Open Access Article
Liam Alexis
a,
Gangchen Ren
a,
Samuel Kielarb,
Jinghang Daia and
Zhiting Tian
*a
aCornell University Sibley School of Mechanical and Aerospace Engineering, Cornell University, Ithaca, New York 14853, USA. E-mail: zt223@cornell.edu
bCornell University Department of Materials Science and Engineering, Cornell University, Ithaca, New York 14853, USA
First published on 19th May 2026
High-electron-mobility-transistor (HEMT) devices, which implement wide-bandgap (WBG) or ultra-wide-bandgap (UWBG) semiconductors, permit the high-voltage and high-frequency regimes necessary for 5G/6G communications and high-power electronics, but are inhibited by the associated adverse temperature rises. A critical barrier to designing effective thermal dissipation architectures is the lack of accurate temperature information provided by current thermal modeling efforts. We develop an ab initio phonon Monte Carlo (MC) framework for nanoscale, temporal temperature mapping of HEMT devices that leverages ab initio mode- and temperature-dependent phonon properties and combines ballistic phonon transport and interfacial phonon transmission to capture thermal transport across multilayered structures. We then apply it to an AlN/GaN HEMT device and demonstrate that the decreased thermal conductivity with increasing temperature and decreasing size and the phonon reflection at AlN/GaN interfaces lead to a significantly higher temperature in the hot spot area than conventional technology computer-aided design (TCAD) prediction (at 7.61 W mm−1 and 8.43 × 105 W mm−3 heat flux, we observe a ∼80 K difference), introducing secondary heating zones and exacerbating temperature discontinuities across material interfaces. The detailed temperature map with temporal evolution not only advances our understanding of the heat dissipation process in the HEMT devices but also reiterates the necessity of accurate phonon modeling for hotspot temperature prediction. This framework can be widely applied to predict the temperature profiles of various electronic devices, including those beyond HEMTs.
Technology computer-aided design (TCAD) simulations have been used to simulate this self-heating effect via the modeling of the electric fields generated within the materials of an HEMT device with given voltage inputs. Given heat generation, conventional TCAD models produce steady-state temperature mapping by utilizing diffusive heat transport models with constant thermal conductivities and no thermal interface resistances between materials. While these TCAD models provide a starting point for estimating the temperature rise from the self-heating effect, further models require integration of (1) size-dependent thermal conductivity, (2) temperature-dependent thermal conductivity, (3) phonon interface transmission and reflection, and (4) transient temperature evolution to precisely predict the hot spot temperature and temperature gradient across the device.
Therefore, we have developed an ab initio phonon Monte Carlo (MC) framework to address the critical needs. By utilizing a phonon MC approach and integrating first-principles mode-dependent phonon inputs, our ab initio MC framework directly captures the (1) ballistic phonon transport and, thus, the size effect, (2) temperature-dependent phonon lifetimes and, thus, the temperature-dependence of thermal conductivity, (3) frequency-dependent phonon interface transmission at AlN/GaN interfaces from an advanced atomistic Green's function method, and (4) temperature evolution with time via tracking the phonon propagation.
Traditional phonon MC uses empirical phonon properties.11–13 While ab initio phonon inputs have been implemented for MC in recent studies,14–21 which focused on characterizing the effects of dopants18,19 and heat spreading20,21 and analyzing the effectiveness of MC approaches,19 one major challenge in multi-material ab initio MC simulations remains—the accurate description of phonon transmission across interfaces. While other works utilized the diffuse mismatch model20 and generalized thermal resistance constants19 to describe phonon transport and thermal resistance across interfaces, we have focused on phonon interfacial transport using the atomistic Green's function (AGF) method with first-principles force constants from density functional theory (DFT) calculations.22,23 In this work, we integrate temperature- and mode-dependent phonon scattering rates24,25 and frequency-dependent interface transmission,22,23 all from first principles, to allow accurate phonon tracking and temperature mapping. We use an AlN/GaN HEMT device as an example to show the application of this ab initio MC framework. By comparing it with traditional TCAD simulations, we demonstrate the importance of preserving nanoscale phonon physics for accurately predicting hotspot temperatures. Otherwise, the hotspot temperature can be significantly underestimated, thereby affecting thermal management strategies.19
For our AGF application, the AlN/GaN structure (Fig. 2) was divided into three parts: the left lead (bulk GaN), the central region (parts of bulk GaN and AlN, AlN/GaN interface), and the right lead (bulk AlN). Here, the 2nd-order DFT FCs of the leads and the interface were separately obtained from QE29 and Phonopy.30 The details can be found in the SI. We want to highlight that we used FCs of the AlN/GaN interface directly obtained from DFT calculations rather than the commonly simplified model of using FCs of one material and only changing the atomic mass for the other. Note that the pseudopotentials used for the interfacial force–constant calculations differ from those employed in the GaN and AlN DFT calculations. Nevertheless, rigorous convergence tests confirm that these differences do not affect the results. The calculated phonon transmission is shown in Fig. 3a. The corresponding phonon transmittance (probability, τ) can be calculated by normalizing the transmission with that of the pure material on the incident phonon side, as shown in eqn (1). The results are shown in Fig. 3b, which is the probability we use for a phonon to transmit across an interface.
