Patent Description:
An illumination optical unit with such a collector is known from <CIT> and from <CIT>. A collector mirror is known from <CIT>. Further EUV collector mirror embodiments are known from <CIT>. <CIT> discloses an EUV light source comprising a collection mirror comprising a diffraction grating to separate in-band and out-of-band radiation. An additional annular mirror is used to retro-reflect the out-of-band radiation back to the collection mirror and the plasma to enhance generation of in-band radiation by the plasma.

<CIT> and <CIT> disclose a collector for illumination light of a light source of a projection exposure apparatus.

It is an object of the present invention to develop an EUV collector mirror enabling a higher conversion efficiency between the energy of pump light of a laser discharged produced plasma (LDPP) EUV light source on the one hand and the resulting usable EUV energy on the other.

According to the invention, this object is achieved by an EUV collector mirror comprising the features specified in claim <NUM>.

According to the invention, it has been realized that a grating structure being designed to retroreflect pump light emanating from a source region of the LDPP source enables a high conversion efficiency from pump light energy into usable EUV light energy. The retroreflective pump light again is used in the source region for conversion to usable EUV light.

In particular, such retroreflecting pump light grating structure on the EUV collector mirror avoids the necessity of a Pre-Pulse/Main Pulse scheme of the pump light source as is known from prior art. This facilitates the construction of the pump light laser source. In particular, it is not necessary to preshape a target of the LDPP source, e.g. a tin droplet, with a Pre-Pulse for increasing the conversion efficiency of the Main Pulse conversion into the usable EUV light. This leads to a cost reduction with respect to the construction of a source collector module including the light source on the one hand and the EUV collector mirror on the other. The effectively used pump light energy as compared with conventional Pre-Pulse/Main Pulse schemes can be increased significantly, e.g. about a number of <NUM> % or even <NUM> %.

In particular, a spherical target can be used to be impinged upon the pump light without the need of specifically further shaping.

The pump light grating structure may be a blazed grating. A blaze angle may be optimized for a <NUM>th or for a +/- <NUM>st order of retroreflective diffraction of the pump light wavelength. A pitch of the pump light grating structure varies over the reflective surface of the EUV collector mirror in order to adapt the retroreflective properties to the angle of incidence condition of the pump light rays impinging upon the pump light grating structure.

In case of a reflection surface of the EUV collector mirror being rotationally symmetric with respect to a rotational symmetry axis, the pitch may increase with increasing distance of the grating structures to such symmetry axis or, in another embodiment, the pitch may decrease with increasing distance. In a further embodiment, a dependency between the pitch and such distance of the grating structures to the symmetry axis may be nonmonotonic.

The pump light grating structure may include two or more different height levels, i.e. may be realized as a two-step grating or as a multi-step grating.

Pump light wavelengths according to claim <NUM> and <NUM> have been proved to be particularly suitable for efficiently producing usable EUV illumination light.

A pitch, e.g. a grating period, according to claim <NUM> satisfies the retroreflecting conditions for the pump light wavelength. The pitch depends on the angle of incidence of the pump light on the reflection surface. Such angle of incidence depends upon the distance between the impingement point of the respective pump light rayon the reflection surface to an axis of rotational symmetry. As a result, the pitch depends upon the distance of a reflection surface area carrying the pump light grating structure to such axis of symmetry. With increasing distance to the axis of symmetry, the pitch may decrease.

A typical dimension of the pitch may be in the range between <NUM> to <NUM>, in particular between <NUM> and <NUM>, more in particular between <NUM> and <NUM>.

Reflectivities according to claim <NUM> can be achieved by using a proper pump light grating structure. The reflection surface of the EUV collector mirror may carry a high reflective coating which of course mainly is optimized for high reflection of the usable EUV illumination light. Such reflective coating also may be optimized for high reflection of the pump light wavelength.

The advantages of a source collector module according to claim <NUM> are those explained above with respect to the EUV collector mirror.

A pulse duration according to claim <NUM> and/or a pulse rise time according to claim <NUM> proved to show a particularly high conversion efficiency.

