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SiliCon
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| SiliCon with Adam Savage | |
|---|---|
| Status | Active |
| Genre | Multi-genre |
| Venue | San Jose Convention Center |
| Location | San Jose, California |
| Country | United States |
| Inaugurated | 2016 (as Silicon Valley Comic Con) |
| Most recent | 2022[1] |
| Leader | Adam Savage |
| Website | www |
SiliCon with Adam Savage (formally Silicon Valley Comic Con) was an annual pop culture and technology convention, at the San Jose Convention Center in San Jose, California. The convention was founded by Steve Wozniak, Stan Lee and Rick White. The inaugural event was held March 18–20, 2016 at San Jose's McEnery Convention Center.[2] The convention was rebranded as SiliCon in early 2020 and Adam Savage appointed as the creative director. It was canceled after the 2022 event.[1]
History
[edit]Silicon Valley Comic Con was first announced April 17, 2015 through an online video featuring Steve Wozniak and Stan Lee.[3] The aim was to bring together popular culture touchstones such as comics, movies, genre TV and technology together as one convention. Including panels featuring creative artists, writers, actors, directors, producers, and science communicators.[4]
Silicon Valley Comic Con will be the San Francisco Bay Area's first large multi-genre convention since the departure of WonderCon after that convention's 2011 show.[5] Since WonderCon's departure the largest convention left in the Bay Area had been Big Wow! Comicfest, which is being added to Silicon Valley Comic Con's schedule.[6]
On July 13, 2016, the second annual event was confirmed to be occurring April 21–23, 2017 at the San Jose Convention Center as well as expanding into several additional venues nearby.[7]
On February 20, 2020, the convention was renamed SiliCon, and Adam Savage was named the new creative director.[8] The 2020 event was to have taken place October 16–18 at the San Jose Convention Center, but the COVID-19 pandemic forced officials to move to a virtual show.
The SiliCon 2023 was cancelled and the convention was discontinued, with the organizers alluding to the continued impact of the COVID-19 pandemic and funding issues.[9] In 2024, a different comic con, GalaxyCon, debuted at the San Jose Convention Center.[1]
Features and events
[edit]The convention aimed to include both popular culture and technology in what Wozniak hopes will be a uniquely Silicon Valley flavor.[10] In that spirit, the convention had typical comic convention staples such as an "artists alley", but it also had an "app alley" featuring new and emerging technology items. Several movie and television studios were represented at the inaugural event including Warner Bros. Pictures, Lionsgate and AMC.[11] Additionally several technology-focused guests were involved as well including astrophysicists and technologists.
Convention locations
[edit]See also
[edit]References
[edit]- ^ a b c Pizarro, Sal (August 13, 2024). "GalaxyCon bringing fandom stars to San Jose this weekend". The Mercury News. San Jose, California. Retrieved October 11, 2024.
- ^ "Silicon Valley Comic Con WOZ Welcome Address, published on YouTube". YouTube. Retrieved May 2, 2016.
- ^ "Silicon Valley Comic Con 2016, published on YouTube". YouTube. Retrieved April 17, 2015.
- ^ "SVCC ABOUT/FAQ".
- ^ "Steve Wozniak and Stan Lee are bringing Silicon Valley its own comic con – GamesBeat – Games – by Mike Minotti". VentureBeat. April 17, 2015. Retrieved July 17, 2015.
- ^ "Silicon Valley Comic Con Announced in Dorky Video With Stan Lee And Woz". SFist. Archived from the original on April 21, 2015. Retrieved July 17, 2015.
- ^ a b Ross, Martha (July 28, 2016). "Woz's 2017 Silicon Valley Comic Con: Got $250? VIP tickets on sale today – The Mercury News". Mercurynews.com. Retrieved July 13, 2017.
- ^ "Adam Savage is the new Creative Director of Silicon Valley Comic Con". 8Bit/Digi. February 20, 2020. Retrieved February 20, 2020.
- ^ Pizarro, Sal (May 8, 2023). "SiliCon, Silicon Valley's pop culture and maker fest, canceled for 2023". The Mercury News.
- ^ "Steve Wozniak Teams With Stan Lee for New Silicon Valley Comic Con". NBC Bay Area. April 17, 2015. Retrieved July 17, 2015.
- ^ a b "Karen Gillan, Jeremy Renner, Stan Lee, William Shatner Coming To Silicon Valley Comic-Con". Cosmic Book News. January 15, 2016. Retrieved July 13, 2017.
