Electrical resistivity (also known as resistivity, specific electrical resistance, or volume resistivity) is a measure of how strongly a material opposes the flow of electric current. A low resistivity indicates a material that readily allows the movement of electric charge. The SI unit of electrical resistivity is the ohm metre (Ωm). It is commonly represented by the Greek letter ρ (rho).
Electrical conductivity or specific conductance is the reciprocal quantity, and measures a material's ability to conduct an electric current. It is commonly represented by the Greek letter σ (sigma), but κ (esp. in electrical engineering) or γ are also occasionally used. Its SI unit is siemens per metre (S·m−1) and CGSE unit is reciprocal second (s−1):
Contents |
Electrical resistivity ρ (Greek: rho) is defined by,
where
and E and J are both inside the conductor.
Many resistors and conductors have a uniform cross section with a uniform flow of electric current and are made of one material. (See the diagram to the right.) In this case, the above definition of ρ leads to:
where
The reason resistivity has the dimension units of ohm-metres can be seen by transposing the definition to make resistance the subject:
The resistance of a given sample will increase with the length, but decrease with greater cross-sectional area. Resistance is measured in ohms. Length over area has units of 1/distance. To end up with ohms, resistivity must be in the units of "ohms×distance" (SI ohm-metre, US ohm-inch).
In a hydraulic analogy, increasing the cross-sectional area of a pipe reduces its resistance to flow, and increasing the length increases resistance to flow (and pressure drop for a given flow).
The scalar equation:
or equivalently
is only valid for resistors and conductors which are homogeneous and isotropic, that is the conductivity is uniform throughout the conductor, carrying a uniform electric current per unit cross-sectional area J, through a uniform internal electric field E, all in one dimension only.
For all three dimensions we have at all points (r = position vector at a point in the conductor):
in which (1, 2, 3 refer to components)
This is still only true if E and J are collinear, under the same conditions as above.
Since E and J are generally vector fields, the material may not be homogeneous or isotropic so the conductivity may vary from point to point, and the E and J are not always collinear at the same point, the definition generalizes by treating conductivity as a rank-2 tensor field σ:
where rank-2 tensors can be represented by matrices
equivalent to the matrix equation
which allows a simple relation between components to be read off, using the Einstein summation convention;
The above tensor equation serves as a definition for the conductivity tensor (or field). A similar analysis for resistivity can be done, introducing a resistivity tensor (or field) in an identical form,
in which
so
Quantum mechanics states that the energy of an electron in an atom cannot be any arbitrary value. Rather, there are fixed energy levels which the electrons can occupy, and values in between these levels are impossible. The energy levels are grouped into two bands: the valence band and the conduction band (the latter is generally above the former). Electrons in the conduction band may move freely throughout the substance in the presence of an electrical field.
In insulators and semiconductors, the atoms in the substance influence each other so that between the valence band and the conduction band there exists a forbidden band of energy levels, which the electrons cannot occupy. In order for a current to flow, a relatively large amount of energy must be furnished to an electron for it to leap across this forbidden gap and into the conduction band. Thus, even large voltages can yield relatively small currents.
A metal consists of a lattice of atoms, each with a shell of electrons. This is also known as a positive ionic lattice. The outer electrons are free to dissociate from their parent atoms and travel through the lattice, creating a 'sea' of electrons, making the metal a conductor. When an electrical potential difference (a voltage) is applied across the metal, the electrons drift from one end of the conductor to the other under the influence of the electric field.
Near room temperatures, the thermal motion of ions is the primary source of scattering of electrons (due to destructive interference of free electron waves on non-correlating potentials of ions), and is thus the prime cause of metal resistance. Imperfections of lattice also contribute into resistance, although their contribution in pure metals is negligible.
