Atom probes are analytical instruments that analyze the atomic-level composition of materials by field evaporation of atoms and small molecules from a specimen, and measuring their time of flight (TOF) from the specimen to a detector some distance away. See, for example, U.S. Pat. Nos. 5,061,850, 5,440,124 and 6,576,900 to Kelly et al.; International Publications WO 99/14793 and WO2004/111604; and Kelly et al., Ultramicroscopy 62:29-42 (1996).
In a typical atom probe, the specimen is in the form of a sharp tip (often having a tip radius of ˜50 nm), and is held at a semi-static standing voltage that is below that necessary to cause field evaporation of the atoms at the tip of the specimen. A counter electrode, which usually has an aperture therein, is spaced about or at a slight distance from the specimen tip, with the specimen tip pointing through the aperture. A pulsed (usually negative) voltage is applied to the counter electrode, and/or a pulsed (usually positive) voltage is applied to the specimen, with sufficient magnitude to ionize the specimen tip, preferably a single atom at a time. Ionization usually does not occur with every pulse, and rather occurs once per several pulses (often with one ionization event for every 10-100 pulses). The amplitude of this pulse, called the “ionization pulse,” is typically 10% to 25% of the standing voltage.
During the initial stages of analysis the specimen tip rapidly adopts a nominally hemispherical end form, since any atom that is more “exposed” to the ionizing field will be preferentially evaporated. The hemispherical end form of the tip creates an electric field that is nearly radial, and consequently when a specimen atom is ionized, it flies radially away from the specimen, through the aperture of any counter electrode, and toward a 2-dimensional (2D) particle detector (generally located 10-100 mm away from the specimen tip). The position at which the ion impacts the detector is measured, and this impact position is uniquely correlated with the ion's original position on the specimen surface. In this manner the specimen tip (of for example 50 nm size) is effectively projected onto the detector (of for example 40-100 mm size), yielding roughly a million-fold factor of magnification.
Apart from monitoring the ion impact position, time of flight (TOF) mass spectroscopy is performed on the evaporated ions by measuring the time between the application of the ionization pulse (which roughly indicates the time of ion departure from the specimen) and the subsequent ion impact at the detector. The TOF measurement can be directly correlated to the mass to charge ratio (MTC) of the ion, which in turn can allow identification of the ionized atomic (or molecular) species. Thus, by utilizing the magnified “image” of the specimen and the elemental identification provided by the TOF mass spectroscopy, a 3-dimensional atom map of the specimen can be created.
One of the inherent limitations of atom probes is that for a given MTC ratio (i.e., for a particular ionized species), a range of TOF values can be measured. This inherent spread in the TOF measurement limits the ability of atom probe techniques to distinguish between atomic (or molecular) species of nearly the same MTC ratio. In other words, the peaks in the TOF histogram of two different species may overlap, making it difficult to assign a specific MTC ratio to each species, and thereby making it difficult to identify the ions that are recorded in the overlapped region. Thus, there is a limit to the mass resolution (ionic species identification) capability of an atom probe.
A second order effect of the finite mass resolution is decreased sensitivity to low concentration species. All atom probes record spurious events—for example, ionization events that occur independent of ionization pulses, “rogue” species in the atom probe which impact the detector, etc.—that contribute to a finite noise floor. In order for a given species to be definitively identified, it must be present in quantities that are statistically significant compared with the noise floor. The smaller the range in measured TOF, the more quickly a valid signal will emerge from the noise.