- ^ Wangberg, David (March 27, 2016). "Recapping the inaugural Silicon Valley Comic Con". AXS. Retrieved July 13, 2017.
- ^ "Boldly Going Where No One Has Gone Before: William Shatner to Host 'Star Trek' 50th Anniversary Celebration at Inaugural Silicon Valley Comic Con". Benzinga. September 21, 2015. Retrieved July 13, 2017.
- ^ "Silicon Valley Comic Con Reveals Celebrity Guest List". Comicbookresources.com. November 5, 2015. Archived from the original on January 12, 2016. Retrieved July 13, 2017.
- ^ Franich, Darren (February 3, 2016). "Back to the Future stars will reunite at the Silicon Valley Comic Con – exclusive". Ew.com. Retrieved July 13, 2017.
- ^ "Silicon Valley Comic Con 2017 was a Success and will Return in 2018". 8bitdigi.com. April 28, 2017. Retrieved July 13, 2017.
- ^ "Silicon Valley Comic Con: What worked and what didn't". April 23, 2017.
- ^ "Third annual silicon valley comic con draws largest crowd to-date" (PDF). Archived from the original (PDF) on April 14, 2018.
- ^ "First Batch of Silicon Valley Comic Con 2018 Guest Revealed". 8Bit/Digi. November 24, 2017. Retrieved January 5, 2018.
- ^ "Arnold Schwarzenegger, Jason Momoa and more booked for Silicon Valley Comic Con 2019".
External links
[edit]SiliCon
View on GrokipediaHistory
Discovery and early isolation
In 1787, French chemist Antoine Lavoisier proposed that silica (silicon dioxide), a common component of rocks and minerals, was likely the oxide of a previously unidentified chemical element, marking the first recognition of silicon's potential existence as a distinct substance.[6] This insight built on earlier observations of silica's refractory properties, which resisted decomposition under heat and acids, suggesting it was not a simple earth but a compound.[7] Attempts to isolate the element soon followed, but silicon's strong affinity for oxygen proved challenging. In 1808, British chemist Humphry Davy tried to reduce silica using electrolysis and other methods, producing impure residues but failing to obtain the pure element; he nonetheless proposed the name "silicium," derived from the Latin word for flint, silex.[8] French chemists Joseph Louis Gay-Lussac and Louis Jacques Thénard also attempted isolation around 1811 by reacting potassium with silicon tetrafluoride, yielding a dark powder that contained silicon but was contaminated with impurities.[7][1] The successful isolation came in 1823–1824, when Swedish chemist Jöns Jacob Berzelius heated potassium fluosilicate (K₂SiF₆) with excess potassium metal, producing amorphous silicon as a brown powder. Berzelius confirmed its elemental nature through further analysis, noting its refractory behavior—resistant to oxidation and melting only at high temperatures—and distinguishing it from metals and other nonmetals. He renamed it "silicon" to emphasize its non-metallic character, retaining the root from silex. In 1854, French chemist Henri Étienne Sainte-Claire Deville produced crystalline silicon by heating silicon tetrachloride with sodium.[1] Subsequent early 19th-century experiments by Berzelius and others, including reactions with halogens to form volatile compounds like silicon tetrachloride, solidified silicon's status as a unique element in the periodic system.[9] Prior to the isolation of elemental silicon, its compounds, particularly silica, had long been utilized in practical applications such as ceramics, pottery glazes, and glassmaking, dating back to ancient civilizations for tools, vessels, and ornaments. These uses exploited silica's durability and heat resistance, though the pure element's scarcity limited its immediate exploitation until later refinements.Development of semiconductors
The development of silicon as a semiconductor material began with key discoveries in crystal purification and junction formation during the early 20th century. In 1940, Russell Ohl at Bell Laboratories accidentally discovered the p-n junction while investigating silicon crystals for use in radar detectors during World War II; he observed that a crack in a silicon boule created a rectifying barrier that exhibited photovoltaic effects, leading to a patent for a light-sensitive device in 1941.[10] This breakthrough demonstrated silicon's potential for electronic rectification, though initial impurities limited its performance compared to germanium.[11] Advancements in purification were essential to harness silicon's properties. In 1952, William Pfann at Bell Labs invented the zone melting (or zone refining) technique, which involved passing a narrow molten zone along a semiconductor rod to segregate impurities, achieving purity levels below one part per million—critical for reproducible device fabrication.[11] This method, initially applied to germanium, was quickly adapted for silicon, enabling the growth of high-quality single crystals via the Czochralski process refined around the same period.