![]() | (1) |
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| Fig. 2 AlN/GaN interface structure showing left and right leads and the central region, with distinct AlN and GaN bulk layers and the interface between them, respectively. | ||
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| Fig. 3 (a) Calculated GaN, AlN, and GaN/AlN transmission functions using AGF. (b) Phonon transmittance calculated from the transmission function. | ||
![]() | (2) |
is the ferroelectric polarization, q is the elementary electronic charge, p is the hole density, n is the electron density, ND is the concentration of ionized donors, NA is the concentration of ionized acceptors, and ρtrap is the charge density contributed by traps and fixed charges. Continuity equations for electrons and holes are used to describe charge conservation in eqn (3) and (4),
![]() | (3) |
![]() | (4) |
is the electron current density,
is the hole current density, and Rnet,n and Rnet,p are the electron and hole net recombination rates, respectively. The thermodynamic model is activated to analyze the self-heating effect of the device. It is an extension of the drift-diffusion model by including the temperature gradient for current density calculation, as shown in eqn (5) and (6),
![]() | (5) |
![]() | (6) |
![]() | (7) |
Thermal boundary contact resistance (3.9 × 10−5 cm2 K W−1) conditions were given by referring to the literature results.32 The Caughey–Thomas highfield saturation model was used for the mobility. Relevant GaN material physics were included, such as Shockley–Reed–Hall (SRH) and radiative recombination models, piezoelectric polarization, material anisotropy, thermionic emission at heterointerfaces, and interface charge trapping. Also, a nonlocal barrier tunneling model was used for the electrodes to account for the electron tunneling between the GaN valence band and the metal conduction bands.
![]() | (8) |
![]() | (9) |
The PDF is then produced by first finding Ni, the equilibrium number of phonons per unit volume in the ith spectral interval for each polarization, which is then combined to produce our ω parametrized PDF, Fi, and our polarization statistical function Pi.
![]() | (10) |
![]() | (11) |
![]() | (12) |
The simulated volume is broken up into cells of volume, Vc, with side length, xc, which are related to our lattice unit cell volume, Vu, via the scale factor,
. In combination with eqn (8) and (10), we use this sf to determine our initial phonon population at our desired temperature and scale it to our volume of increased temperature. Phonons are then randomly drawn with frequency and polarization determined by Fi and Pi. The phonon group velocity and lifetime are then assigned according to phonon frequency and temperature.
Phonon drift is characterized by linear ballistic steps of Δx calculated using
| Δx = Δtvi | (13) |
Two three-phonon scattering events are of interest to our model – normal and Umklapp scattering; however, the intricacies of each lie outside the scope of this analysis, and the statistics of both are factored into the DFT calculated lifetime and DoS. Scattering is handled computationally by resetting the frequency of our scattered phonon, resampling a frequency from our PDF, and reassigning lifetime and group velocity based on frequency and temperature. Random sampling of a new frequency can result in a violation of energy conservation rules. Therefore, we add or delete phonons at the end of each timestep until energy conservation is maintained.
Our main tool in determining which phonons scatter is the lifetime. The lifetime values provide us with the average time between collisions, and according to that, a time of existence scheme is implemented to determine the age (time since initialization), tage, of each phonon with each step. This is then related to the scattering probability, Ps, and the lifetime, τ, via
![]() | (14) |
This scattering probability is a modified version of the scattering function defined in the literature11 and takes into consideration the increasing probability of a scattering event occurring as the tage increases. As this tage approaches the lifetime, the overall scattering probability will increase as
approaches infinity.
