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Binding energy is the energy required to disassemble a whole system into separate parts. A bound system typically has a lower potential energy than the sum of its constituent parts; this is what keeps the system together. Often this means that energy is released upon the creation of a bound state. This definition corresponds to a positive binding energy.

General idea[edit]

In general, binding energy represents the mechanical work that must be done against the forces which hold an object together, disassembling the object into component parts separated by sufficient distance that further separation requires negligible additional work.

At the atomic level the atomic binding energy of the atom derives from electromagnetic interaction and is the energy required to disassemble an atom into free electrons and a nucleus.[1] Electron binding energy is a measure of the energy required to free electrons from their atomic orbits. This is more commonly known as ionization energy.[2]

At the molecular level, bond energy and bond-dissociation energy are measures of the binding energy between the atoms in a chemical bond.

At the nuclear level, binding energy is also equal to the energy liberated when a nucleus is created from other nucleons or nuclei.[3][4] This nuclear binding energy (binding energy of nucleons into a nuclide) is derived from the nuclear force (residual strong interaction) and is the energy required to disassemble a nucleus into the same number of free, unbound neutrons and protons it is composed of, so that the nucleons are far/distant enough from each other so that the nuclear force can no longer cause the particles to interact.[5] Mass excess is a related concept which compares the mass number of a nucleus with its true measured mass.[6]

In astrophysics, the gravitational binding energy of a celestial body is the energy required to expand the material to infinity.

In bound systems, if the binding energy is removed from the system, it must be subtracted from the mass of the unbound system, simply because this energy has mass. Thus, if energy is removed (or emitted) from the system at the time it is bound, the loss of energy from the system will also result in the loss of the mass of the energy, from the system.[7] System mass is not conserved in this process because the system is "open" (i.e., is not an isolated system to mass or energy input or loss) during the binding process.

Mass-energy relation[edit]

Classically a bound system is at a lower energy level than its unbound constituents, and its mass must be less than the total mass of its unbound constituents. For systems with low binding energies, this "lost" mass after binding may be fractionally small. For systems with high binding energies, however, the missing mass may be an easily measurable fraction. This missing mass may be lost during the process of binding as energy in the form of heat or light, with the removed energy corresponding to removed mass through Einstein's equation E = mc2. Note that in the process of binding, the constituents of the system might enter higher energy states of the nucleus/atom/molecule, but these types of energy also have mass, and it is necessary that they be removed from the system before its mass may decrease. Once the system cools to normal temperatures and returns to ground states in terms of energy levels, there is less mass remaining in the system than there was when it first combined and was at high energy. In that case, the removed heat represents exactly the mass "deficit", and the heat itself retains the mass which was lost (from the point of view of the initial system). This mass appears in any other system which absorbs the heat and gains thermal energy.[8]

As an illustration, consider two objects attracting each other in space through their gravitational field. The attraction force accelerates the objects and they gain some speed toward each other converting the potential (gravity) energy into kinetic (movement) energy. When either the particles 1) pass through each other without interaction or 2) elastically repel during the collision, the gained kinetic energy (related to speed), starts to revert into potential form driving the collided particles apart. The decelerating particles will return to the initial distance and beyond into infinity or stop and repeat the collision (oscillation takes place). This shows that the system, which loses no energy, does not combine (bind) into a solid object, parts of which oscillate at short distances. Therefore, in order to bind the particles, the kinetic energy gained due to the attraction must be dissipated (by resistive force). Complex objects in collision ordinarily undergo inelastic collision, transforming some kinetic energy into internal energy (heat content, which is atomic movement), which is further radiated in the form of photons—the light and heat. Once the energy to escape the gravity is dissipated in the collision, the parts will oscillate at closer, possibly atomic, distance, thus looking like one solid object. This lost energy, necessary to overcome the potential barrier in order to separate the objects, is the binding energy. If this binding energy were retained in the system as heat, its mass would not decrease. However, binding energy lost from the system (as heat radiation) would itself have mass, and directly represents the "mass deficit" of the cold, bound system.

Closely analogous considerations apply in chemical and nuclear considerations. Exothermic chemical reactions in closed systems do not change mass, but become less massive once the heat of reaction is removed, though this mass change is much too small to measure with standard equipment. In nuclear reactions, however, the fraction of mass that may be removed as light or heat, i.e., binding energy, is often a much larger fraction of the system mass. It may thus be measured directly as a mass difference between rest masses of reactants and (cooled) products. This is because nuclear forces are comparatively stronger than the Coulombic forces associated with the interactions between electrons and protons, that generate heat in chemistry.

Mass change[edit]

Mass change (decrease) in bound systems, particularly atomic nuclei, has also been termed mass defect, mass deficit, or mass packing fraction.[citation needed]

The difference between the unbound system calculated mass and experimentally measured mass of nucleus (mass change) is denoted as Δm. It can be calculated as follows:

Mass change = (unbound system calculated mass) − (measured mass of system)
i.e., (sum of masses of protons and neutrons) − (measured mass of nucleus)

After nuclear reactions that result in an excited nucleus, the energy that must be radiated or otherwise removed as binding energy for a single nucleus to produce the unexcited state may be in any of several forms. This may be electromagnetic waves, such as gamma radiation, the kinetic energy of an ejected particle, such as an electron, in internal conversion decay, or partly as the rest mass of one or more emitted particles, such as the particles of beta decay. No mass deficit can in theory appear until this radiation or this energy has been emitted, and is no longer part of the system.