The larger the cross-sectional area of the conductor, the more electrons are available to carry the current, so the lower the resistance. The longer the conductor, the more scattering events occur in each electron's path through the material, so the higher the resistance. Different materials also affect the resistance.[2]
In metals, the Fermi level lies in the conduction band (see Band Theory, below) giving rise to free conduction electrons. However, in semiconductors the position of the Fermi level is within the band gap, approximately half-way between the conduction band minimum and valence band maximum for intrinsic (undoped) semiconductors. This means that at 0 kelvins, there are no free conduction electrons and the resistance is infinite. However, the resistance will continue to decrease as the charge carrier density in the conduction band increases. In extrinsic (doped) semiconductors, dopant atoms increase the majority charge carrier concentration by donating electrons to the conduction band or accepting holes in the valence band. For both types of donor or acceptor atoms, increasing the dopant density leads to a reduction in the resistance. Highly doped semiconductors hence behave metallic. At very high temperatures, the contribution of thermally generated carriers will dominate over the contribution from dopant atoms and the resistance will decrease exponentially with temperature.
In electrolytes, electrical conduction happens not by band electrons or holes, but by full atomic species (ions) traveling, each carrying an electrical charge. The resistivity of ionic liquids varies tremendously by the concentration - while distilled water is almost an insulator, salt water is a very efficient electrical conductor. In biological membranes, currents are carried by ionic salts. Small holes in the membranes, called ion channels, are selective to specific ions and determine the membrane resistance.
The degree of doping in semiconductors makes a large difference in conductivity. To a point, more doping leads to higher conductivity. The conductivity of a solution of water is highly dependent on its concentration of dissolved salts, and other chemical species that ionize in the solution. Electrical conductivity of water samples is used as an indicator of how salt-free, ion-free, or impurity-free the sample is; the purer the water, the lower the conductivity (the higher the resistivity). Conductivity measurements in water are often reported as specific conductance, relative to the conductivity of pure water at 25 °C. An EC meter is normally used to measure conductivity in a solution. A rough summary is as follows:
Material | Resistivity ρ (Ω·m) |
Metals | 10−8 |
Semiconductors | variable |
Electrolytes | variable |
Insulators | 1016 |
Superconductors | 0 |
This table shows the resistivity, conductivity and temperature coefficient of various materials at 20 °C (68 °F)
Material | ρ (Ω·m) at 20 °C | σ (S/m) at 20 °C | Temperature coefficient[note 1] (K−1) |
Reference |
---|---|---|---|---|
Silver | 1.59×10−8 | 6.30×107 | 0.0038 | [3][4] |
Copper | 1.68×10−8 | 5.96×107 | 0.0039 | [4] |
Annealed copper[note 2] | 1.72×10−8 | 5.80×107 | ||
Gold[note 3] | 2.44×10−8 | 4.10×107 | 0.0034 | [3] |
Aluminium[note 4] | 2.82×10−8 | 3.5×107 | 0.0039 | [3] |
Calcium | 3.36×10−8 | 2.98×107 | 0.0041 | |
Tungsten | 5.60×10−8 | 1.79×107 | 0.0045 | [3] |
Zinc | 5.90×10−8 | 1.69×107 | 0.0037 | [5] |
Nickel | 6.99×10−8 | 1.43×107 | 0.006 | |
Lithium | 9.28×10−8 | 1.08×107 | 0.006 | |
Iron | 1.0×10−7 | 1.00×107 | 0.005 | [3] |
Platinum | 1.06×10−7 | 9.43×106 | 0.00392 | [3] |
Tin | 1.09×10−7 | 9.17×106 | 0.0045 | |
Lead | 2.2×10−7 | 4.55×106 | 0.0039 | [3] |
Titanium | 4.20×10−7 | 2.38×106 | X | |
Manganin | 4.82×10−7 | 2.07×106 | 0.000002 | [6] |
Constantan | 4.9×10−7 | 2.04×106 | 0.000008 | [7] |
Stainless steel[note 5] | 6.9×10−7 | 1.45×106 | [8] | |
Mercury | 9.8×10−7 | 1.02×106 | 0.0009 | [6] |
Nichrome[note 6] | 1.10×10−6 | 9.09×105 | 0.0004 | [3] |
Carbon (amorphous) | 5×10−4 to 8×10−4 | 1.25 to 2×103 | −0.0005 | [3][9] |
