Hubbry Logo
Gate oxideGate oxideMain
Open search
Gate oxide
Community hub
Gate oxide
logo
7 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
Gate oxide
Gate oxide
from Wikipedia

The gate oxide is the dielectric layer that separates the gate terminal of a MOSFET (metal–oxide–semiconductor field-effect transistor) from the underlying source and drain terminals as well as the conductive channel that connects source and drain when the transistor is turned on. Gate oxide is formed by thermal oxidation of the silicon of the channel to form a thin (5 - 200 nm) insulating layer of silicon dioxide. The insulating silicon dioxide layer is formed through a process of self-limiting oxidation, which is described by the Deal–Grove model. A conductive gate material is subsequently deposited over the gate oxide to form the transistor. The gate oxide serves as the dielectric layer so that the gate can sustain as high as 1 to 5 MV/cm transverse electric field in order to strongly modulate the conductance of the channel.

Above the gate oxide is a thin electrode layer made of a conductor which can be aluminium, a highly doped silicon, a refractory metal such as tungsten, a silicide (TiSi, MoSi2, TaSi or WSi2) or a sandwich of these layers. This gate electrode is often called "gate metal" or "gate conductor". The geometrical width of the gate conductor electrode (the direction transverse to current flow) is called the physical gate width. The physical gate width may be slightly different from the electrical channel width used to model the transistor as fringing electric fields can exert an influence on conductors that are not immediately below the gate.

The electrical properties of the gate oxide are critical to the formation of the conductive channel region below the gate. In NMOS-type devices, the zone beneath the gate oxide is a thin n-type inversion layer on the surface of the p-type semiconductor substrate. It is induced by the oxide electric field from the applied gate voltage VG. This is known as the inversion channel. It is the conduction channel that allows the electrons to flow from the source to the drain.[1]

Overstressing the gate oxide layer, a common failure mode of MOS devices, may lead to gate rupture or to stress induced leakage current.

During manufacturing by reactive-ion-etching the gate oxide may damaged by antenna effect.

History

[edit]

The first MOSFET (metal–oxide–semiconductor field-effect transistor, or MOS transistor) was invented by Egyptian engineer Mohamed Atalla and Korean engineer Dawon Kahng at Bell Labs in 1959.[2] In 1960, Atalla and Kahng fabricated the first MOSFET with a gate oxide thickness of 100 nm, along with a gate length of 20 μm.[3] In 1987, Bijan Davari led a research team at the IBM Thomas J. Watson Research Center that demonstrated the first MOSFET with a 10 nm gate oxide thickness, using tungsten gate technology.[4]

References

[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
The gate oxide is a thin layer, typically composed of (SiO₂), that electrically insulates the gate electrode from the underlying channel in metal-oxide-semiconductor field-effect transistors (MOSFETs). This layer enables the of an applied gate voltage to modulate the channel conductivity, forming the basis for the transistor's switching and amplification functions essential to modern integrated circuits. Formed primarily through of the substrate at temperatures between 900°C and 1100°C in an oxygen ambient, the gate oxide achieves thicknesses as low as 1–2 nm in advanced nodes to support high-speed operation and low power consumption. Its dielectric constant is approximately 3.9, which determines the oxide Cox=ϵox/toxC_{ox} = \epsilon_{ox} / t_{ox} (where toxt_{ox} is the thickness), directly influencing the transistor's and VtV_t. As MOSFET scaling has progressed toward sub-10 nm regimes, challenges such as quantum tunneling-induced gate leakage and reliability degradation from phenomena like time-dependent dielectric breakdown (TDDB) have necessitated alternatives to pure SiO₂, including high-k materials like hafnium oxide (HfO₂) with dielectric constants up to 25. These high-k gate s maintain equivalent oxide thickness (EOT) below 1 nm while reducing physical thickness to mitigate leakage, enabling continued performance improvements in ultra-large-scale integration (ULSI) devices.

Fundamentals

Definition and Function

The gate oxide serves as a thin layer positioned between the gate electrode and the substrate in field-effect transistors (FETs), most notably metal-oxide-semiconductor field-effect transistors (MOSFETs). This insulating layer, typically on the order of 1 to 10 nanometers thick, electrically isolates the gate from the underlying channel region, preventing direct conduction of charge carriers while allowing electrostatic influence across the structure. In operation, the gate oxide enables the application of a gate voltage to modulate the conductivity of the channel beneath it without permitting current to flow through the oxide itself. By generating an that penetrates the , the gate voltage attracts or repels charge carriers in the substrate, forming or depleting an inversion layer that controls the flow of current between the source and drain terminals. This insulated-gate mechanism, central to the field-effect principle, ensures efficient voltage-controlled switching with minimal power dissipation in the gate circuit. At its core, the gate oxide functions as the dielectric in a metal-oxide-semiconductor (MOS) capacitor structure, where the gate electrode and substrate act as the plates, facilitating capacitive coupling between them. This coupling translates the applied gate voltage into a surface potential shift in the semiconductor, enabling precise control over carrier density and device threshold characteristics. Traditionally composed of silicon dioxide (SiO₂), the oxide's high band gap—approximately 9 electron volts—provides robust insulation against carrier injection under typical operating fields. To quantify its insulating effectiveness across different materials, the (EOT) is employed as a standardized metric, representing the thickness of a hypothetical SiO₂ layer that would yield the same as the actual stack. Defined as EOT = (ε₀ ε_SiO₂) / C_ox, where ε₀ is the , ε_SiO₂ is the of SiO₂ (approximately 3.9), and C_ox is the measured oxide per unit area, this parameter accounts for quantum effects and interfacial layers that influence effective electrical thickness. EOT thus allows performance comparisons in scaled devices, targeting sub-1 nm values for advanced nodes to maintain capacitive control amid aggressive thinning.