[12] These techniques addressed silicon's higher melting point and greater affinity for oxygen, making it viable for semiconductor applications. The transistor's invention marked a pivotal shift toward silicon. In December 1947, William Shockley, John Bardeen, and Walter Brattain at Bell Labs demonstrated the first point-contact transistor using germanium, earning them the 1956 Nobel Prize in Physics; however, silicon's superior thermal stability and abundance prompted rapid research to transition the technology.[13] By 1954, Morris Tanenbaum at Bell Labs fabricated the first silicon junction transistor, achieving higher operating temperatures up to 150°C compared to germanium's limits. Independently, Gordon Teal's team at Texas Instruments produced the first commercial silicon transistor that year using grown-junction methods, enabling reliable high-power applications and spurring industry adoption.[10][11] Early commercial exploitation focused on diodes and rectifiers. Building on Ohl's work, companies like General Electric and Sylvania began producing silicon rectifiers in the early 1950s for power conversion in industrial and military uses, offering greater efficiency and durability than vacuum tubes or selenium alternatives.[10] By mid-decade, these devices powered early computers and telecommunications equipment, laying the groundwork for silicon's dominance in electronics.[11]The Silicon Age
The term "Silicon Age" emerged in the late 20th century to describe the era dominated by silicon-based technologies, paralleling historical periods like the Iron Age in marking a transformative shift in materials and society.[14] This designation gained prominence in the 1990s as silicon's role in electronics became ubiquitous, fundamentally altering computing, communications, and daily life. The concept is closely tied to the rise of Silicon Valley, a region in California's Santa Clara Valley that began coalescing as a tech hub in the 1950s with the establishment of firms like Shockley Semiconductor Laboratory in 1955 and Fairchild Semiconductor in 1957, fostering innovation in silicon devices during the 1960s.[15] By the late 1960s, the area's concentration of semiconductor activity had earned it the nickname "Silicon Valley," symbolizing the start of widespread silicon industrialization post-World War II.[16] A pivotal milestone in silicon-based computing arrived in 1971 with Intel's introduction of the 4004 microprocessor, the first commercially available single-chip CPU, which integrated 2,300 transistors and enabled programmable logic on silicon wafers.[17] This innovation marked the transition from discrete components to integrated systems, accelerating the digital revolution by making computing more accessible and compact. The semiconductor industry's growth exploded thereafter, with global sales surpassing $1 billion in 1966 and reaching $627 billion by 2024, propelled by Moore's Law—coined by Gordon Moore in his 1965 Electronics magazine article, which predicted the number of transistors on a chip would double approximately every year, later revised to every two years.[18][19][20] This exponential scaling drove cost reductions and performance gains, fueling the proliferation of personal computers and consumer electronics. The 1980s brought the VLSI (very-large-scale integration) revolution, where advancements in design methodologies, notably from Carver Mead and Lynn Conway's 1980 textbook, enabled millions of transistors per chip, revolutionizing chip complexity and production efficiency.[21] This era solidified silicon's dominance in integrated circuits, supporting the expansion of computing into businesses and homes. The 2000s witnessed a mobile computing boom, ignited by devices like the 2007 iPhone, which spiked demand for advanced silicon processors and memory, integrating computing into portable gadgets and spurring applications in telecommunications and multimedia.[22] Global production dynamics shifted dramatically over decades, with Asia emerging as the dominant force; by 2025, the region accounted for over 70% of worldwide semiconductor manufacturing capacity, led by Taiwan, South Korea, and China, despite ongoing diversification efforts elsewhere.[23] This concentration arose from investments in fabrication facilities starting in the 1970s, enabling cost-effective scaling and supply chain integration that powered the industry's growth into a multi-hundred-billion-dollar ecosystem.[24]Properties
Physical and atomic properties
