Thermal runaway

Diagram of thermal runaway.

Thermal runaway refers to a situation where an increase in temperature changes the conditions in a way that causes a further increase in temperature, often leading to a destructive result. It is a kind of uncontrolled positive feedback.

In other words, "thermal runaway" describes a process which is accelerated by increased temperature, in turn releasing energy that further increases temperature. In chemistry (and chemical engineering), this risk is associated with strongly exothermic reactions that are accelerated by temperature rise. In electrical engineering, thermal runaway is typically associated with increased current flow and power dissipation, although exothermic chemical reactions can be of concern here too. Thermal runaway can occur in civil engineering, notably when the heat released by large amounts of curing concrete is not controlled. In astrophysics, runaway nuclear fusion reactions in stars can lead to nova and several types of supernova explosions, and also occur as a less dramatic event in the normal evolution of solar mass stars, the "helium flash".

There are also concerns regarding global warming that a global average increase of 3-4 degrees Celsius above the preindustrial baseline could lead to a further unchecked increase in surface temperatures. For example, releases of methane, a greenhouse gas more potent than CO2, from wetlands, melting permafrost and continental margin seabed clathrate deposits could be subject to positive feedback.[1][2]

Chemical engineering

See also: Fire

In chemical engineering, thermal runaway is also called thermal explosion, that is a process by which an exothermic reaction goes out of control, often resulting in an explosion. It is also known as a runaway reaction in organic chemistry.

Thermal explosion occurs when the reaction rate increases due to an increase in temperature, causing a further increase in temperature and hence a further rapid increase in the reaction rate. It has contributed to industrial chemical accidents, most notably the 1947 Texas City disaster from overheated ammonium nitrate in a ship's hold, and the disastrous release of a large volume of methyl isocyanate gas from a Union Carbide plant in Bhopal, India in 1984.

Most chemical reactions produce some heat, so many industrial-scale and oil refinery processes have some level of risk of thermal runaway. These include hydrocracking, hydrogenation, alkylation (SN2), oxidation, metalation and nucleophilic aromatic substitution. For example, oxidation of cyclohexane into cyclohexanol and cyclohexanone and ortho-xylene into phthalic anhydride have led to catastrophic explosions when reaction control failed.

Thermal runaway may result from unwanted exothermic side reaction(s) that begin at higher temperatures, following an initial accidental overheating of the reaction mixture. This scenario was behind the Seveso disaster, where thermal runaway heated a reaction to temperatures such that in addition to the intended 2,4,5-trichlorophenol, poisonous 2,3,7,8-tetrachlorodibenzo-p-dioxin was also produced, and was vented into the environment after the reactor's rupture disk burst.[3]

Thermal runaway is most often caused by failure of the reactor vessel's cooling system. Failure of the mixer can result in localized heating, which initiates thermal runaway. Similarly, in flow reactors, localized insufficient mixing causes hotspots to form, wherein thermal runaway conditions occur, which causes violent blowouts of reactor contents and catalysts. Incorrect equipment component installation is also a common cause. Many chemical production facilities are designed with high-volume emergency venting, a measure to limit the extent of injury and property damage when such accidents occur.

At large scale, it is unsafe to "charge all reagents and mix", as is done in laboratory scale. This is because the amount of reaction scales with the cube of the size of the vessel (V ∝ r³), but the heat transfer area scales with the square of the size (A ∝ r²), so that the heat production-to-area ratio scales with the size (V/A ∝ r). Consequently, reactions that easily cool fast enough in the laboratory can dangerously self-heat at ton scale. In 2007, this kind of erroneous procedure caused an explosion of a 2,400 U.S. gallons (9,100 L)-reactor used to metalate methylcyclopentadiene with metallic sodium, causing the loss of four lives and parts of the reactor being flung 400 feet (120 m) away.[4][5] Thus, industrial scale reactions prone to thermal runaway are preferably controlled by the addition of one reagent at a rate corresponding to the available cooling capacity.

