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What is Density – Physics – Definition

What is density. In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. Material Properties

What is Density

Density - Gas - Liquid - Solid
Typical densities of various substances at atmospheric pressure.

Densityis defined as themass per unit volume.It is anintensive property, which is mathematically defined as mass divided by volume:

ρ = m/V

In words, the density (ρ) of a substance is the total mass (m) of that substance divided by the total volume (V) occupied by that substance. The standard SI unit iskilograms per cubic meter(kg/m3). The Standard English unit ispounds mass per cubic foot(lbm/ft3). The density (ρ) of a substance is the reciprocal of itsspecific volume(ν).

ρ = m/V = 1/ρ

Specific volumeis anintensive variable, whereas volume is an extensive variable. The standard unit for specific volume in the SI system is cubic meters per kilogram (m3/kg). The standard unit in the English system is cubic feet per pound mass (ft3/lbm).

Changes of Density
In general,densitycan bechangedby changing either thepressureor thetemperature.Increasing thepressure always increasesthedensityof a material. The effect of pressure on the densities ofliquidsandsolidsis very very small. On the other hand, the density of gases is strongly affected by pressure. This is expressed bycompressibilityCompressibilityis a measure of the relative volume change of a fluid or solid as a response to a pressure change.

Theeffect of temperatureon the densities of liquids and solids is also very important. Most substancesexpand when heatedandcontract when cooled.However, the amount of expansion or contraction varies, depending on the material. This phenomenon is known asthermal expansion.The change in volume of a material which undergoes a temperature change is given by following relation:

thermal-expansion

where ∆T is the change in temperature, V is the original volume, ∆V is the change in volume, andαVis thecoefficient of volume expansion

It must be noted, there are exceptions from this rule. For example,waterdiffers from most liquids in that it becomesless dense as it freezes.It has a maximum of density at 3.98 °C (1000 kg/m3), whereas the density of ice is 917 kg/m3.It differs by about 9% and thereforeice floatson liquid water

Coolant acceleration in a reactor core
See also:Fluid Acceleration – Pressure Loss

It is an illustrative example, following data do not correspond to any reactor design.

Continuity Equation - Flow Rates through Reactor
Example of flow rates in a reactor. It is an illustrative example, data do not represent any reactor design.

Pressurized water reactorsare cooled andmoderatedby high-pressure liquid water (e.g. 16MPa).At this pressure water boils at approximately 350°C (662°F). Inlet temperature of the water is about 290°C (⍴ ~ 720 kg/m3). The water (coolant) is heated in thereactor coreto approximately 325°C (⍴ ~ 654 kg/m3) as the water flows through the core.

The primary circuit of typical PWRs is divided into 4 independent loops (piping diameter ~ 700mm), each loop comprises asteam generatorand onemain coolant pump.Inside the reactor pressure vessel (RPV), the coolant first flows down outside the reactor core (through the downcomer). From the bottom of the pressure vessel, the flow is reversed up through the core, where thecoolant temperature increasesas it passes through the fuel rods and the assemblies formed by them.

Calculate:

  • Pressure loss due to thecoolant accelerationin an isolated fuel channel

when

  • channel inletflow velocity is equal to 5.17 m/s
  • channel outletflow velocity is equal to 5.69 m/s

Solution:

The pressure loss due to the coolant acceleration in an isolated fuel channel is then:

coolant acceleration - example

This fact has important consequences. Due to the different relative power of fuel assemblies in a core, these fuel assemblies havedifferent hydraulic resistanceand this may induce local lateral flow of primary coolant and it must be considered in thermal-hydraulic calculations.

See also:How density influences reactor reactivity

Densest Materials on the Earth

Sincenucleons(protonsandneutrons) make up most of the mass of ordinary atoms, the density of normal matter tends to be limited by how closely we can pack these nucleons and depends on the internal atomic structure of a substance. Thedensest materialfound on earth is themetal osmium, but its density pales by comparison to the densities of exotic astronomical objects such as whitedwarf starsandneutron stars

List of densest materials:

  1. Osmium – 22.6 x 103kg/m3
  2. Iridium – 22.4 x 103kg/m3
  3. Platinum – 21.5 x 103kg/m3
  4. Rhenium – 21.0 x 103kg/m3
  5. Plutonium – 19.8 x 103kg/m3
  6. 金- 19.3 x 103kg/m3
  7. Tungsten – 19.3 x 103kg/m3
  8. Uranium – 18.8 x 103kg/m3
  9. Tantalum – 16.6 x 103kg/m3
  10. Mercury – 13.6 x 103kg/m3
  11. Rhodium – 12.4 x 103kg/m3
  12. Thorium – 11.7 x 103kg/m3
  13. Lead – 11.3 x 103kg/m3
  14. Silver – 10.5 x 103kg/m3

It must be noted, plutonium is a man-made isotope and is created fromuraniuminnuclear reactors.But, In fact, scientists have found trace amounts of naturally-occurring plutonium.