The advantages of an illumination optics according to claim <NUM>, of a projection exposure apparatus according to claim <NUM> and of a production method according to claim <NUM> are those which previously were discussed with respect to the EUV collector mirror and the source collector mirror module.

In particular, a semiconductor component, which is not covered by the subject-matter of the claims, for example a memory chip, may be produced using the projection exposure apparatus.

An exemplary embodiment of the invention is explained in greater detail below with reference to the drawing. In said drawing shows:.

A projection exposure apparatus <NUM> for microlithography comprises a light source module <NUM> for EUV illumination light and/or imaging light <NUM>, which will be explained in yet more detail below. Such light source module <NUM> also is denoted as a source collector module. A light source of the light source module <NUM> is an EUV light source, which produces light in a wavelength range of e.g. between <NUM> and <NUM>, in particular between <NUM> and <NUM>. The illumination light and/or imaging light <NUM> is also referred to as used EUV light below.

In particular, the EUV light source may be a light source with a used EUV wavelength of <NUM> or a light source with a used EUV wavelength of <NUM> or <NUM>. Other used EUV wavelengths are also possible. A beam path of the illumination light <NUM> is depicted very schematically in <FIG>.

An illumination optical unit <NUM> serves to guide the illumination light <NUM> from the light source to an object field <NUM> in an object plane <NUM>. Said illumination optical unit comprises a field facet mirror FF depicted very schematically in <FIG> and a pupil facet mirror PF disposed downstream in the beam path of the illumination light <NUM> and likewise depicted very schematically. A field-forming mirror 6b for grazing incidence (GI mirror; grazing incidence mirror) is arranged in the beam path of the illumination light <NUM> between the pupil facet mirror PF, which is arranged in a pupil plane 6a of the illumination optical unit, and the object field <NUM>. Such a GI mirror 6b is not mandatory.

Pupil facets (not depicted in any more detail) of the pupil facet mirror PF are part of a transfer optical unit, which transfer, and in particular image, field facets (likewise not depicted) of the field facet mirror FF into the object field <NUM> in a manner superposed on one another. An embodiment known from the prior art may be used for the field facet mirror FF on the one hand and the pupil facet mirror PF on the other hand. By way of example, such an illumination optical unit is known from <CIT>.

Using a projection optical unit or imaging optical unit <NUM>, the object field <NUM> is imaged into an image field <NUM> in an image plane <NUM> with a predetermined reduction scale. Projection optical units which may be used to this end are known from e.g. <CIT>.

In order to facilitate the description of the projection exposure apparatus <NUM> and the various embodiments of the projection optical unit <NUM>, a Cartesian xyz-coordinate system is indicated in the drawing, from which system the respective positional relationship of the components illustrated in the fig-ures is evident. In <FIG>, the x-direction runs perpendicular to the plane of the drawing into the latter. The y-direction extends to the left in <FIG> and the z-direction extends upward in <FIG>. The object plane <NUM> extends parallel to the xy-plane.

The object field <NUM> and the image field <NUM> are rectangular. Alternatively, it is also possible for the object field <NUM> and the image field <NUM> to have a bent or curved embodiment, that is to say, in particular, a partial ring shape. The object field <NUM> and the image field <NUM> have an x/y-aspect ratio of greater than <NUM>. Therefore, the object field <NUM> has a longer object field dimension in the x-direction and a shorter object field dimension in the y-direction. These object field dimensions extend along the field coordinates x and y.

One of the exemplary embodiments known from the prior art may be used for the projection optical unit <NUM>. What is imaged in this case as an object is a portion of a reflection mask <NUM>, also referred to as reticle, coinciding with the object field <NUM>. The reticle <NUM> is carried by a reticle holder 10a. The reticle holder 10a is displaced by a reticle displacement drive 10b.

The imaging by way of the projection optical unit <NUM> is implemented on the surface of a substrate <NUM> in the form of a wafer, which is carried by a substrate holder <NUM>. The substrate holder <NUM> is displaced by a wafer or substrate displacement drive 12a.