Some laboratory reactions must be run under extreme cooling, because they are very prone to hazardous thermal runaway. For example, in Swern oxidation, the formation of sulfonium chloride must be performed in a cooled system (–30 °C), because at room temperature the reaction undergoes explosive thermal runaway.[5]

The UK Chemical Reaction Hazards Forum[6] publishes analysis of previously-unreported chemical accidents to assist the education of the scientific and engineering community, with the aim of preventing similar occurrences elsewhere. Almost 150 such reports are available to view as of January 2009.

Microwave heating

Microwaves are used for heating of various materials in cooking and various industrial processes. The rate of heating of the material depends on the energy absorption, which depends on the dielectric constant of the material. The dependence of dielectric constant on temperature varies for different materials; some materials display significant increase with increasing temperature. This behavior, when the material gets exposed to microwaves, leads to selective local overheating, as the warmer areas are better able to accept further energy than the colder areas—potentially dangerous especially for thermal insulators, where the heat exchange between the hot spots and the rest of the material is slow. These materials are called thermal runaway materials. This phenomenon occurs in some ceramics.

Electrical engineering

Some electronic components develop lower resistances or lower triggering voltages (for nonlinear resistances) as their internal temperature increases. If circuit conditions cause markedly increased current flow in these situations, increased power dissipation may raise the temperature further by Joule heating. A vicious circle or positive feedback effect of thermal runaway can cause failure, sometimes in a spectacular fashion (e.g. electrical explosion or fire). To prevent these hazards, well-designed electronic systems typically incorporate current limiting protection, such as thermal fuses, circuit breakers, or PTC current limiters.

To handle larger currents, circuit designers may connect multiple lower-capacity devices (e.g. transistors, diodes, or MOVs) in parallel. This technique can work well, but is susceptible to a phenomenon called current hogging, in which the current is not shared equally across all devices. Typically, one device may have a slightly lower resistance, and thus draws more current, heating it more than its sibling devices, causing its resistance to drop further. The electrical load ends up funneling into a single device, which then rapidly fails. Thus, an array of devices may end up no more robust than its weakest component.

The current-hogging effect can be reduced by carefully matching the characteristics of each paralleled device, or by using other design techniques to balance the electrical load. However, maintaining load balance under extreme conditions may not be straightforward. Devices with an intrinsic positive temperature coefficient (PTC) of electrical resistance are less prone to current hogging, but thermal runaway can still occur because of poor heat sinking or other problems.

Many electronic circuits contain special provisions to prevent thermal runaway. This is most often seen in transistor biasing arrangements for high-power output stages. However, when equipment is used above its designed ambient temperature, thermal runaway can still occur in some cases. This occasionally causes equipment failures in hot environments, or when air cooling vents are blocked.

Semiconductors

Silicon shows a peculiar profile, in that its electrical resistance increases with temperature up to about 160 °C, then starts decreasing, and drops further when the melting point is reached. This can lead to thermal runaway phenomena within internal regions of the semiconductor junction; the resistance decreases in the regions which become heated above this threshold, allowing more current to flow through the overheated regions, in turn causing yet more heating in comparison with the surrounding regions, which leads to further temperature increase and resistance decrease. This leads to the phenomenon of current crowding and formation of current filaments (similar to current hogging, but within a single device), and is one of the underlying causes of many semiconductor junction failures.

Bipolar junction transistors (BJTs)

Leakage current increases significantly in bipolar transistors (especially germanium-based bipolar transistors) as they increase in temperature. Depending on the design of the circuit, this increase in leakage current can increase the current flowing through a transistor and thus the power dissipation, causing a further increase in collector-to-emitter leakage current. This is frequently seen in a push–pull stage of a class AB amplifier. If the pull-up and pull-down transistors are biased to have minimal crossover distortion at room temperature, and the biasing is not temperature-compensated, then as the temperature rises both transistors will be increasingly biased on, causing current and power to further increase, and eventually destroying one or both devices.

