because the con-
ditions of the experiments are well-defined. Slow heating rates can be used to
approach equilibrium as good as possible. Several samples of different compo-
sition are measured. When the peaks of the curves are interpreted correctly
(endothermic peaks stand for melting temperatures), a phase diagram can
be constructed from this data.
In [19] the phase diagram for the rubidium bromide/copper(I) bromide sys-
tem is determined by DSC. In the system two intermediate compounds are
formed: RbCu2Br3 (melting at 537 K) and Rb3CuBr4 (melting at 544 K).
Two eutectic points are found at 501 K (54 mole%) CuBr and 522 K (74
mole%) CuBr.
For DSC measurements a Mettler Toledo DSC25 apparatus with TC15 TA
Controller and STARe Software 4.0 is used. The heating rates were 2 and
0.5 K min−1 for all samples. Further examples of the determination of phase
diagrams can be found in [20–30].
45
Figure 7.1: Phase diagram for the rubidium bromide/copper(I) bromide sys-tem.
7.2 Polymorph detection
DSC can also be used in polymorph research. [31] When heating curves of
different polymorphs of one compound are measured, different melting points
can show up. An example is Venlafaxine, a pharmaceutical compound that
46
acts a an antidepressivum. The melting points of the three polymorphs are
respectively 74.42, 77.72 and 78.47 ◦C. In figure 7.2 it is visible that form I
recrystallizes into form III.
Figure 7.2: Thermogram Venlafaxine: form I recrystallizes into form III.
7.3 Purity determination
The change of melting temperature induced by the presence of an impurity
in the material, is expressed in the Van ’t Hoff equation [32, 33]:
Tf = T0 −RT0Tfus
∆Hf
ln
(
1 − x1
F
)
(7.1)
47
This equation can be simplified to
Tf = T0 −RT 2
0
∆Hf
x1
F(7.2)
In these equations Tf is the melting temperature, T0 is the melting point
of the pure substance, R is the gas constant (8.314 Jmol−1K), ∆Hf is the
molar heat of fusion (calculated from the peak area), x is the mole fraction
of the impurity, Tfus is the melting point of the impure substance and F is
the fraction melted (F = Apart
Atot).
In [32] a ‘short’ method is compared with the commonly used one. For the
short method it is not needed to melt a sample completely, because ∆Hfus is
not used. This can be useful if samples start to decompose quickly after the
melting starts. The results of both methods are comparable.
7.4 High temperature DSC
In gas turbine engines nickel based superalloys are used. These compounds
have complex compositions and small changes in composition can affect the
properties a lot. Because industry is using higher and higher operating tem-
peratures, the alloys must have high melting points. Studies of these com-
pound have to take place at elevated temperatures. DSC is one of the few
techniques that can handle these temperatures.
To perform high temperature experiments some modifications are made to
the DSC setup. Stainless steel gas lines are used and a commercial gas
purification train is used to reduce the effects of oxygen, moisture and other
possible contaminants. Also a one way (Bunsen) valve prevents ingress of
oxygen from the exhaust. With this setup experiments up to 1400 degrees
Celsius are performed on nickel alloys. The melting points of the compounds
investigated are around 1300 and 1350 degrees Celsius. [34]
48
Appendix A
Derivation formula 5.2
Formula 5.2 is mentioned in [18], without derivation.
dq
dt= −
∆T
RR
+ ∆TS0
(
1
RS
+1
RR
)
+ (CR − CS)dTS
dt− CR
d∆T
dt
The formula is – probably – derived from a model that describes heat trans-
port (to the sample and to the reference) and the absorption of heat (by the
sample and the reference) as processes that can occur at the same time. But
physically the transport has to take place before the sample or the reference
can take up heat. From this point of view a serial process is expected to give
a better solution.
For the parallel model, mentioned first, the heat flow to the sample ( dqS
dt) and
to the reference (dqR
dt) are then described by
dqS
dt=
TS − T0
RS
− CS
dTS
dt(A.1)
dqR
dt=
TR − T0
RR
− CR
dTR
dt(A.2)
49
The difference between these heat flows is derived by substracting the two
equations.
d∆q
dt=
dqS
dt−
dqR
dt(A.3)
=TS − T0
RS
− CS
dTS
dt−
TR − T0
RR
+ CR
dTR
dt(A.4)
TS − T0 can be written as TS0. In the third term TR can be rewritten as
TR = TS − ∆T .
d∆q
dt=
∆TS0
RS
− CS
dTS
dt−
TS − ∆T − T0
RR
+ CR
dTR
dt(A.5)
The third term can be split in two parts.
d∆q
dt=
∆TS0
RS
− CS
dTS
dt−
TS − T0
RR
+∆T
RR
+ CR
dTR
dt(A.6)
The third term can be abbreviated to ∆TS0
RRand combined with the first term.
The fourth term is placed as first.
d∆q
dt=
∆T
RR
+ ∆TS0
(
1
RS
−1
RR
)
− CS
dTS
dt+ CR
dTR
dt(A.7)
In this equation TR can be rewritten as TS −∆T . Expanding this term gives
d∆q
dt= . . . − CS
dTS
dt+ CR
dTS
dt− CR
d∆T
dt(A.8)
where . . . stands for ∆TRR
+ ∆TS0
(
1RS
− 1RR
)
.
50
The first two terms of equation (A.8) can be combined.
d∆q
dt= . . . (CR − CS)
dTS
dt− CR
d∆T
dt(A.9)
The complete equation becomes
d∆q
dt=
∆T
RR
+ ∆TS0
(
1
RS
−1
RR
)
(CR − CS)dTS
dt− CR
d∆T
dt(A.10)
The only difference with the formula from [18] is the absence of the minus
sign before ∆TRR
. This minus sign is also absent in the simplified equation
mentioned in the same article.
51
52
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