Silicon is a chemical element with atomic number 14 and the electron configuration [Ne] 3s² 3p², featuring a covalent radius of 111 pm.[1] It has an electronegativity of 1.90 on the Pauling scale, a first ionization energy of 8.15 eV, and common oxidation states of +4 (with -4 possible in certain compounds).[1] These atomic characteristics position silicon within group 14 of the periodic table, where it forms tetrahedral covalent bonds due to its four valence electrons. At room temperature, silicon exists as a solid with a density of 2.329 g/cm³.[3] It transitions to a liquid at its melting point of 1414 °C and vaporizes at a boiling point of 3265 °C.[25] The stable allotrope of silicon adopts a diamond cubic crystal structure, characterized by a lattice parameter of approximately 0.543 nm, and displays a grayish metallic luster.[26][27] Silicon exhibits a linear thermal expansion coefficient of 2.6 × 10⁻⁶ K⁻¹ and a specific heat capacity of 0.71 J/g·K.[28] At the electronic level, it possesses an indirect band gap of 1.12 eV, a property that underlies its classification as a semiconductor and influences its electrical behavior.[29]Electrical and optical properties
Silicon exhibits intrinsic semiconducting behavior with a high resistivity of approximately Ω·cm at 300 K, arising from its indirect bandgap that limits thermal generation of charge carriers.[30] This resistivity can be tuned over several orders of magnitude through doping: phosphorus introduces donor levels for n-type conduction, increasing electron concentration, while boron creates acceptor levels for p-type conduction, enhancing hole concentration.[31] In pure silicon, charge carrier mobilities at 300 K reach 1400 cm²/V·s for electrons and 450 cm²/V·s for holes, reflecting the material's low effective masses and minimal scattering in the diamond cubic lattice.[31] The static dielectric constant of silicon is 11.7, enabling effective electric field screening in devices, while its dielectric breakdown strength is approximately 0.3 MV/cm, beyond which avalanche multiplication occurs.[32][31] Optically, silicon features an absorption edge near 1.1 eV, tied to its indirect bandgap of 1.12 eV, resulting in low absorption for photon energies below this threshold and high transparency in the infrared spectrum beyond about 1.1 μm.[33] This infrared transparency underpins its application in infrared detectors, where it efficiently transmits longer wavelengths while absorbing visible light.[34] Thermoelectrically, silicon displays a Seebeck coefficient that ranges from roughly -100 μV/K in n-type material to +100 μV/K in p-type, modulated by doping concentration which alters the Fermi level position relative to the band edges.[35]Chemical properties
Silicon exhibits tetravalent character, utilizing its four valence electrons to form covalent bonds, primarily in a tetrahedral geometry similar to carbon but with distinct preferences due to atomic size and electronegativity differences.[36] The Si-Si bond strength averages 226 kJ/mol, which is relatively weak compared to carbon-carbon bonds, while the Si-O bond is exceptionally strong at 452 kJ/mol, favoring oxygen-containing structures over extended silicon chains.[36] In contrast, the Si-H bond energy is 318 kJ/mol, enabling some hydridic reactivity but limiting stable molecular analogs to hydrocarbons.[37] This bonding profile contributes to silicon's tendency to form extended network solids rather than discrete molecular compounds, unlike carbon, which readily produces stable liquid-phase organics; silicon lacks analogous stable liquid compounds and instead polymerizes into robust covalent lattices.[36] Silicon demonstrates notable chemical stability under ambient conditions, resisting most acids due to the formation of a thin, impervious SiO₂ passivation layer upon exposure to oxygen, which inhibits further corrosion.[38] However, it dissolves readily in hydrofluoric acid (HF), where the reaction proceeds via formation of soluble fluorosilicates, driven by the high stability of Si-F bonds: Si + 4HF → SiF₄ + 2H₂ (gaseous), though in aqueous media it forms H₂SiF₆.[38] Similarly, silicon reacts with hot, concentrated alkalis such as NaOH to produce silicates and hydrogen: Si + 2NaOH + H₂O → Na₂SiO₃ + 2H₂.[38] Silicon's high affinity for oxygen leads to spontaneous oxidation above approximately 900°C, where it reacts with O₂ to form SiO₂, a process central to thermal oxidation in semiconductor fabrication. The oxide of silicon, SiO₂, displays amphoteric behavior, albeit weakly, reacting with strong acids like HF to form silicon tetrafluoride (SiO₂ + 4HF → SiF₄ + 2H₂O) and with strong bases such as hot concentrated NaOH to yield silicates (SiO₂ + 2NaOH → Na₂SiO₃ + H₂O).[39] This dual reactivity arises from the polarized Si-O bonds, allowing SiO₂ to act as a Lewis acid toward bases while being susceptible to fluoride attack, distinguishing it from purely acidic nonmetal oxides like CO₂.[39]Isotopes