One rule of thumb to avoid thermal runaway is to keep the operating point of a BJT so that Vce ≤ 1/2Vcc

Another practice is to mount a thermal feedback sensing transistor or other device on the heat sink, to control the crossover bias voltage. As the output transistors heat up, so does the thermal feedback transistor. This in turn causes the thermal feedback transistor to turn on at a slightly lower voltage, reducing the crossover bias voltage, and so reducing the heat dissipated by the output transistors.

If multiple BJT transistors are connected in parallel (which is typical in high current applications), a current hogging problem can occur. Special measures must be taken to control this characteristic vulnerability of BJTs.

In power transistors (which effectively consist of many small transistors in parallel), current hogging can occur between different parts of the transistor itself, with one part of the transistor becoming more hot than the others. This is called second breakdown, and can result in destruction of the transistor even when the average junction temperature seems to be at a safe level.

Power MOSFETs

Power MOSFETs typically increase their on-resistance with temperature. Under some circumstances, power dissipated in this resistance causes more heating of the junction, which further increases the junction temperature, in a positive feedback loop. As a consequence, power MOSFETs have stable and instable regions of operation.[7] However, the increase of on-resistance with temperature helps balance current across multiple MOSFETs connected in parallel, so current hogging does not occur. If a MOSFET transistor produces more heat than the heatsink can dissipate, then thermal runaway can still destroy the transistors. This problem can be alleviated to a degree by lowering the thermal resistance between the transistor die and the heatsink. See also Thermal Design Power.

Metal oxide varistors (MOVs)

Metal oxide varistors typically develop lower resistance as they heat up. If connected directly across an AC or DC power bus (a common usage for protection against electrical transients), a MOV which has developed a lowered trigger voltage can slide into catastrophic thermal runaway, possibly culminating in a small explosion or fire.[8] To prevent this possibility, fault current is typically limited by a thermal fuse, circuit breaker, or other current limiting device.

Tantalum capacitors

Tantalum capacitors are under some conditions prone to self-destruction by thermal runaway. The capacitor typically consists of a sintered tantalum sponge acting as the anode, a manganese dioxide cathode, and a dielectric layer of tantalum pentoxide created on the tantalum sponge surface by anodizing. It may happen that the tantalum oxide layer has weak spots that undergo dielectric breakdown during a voltage spike. The tantalum sponge then comes into direct contact with the manganese dioxide, and increased leakage current causes localized heating; usually, this drives an endothermic chemical reaction that produces manganese(III) oxide and regenerates (self-heals) the tantalum oxide dielectric layer.

However, if the energy dissipated at the failure point is high enough, a self-sustaining exothermic reaction can start, similar to the thermite reaction, with metallic tantalum as fuel and manganese dioxide as oxidizer. This undesirable reaction will destroy the capacitor, producing smoke and possibly flame.[9]

Therefore, tantalum capacitors can be freely deployed in small-signal circuits, but application in high-power circuits must be carefully designed to avoid thermal runaway failures.

Digital logic

The leakage current of logic switching transistors increases with temperature. In rare instances, this may lead to thermal runaway in digital circuits. This is not a common problem, since leakage currents usually make up a small portion of overall power consumption, so the increase in power is fairly modest — for an Athlon 64, the power dissipation increases by about 10% for every 30 degrees Celsius.[10] For a device with a TDP of 100 W, for thermal runaway to occur, the heat sink would have to have a thermal resistivity of over 3 K/W (kelvins per watt), which is about 6 times worse than a stock Athlon 64 heat sink. (A stock Athlon 64 heat sink is rated at 0.34 K/W, although the actual thermal resistance to the environment is somewhat higher, due to the thermal boundary between processor and heatsink, rising temperatures in the case, and other thermal resistances..) Regardless, an inadequate heat sink with a thermal resistance of over 0.5 to 1 K/W would result in the destruction of a 100 W device even without thermal runaway effects.