One factor reducing the mass resolution in all atom probes that utilize an ionization pulse to initiate field evaporation of specimen ions is the (relatively small) uncertainty in the time of ion departure upon application of the ionization pulse, and the corresponding energy (velocity) that is imparted to the departing ion. This phenomenon is illustrated in
As a result of the exponential nature of field evaporation, nearly all specimen ion evaporation events occur very near the peak voltage of the ionization pulse 100, with the range Δt in
After being ionized, the atoms or molecules are accelerated by the electric field caused by the combination of the standing voltage and the ionization pulse voltage until the ions enter a relatively field-free region just inside the aperture of the counter electrode (if one is present). An atom or molecule that is ionized before the peak of the ionization pulse experiences an increasing field as it is accelerating away from the specimen and will therefore acquire more energy (i.e. velocity) as compared an atom or molecule that is ionized at the same voltage, but after the peak. Thus, there is a range of ion departure velocities, with most ions having velocities varying in the range Δv shown in
Therefore, any given atom or molecule that is ionized in an atom probe will have an uncertainty Δt in the exact instant of ionization, and in the exact velocity (Δv) it acquires during and after the ionization process. As a given ion type traverses the distance from the specimen to the detector, the combination of Δt and Δv gives rise to a spread in the measured time of flight. This variation limits the ability to resolve species that have nearly identical MTC ratios. By varying the design of the atom probe, the exact form of
In practice, it is the velocity distribution Δv that creates the majority of the uncertainty in measured TOF, and consequently limits mass resolution in conventional atom probes. Traditionally, the atom probe and mass spectrometry communities refer to the velocity distribution Δv inherent in atom probes as the “energy deficit,” and the process of reducing the spread in the velocity distribution is called “energy compensation”. (Additionally, it should be understood that “velocity distribution” usually refers to the distribution of velocities for a particular species of ions evaporated from a specimen, not to the far wider distribution of velocities across all species.) An atom probe without any form of energy compensation will typically possess a mass resolution of 1 part in 80-200 as measured by the full-width at half-maximum (FWHM) of a given mass peak in the spectrum. A variety of energy compensation schemes have been employed, including:
(1) Reflectrons. A reflectron is essentially an electrostatic mirror. Ions from the specimen are directed into the reflectron, where they stopped by a uniform decelerating electrostatic field. The same field then accelerates the ion back out of the reflectron at a small angle to the incident beam. Faster ions penetrate more deeply into the reflectron than slower ions, and therefore spend more time in the reflectron. If the distances between the specimen, reflectron, and detector are carefully chosen, the spread in measured TOP times can be reduced. Mass resolutions of 1 part in 800 (FWHM) have been reported for atom probes with reflectrons. The main disadvantage of reflectrons is that only a small range in the incident angle of incoming ions is properly reflected, limiting the use of the reflectron to 1-D atom probes, and to 3-D atom probes that have a relatively small angle of view.
(2) Post Acceleration. In post acceleration, after the initial ionization event, all of the ions are accelerated to a significantly higher velocity by a constant voltage, known as a post-accelerating voltage, for the remainder of the flight distance to the detector. By increasing the velocity of the ions by a constant voltage, the fraction of the velocity due to the ionization pulse voltage—which is the source of the velocity variation—is minimized, and mass resolution is increased. The main disadvantages to this approach are that the amount of mass resolution improvement is asymptotically limited to a modest amount for reasonable instrument geometries and post acceleration voltages. Experimental results employing this technique suggest that mass resolutions of 1:400 to 1:600 (FWHM) are possible.
(3) 163° Poschenrieder Energy Compensating lens. This technique employs a semicircular ion flight path of 163° created by electrostatic fields to compensate for the differences in ion velocities. A faster ion traverses the semicircular flight path with a slightly larger radius than that of a slower ion, and as a result, it has a longer flight length. If the proper dimensions are calculated—the 163° angle is the result of analytical calculations—the different flight paths/lengths of the ions result in the ions having the same flight times to the detector. Mass resolutions of 1:5000 (FWHM) have been achieved with this technique. The main limitation of this technique is that it destroys information related to ion position, and is therefore limited to 1D atom probes where knowledge of the original positions of the ions on the specimen is not needed.
(4) Ion Deceleration Via a Counter Electrode. This technique is schematically depicted in
It would therefore be useful to have available some means for attaining better mass resolution in atom probes while reducing or eliminating the difficulties involved with the prior mass resolution enhancement techniques.