If we include man made elements, the densest so far isHassiumHassiumis a chemical element with symbolHsand atomic number 108. It is a synthetic element (first synthesised at Hasse in Germany) and radioactive. The most stable known isotope,269Hs, has a half-life of approximately 9.7 seconds. It has an estimated density of40.7 x 103kg/m3.The density of Hassium results from itshigh atomic weightand from the significant decrease inionic radiiof the elements in the lanthanide series, known aslanthanide and actinide contraction

The density of Hassium is followed byMeitnerium(element 109, named after the physicist Lise Meitner), which has an estimated density of37.4 x 103kg/m3

Density - Important property in gamma rays shielding
See also:Shielding of Gamma Radiation

In short, effective shielding of gamma radiation is in most cases based on use of materials with two following material properties:

  • high-density of material.
  • high atomic number of material (high Z materials)

However, low-density materials and low Z materials can be compensated with increased thickness, which is as significant as density and atomic number in shielding applications.

A lead is widely used as a gamma shield. Major advantage of lead shield is in its compactness due to its higher density. On the other handdepleted uraniumis much more effective due to its higher Z. Depleted uranium is used for shielding in portable gamma ray sources.

Innuclear power plantsshielding of areactor corecan be provided by materials of reactor pressure vessel, reactor internals (neutron reflector). Also heavy concrete is usually used to shield bothneutronsand gamma radiation.

Density of various Materials – Examples

水的密度,具体体积
水的密度,具体体积Pure water has its highest density1000 kg/m3at temperature3.98o C(39.2 o F).Water differs from most liquids in that it becomesless dense as it freezes.It has a maximum of density at 3.98 °C (1000 kg/m3), whereas the density of ice is 917 kg/m3.It differs by about 9% and thereforeice floatson liquid water. It must be noted, the change in density is not linear with temperature, because the volumetric thermal expansion coefficient for water is not constant over the temperature range. The density of water (1 gram per cubic centimetre) was originally used to define the gram. The density (⍴) of a substance is the reciprocal of its specific volume (ν).

ρ = m/V = 1/ν

具体的体积(ν)的一种物质是完全的l volume (V) of that substance divided by the total mass (m) of that substance (volume per unit mass). It has units of cubic meter per kilogram (m3/kg).

Density of Heavy Water
Pureheavy water(D2O) has a density about11% greater than water, but is otherwise physically and chemically similar.

This difference is caused by the fact, thedeuteriumnucleus istwice as heavy as hydrogennucleus. Since about 89% of the molecular weight of water comes from the single oxygen atom rather than the two hydrogen atoms, the weight of a heavy water molecule, is not substantially different from that of a normal water molecule. The molar mass of water is M(H2O) = 18.02 and the molar mass of heavy water is M(D2O) = 20.03 (each deuterium nucleus contains one neutron in contrast to hydrogen nucleus), therefore heavy water (D2O) has a density about 11% greater (20.03/18.03 = 1.112).

Pureheavy water(D2O) has itshighest density1110 kg/m3at temperature3.98oC(39.2oF).Also heavy water differs from most liquids in that it becomesless dense as it freezes.It has a maximum of density at 3.98 °C (1110 kg/m3), whereas the density of its solid form ice is 1017 kg/m3.必须指出,密度的变化不是linear with temperature, because the volumetric thermal expansion coefficient for water is not constant over the temperature range.

Density of Steam
steam properties - steam tablesWater and steam are a common medium because their properties are verywell known.Their properties are tabulated in so called Steam Tables .In these tables the basic and key properties, such as pressure, temperature, enthalpy,densityand specific heat, are tabulated along the vapor-liquid saturation curve as a function of both temperature and pressure.

The density (⍴) of any substance is the reciprocal of its specific volume ().

ρ = m/V = 1/

The specific volume () of a substance is the total volume (V) of that substance divided by the total mass (m) of that substance (volume per unit mass). It has units of cubic meter per kilogram (m3/kg).

Density of Steel
The density of steel varies based on the alloying constituents but usually ranges between 7.5 x 103kg/m3and 8 x 103kg/m3
Density of Zirconium
In general, zirconium has very lowabsorption cross-sectionof thermal neutrons, high hardness, ductility and corrosion resistance. One of the main uses of zirconium alloys is in nuclear technology, as cladding of fuel rods in nuclear reactors, due to its very lowabsorption cross-section(unlike the stainless steel). The density of typical zirconium alloy is about 6.6 x 103kg/m3
Density of Uranium
Uraniumis a naturally-occurring chemical element with atomic number 92 which means there are 92 protons and 92 electrons in theatomic structureNatural uraniumconsists primarily of isotope238U(99.28%), therefore the atomic mass of uranium element is close to the atomic mass of238U isotope (238.03u). Natural uranium also consists of two other isotopes:235U(0.71%) and234U(0.0054%). Uranium has the highest atomic weight of the primordially occurring elements. Uranium metal has a very high density of19.1 g/cm3, denser than lead (11.3 g/cm3), but slightly less dense than tungsten and gold (19.3 g/cm3).