Batteries

When handled improperly, or if manufactured defectively, some rechargeable batteries can experience thermal runaway resulting in overheating. Sealed cells will sometimes explode violently if safety vents are overwhelmed or nonfunctional.[11] Especially prone to thermal runaway are lithium-ion batteries, most markedly in the form of the lithium polymer battery. Reports of exploding cellphones occasionally appear in newspapers. In 2006, batteries from Apple, HP, Toshiba, Lenovo, Dell and other notebook manufacturers were recalled because of fire and explosions.[12][13][14][15] The Pipeline and Hazardous Materials Safety Administration (PHMSA) of the U.S. Department of Transportation has established regulations regarding the carrying of certain types of batteries on airplanes because of their instability in certain situations. This action was partially inspired by a cargo bay fire on a UPS airplane.[16] One of the possible solutions is in using safer and less reactive anode (lithium titanates) and cathode (lithium iron phosphate) materials — avoiding the cobalt electrodes in many lithium rechargeable cells — together with non-flammable electrolytes based on ionic liquids.

Astrophysics

Runaway thermonuclear reactions can occur in stars when nuclear fusion is ignited in conditions under which the pressure exerted by overlying layers of the star greatly exceeds thermal pressure, a situation that makes possible rapid increases in temperature. Such a scenario may arise in stars containing degenerate matter, in which electron degeneracy pressure rather than normal thermal pressure does most of the work of supporting the star against gravity, and in stars undergoing implosion. In all cases, the imbalance arises prior to fusion ignition; otherwise, the fusion reactions would be naturally regulated to counteract temperature changes and stabilize the star. When thermal pressure is in equilibrium with overlying pressure, a star will respond to the increase in temperature and thermal pressure due to initiation of a new exothermic reaction by expanding and cooling. A runaway reaction is only possible when this response is inhibited.

Helium flashes in red giant stars

When stars in the 0.8-2.0 solar mass range exhaust the hydrogen in their cores and become red giants, the helium accumulating in their cores reaches degeneracy before it ignites. When the degenerate core reaches a critical mass of about 0.45 solar masses, helium fusion is ignited and takes off in a runaway fashion, called the helium flash, briefly increasing the star's energy production to a rate 100 billion times normal. About 6% of the core is quickly converted into carbon.[17] While the release is sufficient to convert the core back into normal plasma after a few seconds, it does not disrupt the star,[18][19] nor immediately change its luminosity. The star then contracts, leaving the red giant phase and continuing its evolution into a stable helium-burning phase.

Novae

A nova results from runaway hydrogen fusion (via the CNO cycle) in the outer layer of a carbon-oxygen white dwarf star. If a white dwarf has a companion star from which it can accrete gas, the material will accumulate in a surface layer made degenerate by the dwarf's intense gravity. Under the right conditions, a sufficiently thick layer of hydrogen is eventually heated to a temperature of 20 million K, igniting runaway fusion. The surface layer is blasted off the white dwarf, increasing luminosity by a factor on the order of 50,000. The white dwarf and companion remain intact, however, so the process can repeat.[20] A much rarer type of nova may occur when the outer layer that ignites is composed of helium.[21]

X-ray bursts

Analogous to the process leading to novae, degenerate matter can also accumulate on the surface of a neutron star that is accreting gas from a close companion. If a sufficiently thick layer of hydrogen accumulates, ignition of runaway hydrogen fusion can then lead to an X-ray burst. As with novae, such bursts tend to repeat and may also be triggered by helium or even carbon fusion.[22][23] It has been proposed that in the case of "superbursts", runaway breakup of accumulated heavy nuclei into iron group nuclei via photodissociation rather than nuclear fusion could contribute the majority of the energy of the burst.[23]

Type Ia supernovae

A type Ia supernova results from runaway carbon fusion in the core of a carbon-oxygen white dwarf star. If a white dwarf, which is composed almost entirely of degenerate matter, can gain mass from a companion, the increasing temperature and density of material in its core will ignite carbon fusion if the star's mass approaches the Chandrasekhar limit. This leads to an explosion that completely disrupts the star. Luminosity increases by a factor of greater than 5 billion. One way to gain the additional mass would be by accreting gas from a giant star (or even main sequence) companion.[24] A second and apparently more common mechanism to generate the same type of explosion is the merger of two white dwarfs.[24][25]