The invention, which is defined by the claims set forth at the end of this document, is directed to devices and methods which at least partially alleviate the aforementioned problems. A basic understanding of some of the preferred features of the invention can be attained from a review of the following brief summary of the invention, with more details being provided elsewhere in this document.
In an atom probe (or some other mass spectrometer) wherein a specimen is subjected to ionizing pulses which induce field evaporation of ions from the specimen, energy compensation is performed by subjecting the evaporated ions to corrective pulses which are synchronized with the ionizing pulses. These corrective pulses have a timing and magnitude such that they reduce the velocity distribution of the evaporated ions, i.e., evaporated ions of a given mass-to-charge ratio (and thus of a given species) will not have as wide of a range of velocities as they depart the specimen. A preferred arrangement is to provide each corrective pulse from a counter electrode in response to a corresponding one of the ionizing pulses. An exemplary version of this arrangement is depicted in
The corrective pulse may be generated on the counter electrode by a passive component, i.e., one or more resistors, capacitors, inductors, diodes, and/or other components which do not require an independent power supply. Such an arrangement is shown in
Alternatively (or additionally), the corrective pulse may be generated on the counter electrode by an active component, i.e., some component such as a pulser, an amplifier, and/or a biased diode which requires an independent power supply to generate the corrective pulse in response to an ionizing pulse. In this arrangement, exemplified in
Further advantages, features, and objects of the invention will be apparent from the following detailed description of the invention in conjunction with the associated drawings.
The invention provides an energy compensation arrangement for increasing the mass resolution in atom probes and other mass spectrometers which employ a pulsed ionization mechanism. Looking to the exemplary version of the invention depicted in
The amplitude and form of the corrective pulse delivered to the second counter electrode 314 can be designed to reduce the effect of the systematic variation in Δt and Δv on the measured TOF. In practice, the desired form (timing, shape and/or amplitude) of the corrective pulse can be determined by either directly measuring the TOF spread without any corrective pulsing and then forming the corrective pulse to reduce the spread during subsequent ionization pulses on the first counter electrode 310, or by using computer modeling to determine a predicted TOF spread (without corrective pulsing) and devising an appropriate form for the corrective pulse. A combination of both approaches could also be used, e.g., by using computer modeling to devise an initial corrective pulse form, and then refining it empirically after specimen ionization begins and experimental TOF data is available. Since the shape of the corrective pulse (in particular, its skewness about its peak) will depend on many variables including the spacing between the first and second counter electrodes, operational voltages, ion flight distance, and other machine/material parameters, it is preferred that the pulse shape be at least partially based on empirical data so as to achieve better improvement in mass resolution.
In practice, a simple way to generate the corrective pulse on the second counter electrode 314 is to electrically couple the ionization pulse to the second counter electrode 314. By using an appropriate combination of electronic devices (e.g. passive devices such as resistors, inductors, capacitors, diodes, etc. or combinations of these devices, or active devices such as pursers, amplifiers, biased diodes, etc. or combinations of these devices), the corrective pulse can be tailored to an appropriate form for providing reduction in TOF spread. There are limits to the possible pulse shapes that can be generated from the ionization pulse, particularly where passive coupling is used, so the optimal corrective pulse shape may not always be obtained. Nevertheless, in experimental versions of the invention, even imperfect corrective pulse shapes generated by use of passive coupling have resulted in significant increases in mass resolution (as will be discussed below).