Silicon has three stable isotopes: ^{28}Si, ^{29}Si, and ^{30}Si, with no stable isotope at mass number 31.[40] The most abundant is ^{28}Si, comprising 92.223% of naturally occurring silicon, followed by ^{29}Si at 4.685% and ^{30}Si at 3.092%.[40] Their respective atomic masses are 27.97692653465(44) u for ^{28}Si, 28.97649466490(52) u for ^{29}Si, and 29.973770136(23) u for ^{30}Si.[40] These isotopic abundances contribute to silicon's standard atomic weight of [28.084, 28.086].[40] Silicon has over 20 known radioactive isotopes, most with half-lives of less than a day. Among them, ^{32}Si is notable for its relatively long half-life; measurements vary between approximately 100 and 276 years, with a recent value of 153 years, during which it undergoes beta decay to ^{32}P with a maximum energy of 0.21 MeV.[41] Produced cosmogenically in the Earth's atmosphere through spallation of argon by cosmic rays, ^{32}Si serves as a tracer for geological and hydrological processes, enabling dating of groundwater and recent sediments up to about 1,000 years old.[42] The isotope ^{29}Si, with its nuclear spin of 1/2 and natural abundance of approximately 4.7%, is particularly useful in nuclear magnetic resonance (NMR) spectroscopy for studying the structure of silicon-containing compounds, as its spin properties yield sharp, interpretable signals without quadrupolar broadening.[43]| Isotope | Atomic Mass (u) | Natural Abundance (%) | Stability | Notes |
|---|---|---|---|---|
| ^{28}Si | 27.97692653465(44) | 92.223(19) | Stable | Most abundant |
| ^{29}Si | 28.97649466490(52) | 4.685(8) | Stable | Spin 1/2; used in NMR |
| ^{30}Si | 29.973770136(23) | 3.092(11) | Stable | - |
| ^{32}Si | ~31.974 | <0.0001 (cosmogenic) | Radioactive | Half-life ~153 y (measurements vary 100-276 y); β⁻ decay |
Occurrence
Abundance in the universe and Earth
Silicon is the eighth most abundant element in the universe by mass fraction, accounting for approximately 0.065% of the total elemental mass, and ranks seventh by atomic abundance.[1] It is primarily synthesized through the oxygen-burning process in the cores of massive stars, where temperatures reach about 2 billion kelvin, fusing lighter elements like neon and oxygen into silicon and other intermediates such as sulfur and magnesium. This nucleosynthetic pathway contributes significantly to silicon's prevalence in cosmic dust, interstellar medium, and stellar atmospheres. In the solar system, silicon's abundance in the Sun's photosphere is estimated at a mole fraction of about 3.5 × 10^{-5} (or logarithmic abundance A(Si) = 7.51), making it one of the dominant heavy elements after oxygen and carbon.[44] This value aligns closely with cosmic averages and reflects the element's incorporation during the Sun's formation from a protostellar nebula enriched by previous stellar generations.[45] On Earth, silicon is the second most abundant element in the crust, comprising 27.7% by mass, predominantly bound as silicon dioxide (SiO₂) in igneous, sedimentary, and metamorphic rocks.[3] During planetary differentiation, silicon exhibits moderately siderophile behavior, partitioning preferentially into the metallic core under high-pressure and high-temperature conditions, which results in a depletion of silicon in the mantle relative to chondritic meteorites (with bulk silicate Earth Si content ~15-20% lower than CI chondrites).[46] This core sequestration leads to relative enrichment of silicon in the silicate mantle and crust, enhancing its availability in terrestrial rocks. Variations in silicon abundance appear in meteorites; for instance, enstatite chondrites show elevated silicon contents (up to ~18 wt% SiO₂ in some phases) due to their highly reduced formation environments, contrasting with ordinary chondrites at ~15-16 wt%.[47]Natural minerals and sources
Silicon primarily occurs in nature as a component of silicate minerals, which dominate the Earth's crust. Quartz (SiO₂), the most common silicon-bearing mineral, constitutes approximately 12% of the Earth's crust by volume and is found in a wide range of igneous, metamorphic, and sedimentary rocks.[48] It forms colorless to smoky crystals in granitic pegmatites and is a key constituent of sandstones and quartzites.[49] Other silicate minerals are even more prevalent, with feldspars comprising about 60% of the crust and serving as the single most abundant mineral group.[50] Feldspars include alkali varieties like orthoclase (KAlSi₃O₈), which occurs in granites and syenites, and plagioclase types that dominate basaltic and andesitic rocks.[51] Micas, such as muscovite and biotite, contribute to the silicate content in schists and granites through their layered structures incorporating silicon-oxygen sheets. Clays, including kaolinite and illite, form from the weathering of feldspars and other silicates, accumulating in soils and sedimentary deposits as fine-grained phyllosilicates.