<FIG> schematically illustrates, between the reticle <NUM> and the projection optical unit <NUM>, a ray beam <NUM> of the illumination light <NUM> that enters into said projection optical unit and, between the projection optical unit <NUM> and the substrate <NUM>, a ray beam <NUM> of the illumination light <NUM> that emerges from the projection optical unit <NUM>. An image field-side numerical aperture (NA) of the projection optical unit <NUM> is not reproduced to scale in <FIG>.

The projection exposure apparatus <NUM> is of the scanner type. Both the reticle <NUM> and the substrate <NUM> are scanned in the y-direction during the operation of the projection exposure apparatus <NUM>. A stepper type of the projection exposure apparatus <NUM>, in which a stepwise displacement of the reticle <NUM> and of the substrate <NUM> in the y-direction is effected between individual exposures of the substrate <NUM>, is also possible. These displacements are effected synchronously to one another by an appropriate actuation of the displacement drives 10b and 12a.

<FIG> shows a meridional section of an EUV collector mirror <NUM> which is part of the light source module <NUM>, in a meridional section. A reflection surface <NUM> of the EUV collector mirror <NUM> serves to reflect the illumination light which is not shown in <FIG> impinging on the reflection surface <NUM> from a source region <NUM> to the subsequent EUV illumination optical unit <NUM>. To this end, the reflection surface <NUM> has an ellipsoidal shape which is rotationally symmetric with respect to an optical axis <NUM>. The source region <NUM> is arranged in one focal region of the ellipsoidal shape of the reflection surface <NUM>. An intermediate focus not shown in <FIG> which serves to discriminate the usable EUV illumination light <NUM> from other wavelengths and also from debris is located at the other focal point of this ellipsoidal shape.

<FIG> shows a magnified section of the reflection surface <NUM> of the EUV collector mirror <NUM>. Schematically shown in this magnified view is a pump light grating structure <NUM> including periodically alternating positive structures <NUM> ("mountains") and negative structures <NUM> ("valleys"). Such periodicity of the grating structure <NUM> is characterized by a grating pitch p.

The pump light grating structure <NUM> is designed to retroreflect pump light <NUM> (compare also <FIG>) impinging upon the pump light grating structure <NUM> from the source region <NUM> back to the source region.

The pump light <NUM> is emitted from a pump light source <NUM> as shown schematically in <FIG>. The pump light source <NUM> is a CO<NUM> laser source producing pump light having a wavelength around <NUM>, e.g. a pump light wavelength of <NUM>. Alternatively, the pump light source <NUM> may be a Nd based solid state laser source, e.g. a Nd:YAG laser producing a pump light wavelength around <NUM>, e.g. a pump light wavelength of <NUM>. The wavelength of the pump light <NUM> deviates from the wavelength of the illumination light <NUM>, i.e. from the wavelength of the usable EUV light.

The pump light <NUM> is pulsed. The pump light source <NUM> is a MOPA (master oscillator power amplifier) laser source.

The collimated pump light <NUM> passes through a through hole <NUM> arranged in the reflection surface <NUM> of the EUV collector mirror <NUM> and impinges on a tin droplet <NUM> arranged in the source region <NUM> to produce the illumination light <NUM> not shown in <FIG>. The light path of the pump light <NUM> from the pump light source <NUM> to the source region <NUM> is collinear with the optical axis <NUM> of the reflection surface <NUM> of the EUV collector mirror <NUM>.

The tin droplet <NUM> has a spherical shape, i.e. has no pancake shape when being impinged upon by the pump light <NUM>.

Part of the pump light <NUM> impinging upon the tin droplet <NUM> is absorbed by the tin droplet <NUM>. Another part of the impinging pump light <NUM> is reflected from the tin droplet <NUM>. Beam paths of such reflected pump light <NUM> are exemplified shown as pump light rays <NUM>r in <FIG>. Due to the spherical shape of the tin droplet <NUM>, the reflected pump light rays <NUM>r impinge upon the reflection surface <NUM> over a wide area thereof which carries the pump light grating structure <NUM> as schematically shown in <FIG>.

