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  Resist & Steppers

 

 

Resists

  High sensitivity to the wavelength used for imaging, but not for all optical wave lengths.
  High contrast, i.e. little response (= "blackening") to intensities below some level, and strong response to large intensities. This is needed to sharpen edges since diffraction effects do not allow sharp intensity variations at dimensions around the wavelength of the light as illustrated below.
     
   
Resist response
     
  Compatibility with general semiconductor requirements (easy to deposit, to structure, to etch off; no elements involved with the potential to contaminate Si as e.g. heavy metals or alkali metals (this includes the developer), no particle production, and so on).
  Homogeneous "blackening" with depth - this means little absorption. Simply imagine that the resist is strongly absorbing, which would mean only its top part becomes exposed. Removal of the "blackened" and developed resist than would not even open a complete hole to the layer below.
  No reflection of light, especially at the interface resist - substrate. Otherwise we encounter all kinds of interference effects between the light going down and the one coming up (known as "Newton fringes"). Given the highly monochromatic and coherent nature of the light used for lithography, it is fairly easy to even produce standing light waves in the resist layer as shown below. While the ripple structure clearly visible in the resist is not so detrimental in this example, very bad things can happen if the substrate below the resist is not perfectly flat.
     
   
Standing waves in photo resist
     
  Strongly absorbing resist - in direct contradiction to the requirement stated above. An anti-reflection coating (ARC) might be used between substrate and resist, adding process complexity and cost.
  Suitability of the resist as direct mask for ion-implantation or for plasma etching.
  Easy stripping of the resist, even after it was turned into a tough polymer or carbonized by high-energy ion bombardment.

Stepper

  Optimize optical resolution
  The resolution limit of optical instruments is equal to about the wave-length l. More precisely and quantitatively we have
     
   
dmin  »  l

2NA

     
  With dmin = minimal distinguishable feature size; i.e the distance between two Al lines, and NA = numerical aperture of the optical system (the NA for a single lens is roughly the quotient of focal length : diameter; i.e. a crude measure of the size of the lens).
  Blue light has a wave length of about 0,4 µm, and the numerical apertures NA of very good lenses are principally < 1; a value of 0,6 is about the best you can do (consider that all distortions and aberrations troubling optical lenses become more severe with increasing NA). This would give us a minimum feature size of .
     
   
dmin  »  0,4

1,2

  = 0,33 µm
     
  Since nowadays you can buy chips with minimum features of 0,18 µm or even 0,13 µm; we obviously must do better than to use just the visible part of the spectrum.
  2. Adjust depth of focus
  Adjust the NA of the lens using the formulas:
     
   
Df  »  l

(NA)2

 =  0,4

0,62

  = 1,11 µm
     
  3. Align one exposure exactly on top of the preceding one. We need a wafer stage that can move the wafer around with a precision of lets say 1/5 of dmin - corresponding to 0,18/5 µm = 0,036 µm = 36 nm.
  Control the stage movement and measure where we are with respect to some alignment marks on the chip with the same kind of precision.
  Alignment is done optically, too, as an integral part of stepper technology.
  4. Reliable & Reproducible - 10 000 and more exposures a day in one stepper.

 

 
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