[52] Amorphous forms of silica, lacking a crystalline structure, are also significant sources. Opal consists of hydrated amorphous silica (SiO₂·nH₂O) and forms colorful deposits in sedimentary environments or as infillings in voids.[53] Diatomaceous earth arises from the accumulation of opal skeletons from diatoms, microscopic algae, creating porous, lightweight sediments in ancient lake and ocean basins.[53] Native silicon, in its elemental form, is exceedingly rare on Earth but has been identified in extraterrestrial materials. Silicon carbide (SiC), a presolar mineral, occurs in carbonaceous chondrites like the Murray meteorite, preserved as interstellar grains within these primitive asteroids.[54] Siliceous deposits also form through geothermal and volcanic activity. Hot springs in volcanic regions precipitate siliceous sinter, a low-density, porous material rich in opal, as silica supersaturates and deposits from cooling geothermal fluids.[55] Volcanic sources contribute via rhyolitic lavas and ash, which are high in silica content, leading to extensive siliceous rock formations in caldera systems.[56]Production
Metallurgical processes
Metallurgical-grade silicon, with a purity of 98-99%, is primarily produced through high-temperature reduction processes starting from silica-rich raw materials such as quartz.[57] The dominant method is carbothermic reduction, accounting for approximately 95% of global production, where silica (SiO₂) is reduced by carbon in submerged electric arc furnaces.[58] This process operates at temperatures around 1900°C, yielding silicon metal along with carbon monoxide gas as a byproduct.[59] The reaction can be represented as: The process involves feeding quartz and carbonaceous reductants like coke, charcoal, or wood chips into the furnace, where the arc generates the necessary heat for the endothermic reaction.[60] An alternative approach for achieving slightly higher purity levels is aluminothermic reduction, which uses aluminum as the reductant instead of carbon, producing silicon and alumina slag.[61] This method follows the reaction: It is less common than carbothermic reduction but offers potential for reduced carbon emissions and integration with aluminum recycling streams, though it remains primarily experimental or used for alloy production.[62] These processes are highly energy-intensive, requiring 10-13 kWh per kilogram of silicon produced, with electricity sourced mainly from hydropower in regions like Norway or coal in major producers like China.[62] A key byproduct is ferrosilicon, an iron-silicon alloy formed when iron impurities are present, which is widely used in steel deoxidation to remove oxygen and improve castability.[63] Global production of metallurgical-grade silicon reached an estimated 4.6 million metric tons in 2024, with projections for similar or slightly higher output in 2025, dominated by China at approximately 85% of the total.[64]High-purity silicon for electronics
High-purity silicon for electronics begins with metallurgical-grade silicon, which contains 0.5% to 1.5% impurities and serves as the starting material for further refinement.[65] The primary method for producing electronic-grade polysilicon is the Siemens process, which involves converting metallurgical silicon into trichlorosilane (TCS) through the reactionat approximately 300°C in a fluidized bed reactor.[65] The TCS is then purified via fractional distillation to remove impurities with differing boiling points, followed by decomposition in a high-temperature reactor at 1150°C using hydrogen:
This deposits silicon onto heated seed rods, yielding polysilicon rods up to 2 meters long.[65] An alternative to the batch-style Siemens deposition is the fluidized bed reactor (FBR) process, which enables continuous silicon deposition from silane gas () onto silicon particles, achieving up to 90% lower energy consumption compared to traditional methods.[66] To produce single-crystal ingots suitable for semiconductors, purified polysilicon is melted and grown via the Czochralski process, the predominant method accounting for over 90% of semiconductor silicon production, involving the controlled pulling of a seed crystal from the melt to form large cylindrical ingots.[67][68] The float-zone (FZ) process is an alternative niche method for growing high-purity single-crystal silicon, particularly for applications requiring ultra-low oxygen content, though it accounts for less than 10% of production compared to Czochralski.[69] Advanced semiconductor applications require silicon at 11N purity (99.999999999%), achieved through these combined refining steps to minimize defects and ensure optimal electrical performance in integrated circuits.[70][71]