When nucleons bind together to form a nucleus, they must lose a small amount of mass, i.e., there is a change in mass, in order to stay bound. This mass change must be released as various types of photon or other particle energy as above, according to the relation E = mc2. Thus, after binding energy has been removed, binding energy = mass change × c2. This energy is a measure of the forces that hold the nucleons together, and it represents energy that must be supplied again from the environment, if the nucleus were to be broken up into individual nucleons.

The energy given off during either nuclear fusion or nuclear fission is the difference between the binding energies of the "fuel", i.e., the initial nuclide(s), and the fission or fusion products. In practice, this energy may also be calculated from the substantial mass differences between the fuel and products, which uses previous measurement of the atomic masses of known nuclides, which always have the same mass for each species. This mass difference appears once evolved heat and radiation have been removed, which is a given requirement for measuring the (rest) masses of the (non-excited) nuclides involved in such calculations.

See also[edit]

References[edit]

  1. ^ "Nuclear Power Binding Energy". Retrieved 16 May 2015. 
  2. ^ IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version:  (2006–) "Ionization energy".
  3. ^ Britannica Online Encyclopaedia - "nuclear binding energy". Accessed 8 September 2010. http://www.britannica.com/EBchecked/topic/65615/binding-energy
  4. ^ Nuclear Engineering - "Binding Energy". Bill Garland, McMaster University. Accessed 8 September 2010. http://www.nuceng.ca/igna/binding_energy.htm
  5. ^ Atomic Alchemy: Nuclear Processes - "Binding Energy". About. Accessed 7 September 2010. http://library.thinkquest.org/17940/texts/binding_energy/binding_energy.html
  6. ^ Krane, K. S (1987). Introductory Nuclear Physics. John Wiley & Sons. ISBN 0-471-80553-X. 
  7. ^ HyperPhysics - "Nuclear Binding Energy". C.R. Nave, Georgia State University. Accessed 7 September 2010. http://hyperphysics.phy-astr.gsu.edu/hbase/nucene/nucbin.html
  8. ^ E. F. Taylor and J. A. Wheeler, Spacetime Physics, W.H. Freeman and Co., NY. 1992. ISBN 0-7167-2327-1, see pp. 248-9 for discussion of mass remaining constant after detonation of nuclear bombs, until heat is allowed to escape.

External links[edit]


Original courtesy of Wikipedia: http://en.wikipedia.org/wiki/Binding_energy — Please support Wikipedia.
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569 news items

Science 2.0

Science 2.0
Fri, 24 Jul 2015 18:57:54 -0700

If you have a mixed liquid (such as salt in water), those molecules having the lowest binding energy to the liquid will evaporate first. With salt water, the salt is attracted to the water and other salt far stronger than the water molecules are ...

Phys.Org

Phys.Org
Fri, 17 Jul 2015 06:50:36 -0700

For example, the binding energy of the Earth is 2.2 x 10^32 joules. It's a lot. The binding energy of a smaller object, like our moon is a tidy little 1.2 x 10^29 joules. It takes about 1800 times more energy to destroy the Earth than it takes to ...

Nature.com

Nature.com
Thu, 23 Jul 2015 02:33:45 -0700

Owing to protocols for coating nanoparticles with organic shells and to advances in DNA synthesis, as well as to the ability to design multiple DNA 'recognition' sequences with equivalent binding energy and flexible DNA 'spacers' with varied lengths ...

The Guardian

The Guardian
Sat, 18 Jul 2015 10:35:54 -0700

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Azom.com

Azom.com
Fri, 10 Jul 2015 09:03:47 -0700

The aluminum and hafnium occur at the same approximate position, and oxygen exists in two chemical states, as indicated by the two O 1s binding energies in the XPS spectrum; the high binding energy is related to hafnium and the low binding energy is ...
 
Nature.com
Thu, 16 Jul 2015 23:22:30 -0700

Based on our measured optical gap and the previously measured electronic energy gap, we determined the exciton binding energy to be ~0.3 eV for the monolayer phosphorene on SiO2/Si substrate, which agrees well with theoretical predictions. A huge ...

Nature.com

Nature.com
Tue, 14 Jul 2015 09:18:45 -0700

The binding energy scales of the high-resolution spectra were calibrated by assigning the lowest binding energy peak a binding energy of 285.0 eV. ToF-SIMS images were acquired on a ToF-SIMS 5 spectrometer (IonToF) using a 25 keV Bi3+ cluster ion ...

Azom.com

Azom.com
Fri, 10 Jul 2015 09:15:27 -0700

Theta Probe and Theta 300 instruments from Thermo Scientific have been utilized to define very thin layers of silicon dioxide (SiO2) and silicon oxynitride on silicon by means of parallel angle resolved XPS (PARXPS) method. Comparison between PARXPS ...
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