Pair-instability supernovae

A pair-instability supernova is believed to result from runaway oxygen fusion in the core of a massive, 130-250 solar mass, low to moderate metallicity star.[26] According to theory, in such a star, a large but relatively low density core of nonfusing oxygen builds up, with its weight supported by the pressure of gamma rays produced by the extreme temperature. As the core heats further, the gamma rays eventually begin to pass the energy threshold needed for collision-induced decay into electron-positron pairs, a process called pair production. This causes a drop in the pressure within the core, leading it to contract and heat further, causing more pair production, a further pressure drop, and so on. The core starts to undergo gravitational collapse. At some point this ignites runaway oxygen fusion, releasing enough energy to obliterate the star. These explosions are rare, perhaps about one per 100,000 supernovae.

Comparison to nonrunaway supernovae

Not all supernovae are triggered by runaway nuclear fusion. Type Ib, Ic and type II supernovae also undergo core collapse, but because they have exhausted their supply of atomic nuclei capable of undergoing exothermic fusion reactions, they collapse all the way into neutron stars, or in the higher-mass cases, stellar black holes, powering explosions by the release of gravitational potential energy. It is the absence of runaway fusion reactions that allows such supernovae to leave behind compact stellar remnants.

See also

References

  1. ↑ Clark, P.U.; et al. (December 2008). "Executive Summary". Abrupt Climate Change. A Report by the U.S. Climate Change Science Program and the Subcommittee on Global Change Research. Reston, Virginia, USA: U.S. Geological Survey., pp. 163–201. Report website
  2. ↑ IMPACTS: On the Threshold of Abrupt Climate Changes, Lawrence Berkeley National Laboratory News Center, 17 September 2008
  3. ↑ Kletz, Trevor A. (2001). Learning from Accidents (3rd ed.). Oxford U.K.: Gulf Professional. pp. 103–9. ISBN 978-0-7506-4883-7.
  4. ↑ Lowe, Derek (2009-09-18). "175 Times. And Then the Catastrophe". Corante. Archived from the original on 2015-03-20. Retrieved 16 April 2016.
  5. 1 2 Lowe, Derek (2008-04-30). "How Not To Do It: Diazomethane". Science Translational Magazine. American Association for the Advancement of Science. Retrieved 16 April 2016.
  6. ↑ UK Chemical Reaction Hazards Forum
  7. ↑ Ferrara, A.; Steeneken, P. G.; Boksteen, B. K.; Heringa, A.; Scholten, A. J.; Schmitz, J.; Hueting, R. J. E. (November 2015). "Physics-based stability analysis of MOS transistors". Solid-State Electronics 113: 28–34. doi:10.1016/j.sse.2015.05.010.
  8. ↑ Brown, Kenneth (March 2004). "Metal Oxide Varistor Degradation". IAEI Magazine. Retrieved 2011-03-30.
  9. ↑ http://www.avx.com/docs/techinfo/failure.pdf Failure modes of tantalum capacitors manufactured in different ways
  10. ↑ LostCircuits, CPU Guide
  11. ↑ Finegan, D. P.; Scheel, M.; Robinson, J. B.; Tjaden, B.; Hunt, I.; Mason, T. J.; Millichamp, J.; Di Michiel, M.; Offer, G. J.; Hinds, G.; Brett, D. J. L.; Shearing, P. R. (2015). "In-operando high-speed tomography of lithium-ion batteries during thermal runaway". Nature Communications 6: 6924. doi:10.1038/ncomms7924. PMC 4423228. PMID 25919582.