Carbon (graphite)[note 7] | 2.5e×10−6 to 5.0×10−6 ⊥basal plane 3.0×10−3 //basal plane |
2 to 3×105 ⊥basal plane 3.3×102 //basal plane |
[10] | |
Carbon (diamond)[note 8] | 1×1012 | ~10−13 | [11] | |
Germanium[note 8] | 4.6×10−1 | 2.17 | −0.048 | [3][4] |
Sea water[note 9] | 2×10−1 | 4.8 | [12] | |
Drinking water[note 10] | 2×101 to 2×103 | 5×10−4 to 5×10−2 | ||
Deionized water[note 11] | 1.8×105 | 5.5×10−6 | [13] | |
Silicon[note 8] | 6.40×102 | 1.56×10−3 | −0.075 | [3] |
GaAs | 5×10−7 to 10×10−3 | 5×10−8 to 103 | [14] | |
Glass | 10×1010 to 10×1014 | 10−11 to 10−15 | ? | [3][4] |
Hard rubber | 1×1013 | 10−14 | ? | [3] |
Sulfur | 1×1015 | 10−16 | ? | [3] |
Air | 1.3×1016 to 3.3×1016 | 3 to 8×10−15 | [15] | |
Paraffin | 1×1017 | 10−18 | ? | |
Fused quartz | 7.5×1017 | 1.3×10−18 | ? | [3] |
PET | 10×1020 | 10−21 | ? | |
Teflon | 10×1022 to 10×1024 | 10−25 to 10−23 | ? |
The effective temperature coefficient varies with temperature and purity level of the material. The 20 °C value is only an approximation when used at other temperatures. For example, the coefficient becomes lower at higher temperatures for copper, and the value 0.00427 is commonly specified at 0 °C.[16]
The extremely low resistivity (high conductivity) of silver is characteristic of metals. George Gamow tidily summed up the nature of the metals' dealings with electrons in his science-popularizing book, One, Two, Three...Infinity (1947): "The metallic substances differ from all other materials by the fact that the outer shells of their atoms are bound rather loosely, and often let one of their electrons go free. Thus the interior of a metal is filled up with a large number of unattached electrons that travel aimlessly around like a crowd of displaced persons. When a metal wire is subjected to electric force applied on its opposite ends, these free electrons rush in the direction of the force, thus forming what we call an electric current." More technically, the free electron model gives a basic description of electron flow in metals.
The electrical resistivity of most materials changes with temperature. If the temperature T does not vary too much, a linear approximation is typically used:
where is called the temperature coefficient of resistivity, is a fixed reference temperature (usually room temperature), and is the resistivity at temperature . The parameter is an empirical parameter fitted from measurement data. Because the linear approximation is only an approximation, is different for different reference temperatures. For this reason it is usual to specify the temperature that was measured at with a suffix, such as , and the relationship only holds in a range of temperatures around the reference.[17] When the temperature varies over a large temperature range, the linear approximation is inadequate and a more detailed analysis and understanding should be used.
In general, electrical resistivity of metals increases with temperature. Electron–phonon interactions can play a key role. At high temperatures, the resistance of a metal increases linearly with temperature. As the temperature of a metal is reduced, the temperature dependence of resistivity follows a power law function of temperature. Mathematically the temperature dependence of the resistivity ρ of a metal is given by the Bloch–Grüneisen formula:
where is the residual resistivity due to defect scattering, A is a constant that depends on the velocity of electrons at the Fermi surface, the Debye radius and the number density of electrons in the metal. is the Debye temperature as obtained from resistivity measurements and matches very closely with the values of Debye temperature obtained from specific heat measurements. n is an integer that depends upon the nature of interaction:
If more than one source of scattering is simultaneously present, Matthiessen's Rule (first formulated by Augustus Matthiessen in the 1860s) [18][19] says that the total resistance can be approximated by adding up several different terms, each with the appropriate value of n.