<FIG> also shows schematically the retroreflecting conditions of one exemplified reflected pump light rays <NUM>r. Such pump light ray <NUM>r impinges upon the reflection surface <NUM> with an angle of incidence α which is also denoted as Θr. Such angle of incidence Θr depends upon the radial distance of an impingement point IP of the pump light ray <NUM>r on the reflection surface <NUM> from the optical axis <NUM>. Such distance between the impingement point IP and the optical axis <NUM> in <FIG> is denoted as r.

The pitch p of the pump light grating structure <NUM> varies over the reflection surface <NUM> depending on the distance r of the respective positive and negative structures <NUM>/<NUM> to the optical axis according to the following equation: <MAT> Here.

A small angle of incidence Θr according to the above equation leads to a larger pitch p and, vice versa, a large angle of incidence Θr leads to a smaller pitch p. Depending on the incidence geometry, i.e. depending on the arrangement of the reflection surface <NUM>, its curvature and the position of the source region, this leads to the following variants regarding the dependency of the pitch from the distance r of the respective rating structures <NUM>/<NUM> to the optical axis <NUM>:.

The pitch of the pump light grating structure <NUM> satisfies for the +<NUM>st order of diffraction the retroreflecting condition for each of the pump light rays <NUM>r. Consequently, all of the pump light rays <NUM>r impinging on the pump light grating structure <NUM> on the reflection surface <NUM> of the EUV collector mirror <NUM> are retroreflected as shown in <FIG> and, exemplified for one of the pump light rays <NUM>r also in <FIG>.

In addition, <FIG> also shows a diffracted beam of the -<NUM>st order of diffraction.

The pump light grating structure <NUM> is blazed for the +<NUM>st order of reflection of the pump light ray <NUM>r which is not shown in <FIG>. Thus, the +<NUM>st order of diffraction carries almost all of the energy of the incoming pump light ray 22r.

The retroreflected pump light rays <NUM>r again impinge upon the tin droplet <NUM> increasing therefore the pumping efficiency of the light source module <NUM>.

The individual pulses of the pump light <NUM> have a pulse duration (full width half max) below <NUM> ns, preferably below <NUM> ns, preferably below <NUM> ns, preferably below <NUM> ns, preferably below <NUM> ns, preferably below <NUM> ns, preferably below <NUM> ns.

In particular, a rise time of the pump light pulse between a low light level which is less than <NUM> % of the maximum pulse intensity and a high light level which is more than <NUM> % of the maximal pulse intensity is below <NUM> ns, below <NUM> ns, or even below <NUM> ns. Such short pulse duration and/or such small rise time leads to a good conversion efficiency from the pump light energy into the energy of the usable EUV illumination light <NUM>.

The pump light grating structure <NUM> has a reflectivity for the pump light <NUM> which is larger than <NUM> %. In particular, such reflectivity is in the range between <NUM> % and <NUM> % and can be in the range between <NUM> % and <NUM> % or in the range between <NUM> % and <NUM> %.

By interaction of the pump light <NUM> with the tin droplet <NUM>, the usable EUV illumination light <NUM> is produced having a wavelength of e.g. <NUM> or <NUM>.

Claim 1:
EUV collector mirror (<NUM>)
- having a reflection surface (<NUM>) to reflect usable EUV light (<NUM>) which impinges on the reflection surface (<NUM>) from a source region (<NUM>) to a subsequent EUV optics (<NUM>, <NUM>),
- wherein the reflection surface (<NUM>) carries a pump light grating structure (<NUM>) being designed to retroreflect pump light (<NUM>) which impinges upon the pump light grating structure (<NUM>) from the source region (<NUM>) back to the source region (<NUM>), the pump light (<NUM>) having a wavelength (λPL) deviating from the wavelength of the usable EUV light (<NUM>),
- wherein a pitch of the pump light grating structure (<NUM>) varies over the reflective surface (<NUM>) of the EUV collector mirror (<NUM>).