A particularly elegant implementation of this technique is to exploit the fact that two closely spaced counter electrodes 310 and 314 are inherently capacitively coupled (as discussed above with reference to
This approach was experimentally implemented in a LEAP atom probe (Imago Scientific Instruments, Madison, Wis., USA), wherein a 1 kohm resistor placed between the second counter electrode 314 and ground 316 increased the mass resolution by about 20%. See
Where passive pulse shaping elements 322 are used to generate the desired corrective pulse on the second counter electrode 314, it is particularly preferred that the passive shaping elements 322 be tunable (i.e., that variable resistors, capacitors, etc. be used). This is because a variety of other parameters in the atom probe will affect mass resolution—e.g., electrode 310/314 configuration and placement, distance to the detector 304, the form of the ionization pulse, etc.- and these parameters may be changed not only between different operating sessions of the atom probe, but possibly during the course of a single session. For example, it is common to adapt the form of the ionization pulse during an operating session; in particular, its voltage is generally increased as more of the specimen 300 is ionized. As another example, it is also common to adjust the distance between the electrodes 310/314 and the detector 304 between operating sessions to obtain some desired magnification, field of view, and/or nominal mass resolution (with a discussion of such adjustment being provided in WO2004/111604). Thus, the ability to adapt resistance, capacitance, diode voltage bias, etc. values between or during operating sessions can allow the corrective pulse to be appropriately modified to obtain mass resolution enhancement for whatever operating parameters (detector distance, etc.) are presently in place. Additionally, since the amount of mass resolution enhancement will also depend to some degree on the MTC ratio of the ion species being evaporated, tunable components allow a corrective pulse to be optimized for the range of MTC ratios of greatest interest.
As noted above and as depicted in
It should be understood that the various preferred versions of the invention described above are provided to illustrate different possible features of the invention and the varying ways in which these features may be combined. Apart from combining the different features of the foregoing versions in varying ways, other modifications are also considered to be within the scope of the invention. Following is an exemplary list of such modifications.
First, it should be understood that the correctively pulsed counter electrode may take a wide variety of forms, such as an apertured plate, a funnel-like member (as depicted in
Second, it is also possible to provide additional counter electrodes—a third, fourth, and so on—which can also provide corrective pulses when desired, with the corrective pulses between the different electrodes cooperating to provide the desired mass resolution enhancement.
Third, recall from the prior discussion that some prior atom probes provided ionization pulses not to a counter electrode, but to the specimen itself (via the specimen mount). The corrective pulses of the invention could be generated from any source of ionizing pulses, whether the ionizing pulses are provided on a first counter electrode, on the specimen, or on both the specimen and the counter electrode. To illustrate, the invention could be utilized in a system such as that described in International Application PCT/US2004027062, wherein ionization pulses are delivered via a laser. In this case, only a single counter electrode is needed (though more could be present), and it could bear a corrective pulse which is synchronized with respect to the laser pulse delivery.
Fourth, the invention may utilize corrective pulses which have timing dependent on ionization pulses, but which otherwise have shapes and amplitudes which are independent of the ionization pulses. As an example, the pulse shaping device 422 could always emit a corrective pulse having the same size and shape, with the corrective pulse simply being synchronized with respect to the ionization pulse to adjust the velocities of ions having late evaporation. While such corrective pulses may be less than optimal, they should nonetheless provide some improvement in mass resolution.
Fifth, as discussed above, the corrective pulses may be generated by use of a passive component (including resistors, capacitors, inductors, diodes, etc. or some combination of these components), an active component (including pulsers, amplifiers, biased diodes, etc. or some combination of these components), or a combination of active and passive components. It should be understood that the location of these components may vary, i.e., they may be in the vacuum chamber of the atom probe, or remote from the counter electrode with their corrective pulses provided by some feedthrough connection (preferably one which is tailored to provide beneficial impedance).
The invention is not intended to be limited to the preferred versions of the invention described above, but rather is intended to be limited only by the claims set out below. Thus, the invention encompasses all different versions that fall literally or equivalently within the scope of these claims.
Filing Document | Filing Date | Country | Kind | 371c Date |
---|---|---|---|---|
PCT/US2005/021552 | 6/17/2005 | WO | 00 | 10/24/2008 |
Number | Date | Country | |
---|---|---|---|
60581508 | Jun 2004 | US |