  12. ↑ Apple to recall 1.8 million notebook batteries
  13. ↑ PC Notebook Computer Batteries Recalled Due to Fire and Burn Hazard
  14. ↑ Lenovo and IBM Announce Recall of ThinkPad Notebook Computer Batteries Due to Fire Hazard
  15. ↑ Dell laptop battery fires
  16. ↑ PHMSA article on the UPS airplane fire
  17. ↑ The End Of The Sun
  18. ↑ Chapter 9: Post-main sequence evolution through helium burning
  19. ↑ Dearborn, D. S. P.; Lattanzio, J. C.; Eggleton, P. P. (2006-03-01). "Three‐dimensional Numerical Experimentation on the Core Helium Flash of Low‐Mass Red Giants". The Astrophysical Journal 639 (1): 405–415. arXiv:astro-ph/0512049. Bibcode:2006ApJ...639..405D. doi:10.1086/499263. ISSN 0004-637X.
  20. ↑ JPL/NASA (12 August 2010). "Fermi detects 'shocking' surprise from supernova's little cousin". PhysOrg. Retrieved 15 August 2010.
  21. ↑ Kato, M.; Hachisu, I. (December 2003). "V445 Puppis: Helium Nova on a Massive White Dwarf". The Astrophysical Journal 598 (2): L107–L110. arXiv:astro-ph/0310351. Bibcode:2003ApJ...598L.107K. doi:10.1086/380597.
  22. ↑ Cumming, A.; Bildsten, L. (2001-09-10). "Carbon flashes in the heavy-element ocean on accreting neutron stars". The Astrophysical Journal Letters 559 (2): L127–L130. arXiv:astro-ph/0107213. Bibcode:2001ApJ...559L.127C. doi:10.1086/323937. Retrieved 2012-06-03.
  23. 1 2 Schatz, H.; Bildsten, L.; Cumming, A. (2003-01-03). "Photodisintegration-triggered Nuclear Energy Release in Superbursts". The Astrophysical Journal Letters 583 (2): L87–L90. Bibcode:2003ApJ...583L..87S. doi:10.1086/368107. Retrieved 2012-06-02.
  24. 1 2 Dilday, B.; Howell, D. A.; Cenko, S. B.; Silverman, J. M.; Nugent, P. E.; Sullivan, M.; Ben-Ami, S.; Bildsten, L.; Bolte, M.; Endl, M.; Filippenko, A. V.; Gnat, O.; Horesh, A.; Hsiao, E.; Kasliwal, M. M.; Kirkman, D.; Maguire, K.; Marcy, G. W.; Moore, K.; Pan, Y.; Parrent, J. T.; Podsiadlowski, P.; Quimby, R. M.; Sternberg, A.; Suzuki, N.; Tytler, D. R.; Xu, D.; Bloom, J. S.; Gal-Yam, A.; Hook, I. M.; Kulkarni, S. R.; Law, N. M.; Ofek, E. O.; Polishook, D.; Poznanski, D. (2012-08-24). "PTF 11kx: A Type Ia Supernova with a Symbiotic Nova Progenitor". Science 337 (6097): 942–945. arXiv:1207.1306. Bibcode:2012Sci...337..942D. doi:10.1126/science.1219164. ISSN 0036-8075. PMID 22923575.
  25. ↑ "NASA's Chandra Reveals Origin of Key Cosmic Explosions". Chandra X-ray Observatory web site. Harvard-Smithsonian Center for Astrophysics. 17 February 2010. Retrieved 28 March 2012.
  26. ↑ Gal-Yam, A.; Mazzali, P.; Ofek, E. O.; Nugent, P. E.; Kulkarni, S. R.; Kasliwal, M. M.; Quimby, R. M.; Filippenko, A. V.; Cenko, S. B.; Chornock, R.; Waldman, R.; Kasen, D.; Sullivan, M.; Beshore, E. C.; Drake, A. J.; Thomas, R. C.; Bloom, J. S.; Poznanski, D.; Miller, A. A.; Foley, R. J.; Silverman, J. M.; Arcavi, I.; Ellis, R. S.; Deng, J. (2009-12-03). "Supernova 2007bi as a pair-instability explosion". Nature 462 (7273): 624–627. arXiv:1001.1156. Bibcode:2009Natur.462..624G. doi:10.1038/nature08579. ISSN 0028-0836. PMID 19956255.

External links

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