Spring04 implementation high res reticle

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Implementation of High Resolution Reticle Inspection in Wafer Fabs Aditya Dayal, KLA-Tencor Corporation Nathan Bergmann, Peter Sanchez, Intel Corporation

Many advanced wafer fabs are currently fabricating devices with 130 nm or smaller design rules. To meet the challenges at these sub-wavelength technology nodes, fabs are using a variety of resolution enhancement techniques (RETs) in lithography and exploring new methods of processing, inspecting and requalifying photomasks. The acceleration of the lithography roadmap imposes more stringent requirements on mask qualification and requalification to ensure that device yields are not compromised: mask inspection tools of today need to find smaller defects on reticles against considerably more complicated patterns or tighter critical dimensions (CDs). In this paper we describe the early stages of implementation and proliferation of advanced reticle inspection tools at high volume manufacturing wafer fabs. We describe the tools and procedure used to streamline reticle requalification at the fabs and improve the feedback loop between the fabs and the mask shop.

Introduction

This paper describes an SL3UV inspection tool-based infrastructure for contamination inspection of reticles in wafer fabs. This tool scans the patterned surface of the reticle using a 364 nm laser in simultaneous transmitted and reflected (STARlight™) mode to detect defects. Such defects include particle contaminants, stains, scratches, crystal growth or also certain kinds of pattern defects/irregularities.1 Central to the defect detection methodology of these requalification tools is the procedure of STARlight calibration. During this procedure, the tool acquires images by sampling various geometries on the reticle and constructs a database of their transmitted and reflected (T/R) light properties. Then, during inspection, the tool scans the reticle, one swath at a time, and the algorithms compare the digitized T/R measurements at each point on the reticle against the previously constructed T/R database to identify outliers or defects. Unlike pattern defect tools, which use a die-to-die or die-to-database comparison,

the SL3UV tool does not require a reference comparison image to identify defects. The STARlight tools have a sensitivity limit of ~0.18 µm at the 0.25 µm pixel (P250), as measured on polystyrene latex spheres (PSLs). The tools can also be equipped with the unpatterned reticle surface analysis (URSA) option, which allows quick inspection of the chrome-side pellicle, the back glass surface and, if present, a back glass pellicle. URSA is a darkfield (off-axis illumination) inspection system which uses 690 nm laser light to look for particles, scratches or pellicle tears down to a resolution limit of ~4 µm. Figure 1 on the following page shows a schematic of an SL3UV system with STARlight and URSA. In the following sections we describe the early stages of implementation of the SL3UV inspection tools at high volume manufacturing wafer fabs. First, we discuss the reticle qualification and requalification methodology, followed by a section which compares the differences and improvements of using the SL3UV tool in a wafer fab, as compared with previous methods of reticle verification. Then, we present some data illustrating the success of these tools for reticle requalification. Spring 2004

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