Uranium metal is one of the densest materials found on earth:

  1. Osmium – 22.6 x 103kg/m3
  2. Iridium – 22.4 x 103kg/m3
  3. Platinum – 21.5 x 103kg/m3
  4. Rhenium – 21.0 x 103kg/m3
  5. Plutonium – 19.8 x 103kg/m3
  6. 金- 19.3 x 103kg/m3
  7. Tungsten – 19.3 x 103kg/m3
  8. Uranium – 18.8 x 103kg/m3
  9. Tantalum – 16.6 x 103kg/m3
  10. Mercury – 13.6 x 103kg/m3
  11. Rhodium – 12.4 x 103kg/m3
  12. Thorium – 11.7 x 103kg/m3
  13. Lead – 11.3 x 103kg/m3
  14. Silver – 10.5 x 103kg/m3

But most ofLWRsuse theuranium fuel, which is in the form ofuranium dioxide.Uranium dioxide is a black semiconducting solid with very low thermal conductivity. On the other hand the uranium dioxide has very high melting point and has well known behavior.

Uranium dioxide has significantly lower density than uranium in the metal form. Uranium dioxide has a density of10.97 g/cm3, but this value may vary with fuel burnup, because at low burnup densification of pellets can occurs and at higher burnup swelling occurs.

Density of Nuclear Matter

Nuclear densityis the density of the nucleus of an atom. It is the ratio of mass per unit volume inside the nucleus. Since atomic nucleus carries most of atom’s mass and atomic nucleus is very small in comparison to entire atom, the nuclear density is very high.

The nuclear density for a typical nucleus can be approximately calculated from the size of the nucleus and from its mass.Typicalnuclear radiiare of the order10−14m.Assuming spherical shape, nuclear radii can be calculated according to following formula:

r = r0.A1/3

where r0= 1.2 x 10-15m = 1.2 fm

For example,natural uraniumconsists primarily of isotope238U(99.28%), therefore the atomic mass of uranium element is close to the atomic mass of238U isotope (238.03u). Its radius of this nucleus will be:

r = r0.A1/3= 7.44 fm.

Assuming it is spherical, its volume will be:

V = 4πr3/3 = 1.73 x 10-42m3

The usual definition of nuclear density gives for its density:

ρnucleus= m / V = 238 x 1.66 x 10-27/ (1.73 x 10-42) =2.3 x 1017kg/m3

Thus, the density of nuclear material is more than 2.1014times greater than that of water. It is an immense density. The descriptive termnuclear density也适用于类似的情况下高吗densities occur, such as within neutron stars. Such immense densities are also found in neutron stars.

Density of Neutron Star
The densest material found on earth is the metal osmium, but its density pales by comparison to the densities of exotic astronomical objects such as white dwarf stars and neutron stars.

Aneutron staris the collapsed core of a large star (usually of a red giant). Neutron stars are the smallest and densest stars known to exist and they arerotating extremely rapidly.A neutron star is basically a giant atomic nucleus about 11 km in diameter made especially of neutrons. It is believed that under the immense pressures of a collapsing massive stars going supernova it is possible for the electrons and protons to combine to form neutrons via electron capture, releasing a huge amount ofneutrinos

They are so dense that one teaspoon of its material would have a mass over 5.5×1012kg. It is assumed they have densities of 3.7 × 1017to 6 × 1017kg/m3, which is comparable to the approximate density of an atomic nucleus of 2.3 × 1017kg/m3

References:
Reactor Physics and Thermal Hydraulics:
  1. J. R. Lamarsh, Introduction to Nuclear Reactor Theory, 2nd ed., Addison-Wesley, Reading, MA (1983).
  2. J. R. Lamarsh, A. J. Baratta, Introduction to Nuclear Engineering, 3d ed., Prentice-Hall, 2001, ISBN: 0-201-82498-1.
  3. W. M. Stacey, Nuclear Reactor Physics, John Wiley & Sons, 2001, ISBN: 0- 471-39127-1.
  4. Glasstone, Sesonske. Nuclear Reactor Engineering: Reactor Systems Engineering, Springer; 4th edition, 1994, ISBN: 978-0412985317
  5. Todreas Neil E., Kazimi Mujid S. Nuclear Systems Volume I: Thermal Hydraulic Fundamentals, Second Edition. CRC Press; 2 edition, 2012, ISBN: 978-0415802871
  6. Zohuri B., McDaniel P. Thermodynamics in Nuclear Power Plant Systems. Springer; 2015, ISBN: 978-3-319-13419-2
  7. Moran Michal J., Shapiro Howard N. Fundamentals of Engineering Thermodynamics, Fifth Edition, John Wiley & Sons, 2006, ISBN: 978-0-470-03037-0
  8. Kleinstreuer C. Modern Fluid Dynamics. Springer, 2010, ISBN 978-1-4020-8670-0.
  9. U.S. Department of Energy, THERMODYNAMICS, HEAT TRANSFER, AND FLUID FLOW. DOE Fundamentals Handbook, Volume 1, 2 and 3. June 1992.

See also:

Thermodynamic Properties

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