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Lithography & Patterning / Lithographic techniques

Optical-Lithography

Optical lithography is a fast patterning technique as all patterns are transferred to the photoresist through the mask in parallel. This requires that the relevant photomasks are already available or that they also need to be fabricated usually by electron beam lithography (in the case of non-standard patterns). Standard photomasks are made of fused quartz coated with a layer of chromium. During mask fabrication Cr is etched away where the geometric patterns need to be. This way UV light has a clear path through the mask, so as to expose the photosensitive resist and transfer the patterns, while Cr acts as a light-stop layer to prevent the illumination of the rest of the photoresist. The most common UV light wavelengths used in standard photolithography are the 436 nm ("g-line"), the 405 nm ("h-line") and the 365 nm ("i-line"), all being spectral lines of an Hg lamp. The achievable resolutions at these wavelengths go down to below 1 μm. There are different modes one can perform standard photolithography either with the mask being in contact with the resist-coated sample (contact lithography) or leaving a small gap (proximity lithography) each one having its own advantages and disadvantages.

The present implementation of the technique is suitable for mm to cm-size samples as those typically studied by spectroscopy and microscopy.

Available instruments

Select instruments to view their specifications and compare them (3 max)

Lab's Facility

Milano

POLIMI-POLIFAB

Bologna

CNR-ISMN@BO

Instruments' description and comparison

Also consider

In a scanning electron microscope (SEM), an electron beam is scanned over the sample surface in a raster pattern while signals from secondary electrons (SE) or Back-scattered electrons (BSE) are recorded by specific electron detectors. The electron beam, typically with an energy ranging from a few hundred eV up to 30 keV, is focused to a spot of about 0.4 nm to 5 nm in diameter. The latest generation of SEMs can achieve a resolution of 0.4 nm at 30 kV and 0.9 nm at 1 kV.

Beyond the ability to image a comparatively large area of the specimen, SEM can be equipped with a variety of analytical techniques for measuring the specimen's composition. Chemical composition analysis can be performed by Energy Dispersive X-ray Spectroscopy (EDS), which relies on generating an X-ray spectrum from the entire scan area of the SEM. An EDS detector mounted in the SEM chamber collects and separates the characteristic X-rays of different elements into an energy spectrum. The EDS system software then analyzes this energy spectrum to determine the abundance of specific elements. EDS can identify the chemical composition of materials down to a spot size and create elemental composition maps over a much broader raster area.

By employing a suitable polarimeter, such as a Mott analyzer, the spin polarization of secondary electrons can be detected, thus revealing the magnetization orientation in a ferromagnetic sample with high spatial resolution. This technique is known as Scanning Electron Microscopy with Polarization Analysis (SEMPA).

Scanning transmission electron microscopy (STEM) can be also performed in a SEM. It provides high-resolution images and detailed information about the composition and structure of samples, making it an essential tool in various scientific fields. STEM Images can be of different types: Bright-Field (BF) images formed by transmitted electrons that pass through the sample without significant scattering; Annular Dark-Field (ADF) images formed by high-angle scattered electrons, providing information about the atomic number distribution in the sample, and; High-Angle Annular Dark-Field (HAADF) images formed by very high-angle scattered electrons, revealing the heaviest elements in the sample with high contrast.

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SEM

Scanning Electron Microscopy

Advanced Characterization and Fine Analysis

The Vector Network Analyser is typically used to characterize the electrical response of a system as a function of frequency (from 10 MHz up to 40 GHz). The tool can apply a calibrated electrical stimulus of specific frequency and measure the reflected/transmitted voltage and current both in magnitude and phase. The resulting measurement presents a detailed electrical characterization of the system in terms of equivalent impedance of the network or device under test (DUT) as a function of frequency throughout the measured frequency range. Obtaining this information as a function of frequency enables detailed electrical description of complex electrical response in a simple and concise way. The technique is extremely powerful in the sense that it can provide complete electrical response information on any linear electrical system. It is commonly used to measure high frequency devices as well as measure the material properties in extended frequency ranges. The VNA can be coupled with an external dipole/quadrupole electromagnet to perform broadband FMR and spin wave spectroscopy. FMR VNA is a powerful all electric experimental technique that can be used to resolve fundamental material properties (e.g. saturation magnetization, damping coefficient, gyromagnetic ratio). The FMR VNA can sweep the frequency of the input signal and measure reflected/transmitted signal while the external magnet can sweep the magnetic field providing much bigger set of data. The quadrupole magnet can generate a vectorial magnetic field tunable in the sample plane with a maximum intensity > 0.2 T (> 0.15 T in the dipolar configuration). The sample is excited by passing the RF signals through a standing coplanar waveguide (CPW) over which the sample is positioned. The VNA setup can be used to detect spin waves propagating in the magnetic ordering of a material under study. The VNA can be connected to a pair of parallel microwave antennas through RF microprobes (e.g. coplanar waveguides and ground-signal-ground (GSG) RF probes). Each microstrip is connected to a separate port of the VNA. Spin waves are excited from the first antenna (transmitter) and detected by the second one (receiver). This analysis is most useful to understand the behavior of magnetic materials.

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RF-VNA

RF VNA characterization with probe station

Upscale to Intermediate TRL

The principle of wet etching processes is the conversion of a solid material into liquid compounds using chemical solutions. The selectivity is usually very high, and for most solutions is greater than 100:1. Material removal rate for wet etching is usually faster than the rates for many dry etching processes and can easily be changed by varying temperature and concentration of the active species. Multiple wafers can be etched simultaneously in batch etching; in this case filters and circulating pumps prevent particles from reaching the wafers.

When a material is attacked by a liquid or vapor etchant, it can be removed with isotropic (uniformly in all directions) or with anisotropic etching. In anisotropic etching the liquid etchants etch crystalline materials at different rates depending upon which crystal face is exposed to the etchant.

Wet or dry etching processes are common steps in the technological process flow for obtaining the material under study well patterned, isolated and ready to be contacted.

In particular, the process flow usually contains the required suite of pattern transfer and/or etching processes for ancillary materials, such as silicon nitride, silicon oxide, polysilicon that can be used as etching masks, implantation and diffusion barriers, dielectric barriers, spacers or conductive layers. Those materials can be etched and patterned by chemical wet etching or by Reactive Ion Etching (RIE) using appropriate masks or making use of lift-off process. Those materials can be used themselves as etching masks (for instance in the case of Al layers for deep RIE patterning of substrates), or as adhesion or barrier layers or directly as layers for providing the required electrical contact. 

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WE

Wet Etching

Lithography & Patterning