As the temperature of the metal is sufficiently reduced (so as to 'freeze' all the phonons), the resistivity usually reaches a constant value, known as the residual resistivity. This value depends not only on the type of metal, but on its purity and thermal history. The value of the residual resistivity of a metal is decided by its impurity concentration. Some materials lose all electrical resistivity at sufficiently low temperatures, due to an effect known as superconductivity.
An investigation of the low-temperature resistivity of metals was the motivation to Heike Kamerlingh Onnes's experiments that led in 1911 to discovery of superconductivity. For details see History of superconductivity.
In general, resistivity of intrinsic semiconductors decreases with increasing temperature. The electrons are bumped to the conduction energy band by thermal energy, where they flow freely and in doing so leave behind holes in the valence band which also flow freely. The electric resistance of a typical intrinsic (non doped) semiconductor decreases exponentially with the temperature:
An even better approximation of the temperature dependence of the resistivity of a semiconductor is given by the Steinhart–Hart equation:
where A, B and C are the so-called Steinhart–Hart coefficients.
This equation is used to calibrate thermistors.
Extrinsic (doped) semiconductors have a far more complicated temperature profile. As temperature increases starting from absolute zero they first decrease steeply in resistance as the carriers leave the donors or acceptors. After most of the donors or acceptors have lost their carriers the resistance starts to increase again slightly due to the reducing mobility of carriers (much as in a metal). At higher temperatures it will behave like intrinsic semiconductors as the carriers from the donors/acceptors become insignificant compared to the thermally generated carriers.[20]
In non-crystalline semiconductors, conduction can occur by charges quantum tunnelling from one localised site to another. This is known as variable range hopping and has the characteristic form of , where n=2,3,4 depending on the dimensionality of the system.
When analyzing the response of materials to alternating electric fields, in applications such as electrical impedance tomography,[21] it is necessary to replace resistivity with a complex quantity called impeditivity (in analogy to electrical impedance). Impeditivity is the sum of a real component, the resistivity, and an imaginary component, the reactivity (in analogy to reactance). The magnitude of Impeditivity is the square root of sum of squares of magnitudes of resistivity and reactivity.
Conversely, in such cases the conductivity must be expressed as a complex number (or even as a matrix of complex numbers, in the case of anisotropic materials) called the admittivity. Admittivity is the sum of a real component called the conductivity and an imaginary component called the susceptivity.
An alternative description of the response to alternating currents uses a real (but frequency-dependent) conductivity, along with a real permittivity. The larger the conductivity is, the more quickly the alternating-current signal is absorbed by the material (i.e., the more opaque the material is). For details, see Mathematical descriptions of opacity.
In some applications where the weight of an item is very important resistivity density products are more important than absolute low resistivity- it is often possible to make the conductor thicker to make up for a higher resistivity; and then a low resistivity density product material (or equivalently a high conductance to density ratio) is desirable. For example, for long distance overhead power lines— aluminium is frequently used rather than copper because it is lighter for the same conductance.
Material | Resistivity (nΩ·m) | Density (g/cm3) | Resistivity-density product (nΩ·m·g/cm3) |
---|---|---|---|
Sodium | 47.7 | 0.97 | 46 |
Lithium | 92.8 | 0.53 | 49 |
Calcium | 33.6 | 1.55 | 52 |
Potassium | 72.0 | 0.89 | 64 |
Beryllium | 35.6 | 1.85 | 66 |
Aluminium | 26.50 | 2.70 | 72 |
Magnesium | 43.90 | 1.74 | 76.3 |
Copper | 16.78 | 8.96 | 150 |
Silver | 15.87 | 10.49 | 166 |
Gold | 22.14 | 19.30 | 427 |
Iron | 96.1 | 7.874 | 757 |
Silver, although it is the least resistive metal known, has a high density and does poorly by this measure. Calcium and the alkali metals make for the best products, but are rarely used for conductors due to their high reactivity with water and oxygen. Aluminium is far more stable. And the most important attribute, the current price, excludes the best choice: Beryllium.