Download presentation
Presentation is loading. Please wait.
Published byCecilia Mosley Modified over 6 years ago
1
NBTI and Spin Dependent Charge Pumping in 4H-SiC MOSFETs
Mark A. Anders, Patrick M. Lenahan, Pennsylvania State University Aivars Lelis, US Army Research Laboratory
2
Physical Basis for ESR (Simple Case) At resonance, spin flips
Deviations from the resonance condition provide useful information about the nature of specific defects Energy Magnetic Field Electron-Nuclear Hyperfine Interaction: due to nearby nucleus with magnetic moment g bH + mIA Energy Magnetic Field Spin-Orbit Coupling: due to electron’s orbital angular momentum about the nucleus g bH At resonance, spin flips
3
Spin-Orbit Coupling In the data shown, the factor most responsible for deviations from hv=geβH Bohr model: electron orbits nucleus; angular momentum n h (units of h). To an observer on the electron, it looks like the nucleus is orbiting the electron. The greater the nuclear charge and orbital angular momentum quantum number, the greater the spin orbit coupling. The orbiting nucleus looks like a current loop generating a magnetic field. This contribution is expressed in the g tensor.
4
Electrically Detected Magnetic Resonance (EDMR)
Problem Conventional EPR has a sensitivity of about 1010 total paramagnetic defects It is also sensitive to ALL paramagnetic defects in a sample We want to identify defects in transistors We want to know what different defects do to device performance A main problem for electronic materials science is performing resonance inside fully processed transistors in integrated circuits EDMR provides sensitivity about 7 orders of magnitude higher than conventional EPR Solution: EDMR, spin dependent recombination (SDR), and spin dependent trap-assisted tunneling (SDT)
5
Spin Dependent Recombination (SDR): Shockley-Read-Hall Model
6
Pauli Exclusion Principle
EDMR via SDR: Pauli Exclusion Principle
7
Background: What are these defects?
Anticipated spectrum of the negatively charged silicon vacancy with the field parallel to the c-axis utilizing the hyperfine parameters of Isoya et al. J. Isoya, T. Umeda, N. Mizuochi, N. T. Son, E. Janzen, and T. Ohshima, Phys. Status Solidi B 245(7), 1298 (2008). 7
8
Background: Silicon Vacancies
Silicon Vacancy Model Experimental Results
9
Previous Work: NBTI x5 Hydrogen or Nitrogen related defect
Pre-stress 190oC Post-stress Hydrogen or Nitrogen related defect At interface, bulk, or possibly oxide Possible nitrogen related defect At interface or bulk
10
NBTI: “Bulk Defects” +++++
Utilizing VDMOSFET geometry, we probe bulk defects Biasing scheme: Strongly accumulate channel Forward bias drain/body diode “Bulk” recombination dominant current N+ P Source i -Vg Gate P+ Vd Drain N+ SiC substrate N SiC Epi Source Gate +++++ N+ accumulated channel P+ P
11
Low Frequency EDMR 150, or 250, or 360 MHz (low field) vs. ~9.5 GHz (X-band) Broadening due to g is field/frequency dependent Broadening due to hyperfine interactions is field/frequency independent (to first order) Simulated using easyspin
12
NBTI: Hydrogen Movement in Bulk
X-band Low field Previously, X-band measurements suggests broadening due to g or hyperfine EDMR measurements at low field reveal that broadening is at least partially due to hyperfine interactions
13
The Fundamental Problem
EDMR via SDR: The Fundamental Problem This technique is appropriate for levels around mid-gap. It does not, however, address traps near the band edges. We are interested in what’s happening near the conduction band and valence band. Spin dependent charge pumping: a solution.
14
Spin Dependent Charge Pumping (SDCP)
By utilizing a pulse wave at the gate voltage, we can explore more of the band gap with larger amplitude.
15
3-level Energy Resolved Charge Pumping
semiconductor oxide G D S Waveform Generator 𝑖 … a b c time Gate Voltage (Vary b Voltage) Flood interface with holes to recombine with interface trap electrons (a) (b) (c) EF EF EF Fill Traps Allow time for traps above EF to empty
16
Enhanced sensitivity (2000x greater)
Recap: SDCP Enhanced sensitivity (2000x greater)
17
SDCP (full bandgap) vs BAE (midgap)
NO-annealed pMOSFET Probing states throughout most of the bandgap shows a different line shape and broader center line compared to only mid-gap states
18
SDCP (full bandgap) vs BAE (midgap)
The “full bandgap” spectra have g-values much lower than the “mid-gap” spectra in this sample Mid gap (BAE) spectra are mostly due to silicon vacancy
19
NO vs non-NO 350 MHz ~9.5 GHz C-axis is parallel to magnetic field
c-axis parallel to magnetic field c-axis parallel to magnetic field C-axis is parallel to magnetic field NO annealed nMOSFET has broader shoulders than an nMOSFET which did not receive an NO anneal Many abundant magnetic nuclei, likely nitrogen, would cause broadening
20
NO vs non-NO 350 MHz ~9.5 GHz NO annealed nMOSFET has a broader center line at both high and low fields Many abundant magnetic nuclei, likely nitrogen, would cause broadening
21
NO vs non-NO ~9.5 GHz The NO annealed device spectra is much broader than the non-NO device spectra More evidence for Nitrogen hyperfine interactions
22
Carbon Dangling Bonds? C dangling bond: g//c = 2.0023 g⊥c = 2.0032
J. L. Cantin et al. If carbon dangling bonds largely contributed to the interface state density, we would observe a line at g//c = and g⊥c = We do not. There are no carbon dangling bonds at the interface.
23
3-level SDCP Non-NO nMOSFET
24
3-level SDCP Non-NO nMOSFET Side peak amplitudes are reduced
Defect responsible for side peaks are not near the conduction band edge
25
Frequency-dependent SDCP
w/out NO nMOSFET NO nMOSFET Lower charge pumping frequencies probe further into the oxide Could provide a way to look a little into the gate oxide More work needs to be done to fully understand multi-frequency SDCP results
26
Prelim Results on GaN Low -field EDMR: GaN p-n diode
The complex spectra is clearly due to hyperfine interactions
27
Prelim Results on GaN EDMR Amplitude vs Gate Bias
EDMR amplitude of several different spectrum peaks Calculated recombination current
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.