Materials Used

The primary material used for gate oxides is silicon dioxide (SiO₂), valued for its excellent compatibility with silicon substrates and its ability to form as a native oxide layer during processing. This compatibility arises from the natural thermodynamic stability of SiO₂ on silicon, enabling high-quality interfaces with low defect densities in metal-oxide-semiconductor (MOS) structures. To enhance reliability beyond pure SiO₂, silicon oxynitride (SiON) serves as an alternative dielectric, incorporating nitrogen to reduce boron penetration and improve time-dependent dielectric breakdown (TDDB) characteristics. For further scaling, high-k materials such as hafnium oxide (HfO₂), zirconium oxide (ZrO₂), and aluminum oxide (Al₂O₃) are employed, offering higher dielectric constants that allow for physically thicker layers while achieving equivalent oxide thickness (EOT) values comparable to ultrathin SiO₂, thereby maintaining capacitive coupling without excessive leakage. These high-k options, with k-values ranging from approximately 9 for Al₂O₃ to 25 for HfO₂, enable better gate control in advanced nodes. Material selection for gate oxides prioritizes several key criteria, including a wide bandgap to ensure low leakage and high breakdown strength, a high constant (k-value) to maximize , good lattice matching with the substrate to minimize interfacial traps, and thermal stability to withstand high-temperature fabrication steps. For instance, SiO₂ offers a bandgap of about 9 eV and excellent thermal stability up to 1000°C, while high-k alternatives like HfO₂ provide a bandgap around 6 eV but require careful for lattice mismatch (e.g., ~2% for HfO₂ on Si). These properties ensure robust electrical performance and process integration. The transition from SiO₂ to high-k dielectrics has been driven by the physical thickness limits of SiO₂, where scaling below 1 nm leads to prohibitive quantum tunneling and leakage currents, necessitating alternatives to sustain in sub-10 nm technologies. This shift allows equivalent at thicker physical dimensions, addressing the exponential increase in leakage observed in pure SiO₂ at atomic-scale thicknesses.

Fabrication Techniques

Thermal Oxidation

Thermal oxidation serves as the foundational technique for fabricating silicon dioxide (SiO₂) gate oxide layers by directly reacting substrates with an oxidant at elevated temperatures, typically between 800°C and 1200°C. This process leverages the native affinity of for oxygen to form a stoichiometric, amorphous SiO₂ film that integrates seamlessly with the substrate. The reaction occurs in a controlled furnace environment, where the silicon wafer is exposed to the oxidant, enabling atomic-scale growth from the surface inward. Two primary variants distinguish the process: dry oxidation and wet oxidation. Dry oxidation employs purified oxygen gas (O₂, with less than 5 ppm water vapor) in a reaction given by Si + O₂ → SiO₂, proceeding at a slower rate of approximately 14–25 nm per hour to produce dense, high-purity films ideal for precision applications. In contrast, wet oxidation utilizes (H₂O), often generated by bubbling O₂ through heated (around 95°C) or via pyrogenic combustion (2H₂ + O₂ → 2H₂O), following the reaction Si + 2H₂O → SiO₂ + 2H₂; this method achieves faster growth due to the higher and of H₂O in SiO₂, though the resulting films exhibit slightly greater . Dry oxidation is preferred for thin layers where superior and electrical integrity are paramount, while wet oxidation suits thicker field oxides in legacy processes. The kinetics of oxide growth in thermal oxidation are governed by the Deal-Grove model, which integrates molecular diffusion through the growing oxide layer and the surface reaction at the Si/SiO₂ interface. This model yields a linear-parabolic growth law expressed as: x2+Ax=B(t+τ)x^2 + A x = B (t + \tau) where xx is the oxide thickness, tt is the oxidation time, τ\tau accounts for any initial oxide layer (τ=(xi2+Axi)/B\tau = (x_i^2 + A x_i)/B), A=2D/ksA = 2D/k_s is the linear rate constant (with DD as the oxidant diffusivity in SiO₂ and ksk_s the surface reaction rate constant), and B=2DC/NB = 2DC^*/N is the parabolic rate constant (with CC^* the equilibrium oxidant concentration in the oxide and NN the number of oxidant molecules incorporated per unit volume of SiO₂). For thin oxides (early stages), growth is reaction-limited and linear (dx/dtB/Adx/dt \approx B/A); as thickness increases, it becomes diffusion-limited and parabolic (dx/dtB/(2t)dx/dt \approx \sqrt{B/(2t)}
Add your contribution
Related Hubs
User Avatar
No comments yet.