The final runtime consideration necessary to holistically simulate our device geometry is transmission. The transmittance is presented as a normalized probability dependent on the phonon frequency. As phonons approach the material interface, a random number is drawn and compared with their transmittance. If a higher number is drawn, the phonon is reflected; if a lower number is drawn, the phonon is transmitted. Upon transmission, the frequency is maintained, but the group velocity and lifetime are changed according to the dynamics of the new material. More detailed descriptions can be found in the literature.11
Adherence to both the expected distribution as determined by the DoS and BE distribution and the interfacial transmittance statistics as defined by AGF calculations is shown in Fig. 5, with the expected statistical trendlines being closely followed by the histograms of initialized and transmitted phonons, respectively.
This modeled device has a background temperature of 300 K, which represents the environment in which the device is expected to operate. Instead of increasing the number of phonons or reducing the ratio of the simulated vs. real number of phonons to simulate higher temperature, we treat 300 K as the background and introduce thermal phonons on top of the background energy. We intentionally keep a large ratio of the simulated vs. real number of phonons (1
:
10) to best represent the actual dynamics. If we were to directly simulate the 300 K phonon ensemble within our volume, we would deal with the order of 109 simulated phonons, which only increases with heat injection.
Deviated density of states (DoS) and scattering functions were utilized in our simulations, which allow us to build our phonon ensemble on top of an equilibrium background phonon flux maintained at 300 K to reduce the computational cost. This relies on adjusted probability distributions and scattering mechanics obtained via the calculation of the deviated phonon occupation 〈nd〉.33
Two simulation modes are utilized within our study. The first mode focuses on the time interval from heat initialization at 0 ps to 30 ps. This simulated space is broken into 1 nm3 cells and cycles through 400 iterations of 7.5 × 10−2 ps each. This ensures that phonons are allowed to begin impinging upon each AlN/GaN interface, focusing on the initial effects around the z20 interface. The second mode focuses on longer-term interactions up to 200 ps. This simulation space is broken into 8 nm3 cells and cycles through 1300 iterations of 1.55 × 10−1 ps each. This allows us to observe longer-scale temporal effects and the development of thermal gradients that encompass the z12 interface. We place the same heat flux volume on the GaN side of the z20 interface as TCAD.
For the shorter time simulation using the 1 nm3 resolution, our MC attains a temperature of 358 K at 15 ps (Fig. 7a) and a maximum temperature of 382 K at 30 ps (Fig. 7b). The hot spot in the MC simulation attains a higher temperature than the steady-state hot spot temperature from TCAD of 354 K due to the influence of temperature and size on scattering rates and thermal conductivity, as well as the thermal interface resistance. Scattering rates increase with increasing temperature due to the Umklapp phonon scattering, meaning that using a constant thermal conductivity value at room temperature in TCAD overestimates thermal conductivity and underestimates the temperature rise. In addition, the nm-thick layers strongly suppress the thermal conductivity from the bulk value due to the boundary scattering (size effect). Using a bulk value also contributes to overestimating thermal conductivity and underestimating temperature rise in TCAD. Moreover, there is thermal resistance at the material interfaces, and one should expect a temperature discontinuity at the interface accordingly. A temperature drop was not seen in TCAD because the thermal interface resistance was not considered. In contrast, our MC framework integrates the first-principles phonon interface transmission for the first time and properly captures the temperature drop at the interface. With these statistical effects, as phonons hit the z20 interface from GaN to AlN, only 15–20% of phonons are transmitted, with the other 80–85% being reflected back into the GaN layer; not only is AlN heating less due to receiving only a small portion of phonons, but heating within GaN is augmented due to losing a small portion of phonons to the AlN layer, further increasing the temperature drop across the z20 interface.
As time progresses to 30 ps (Fig. 7b) the interfacial transmittance trend continues with the reflection of phonons back into the GaN layer at the z20 interface, further increasing the GaN temperature and increasing the temperature drop. The interfacial effects also increase the size of the central hot spot region and broaden the surrounding excited region on the GaN side, with minimal heating still observed on the AlN side.
Looking further past the hot spot area into the lower range (below z = 0), a runtime of 30 ps also begins to show the onset of temperature drops at the z12 interface, this being totally attributed to the 15%–20% phonon transmission across the interface. The z = 0 to z = −12 range shows lower temperatures directly adjacent to the hot spot area because phonons generated in the hot spot area have been slowed down by the increased temperature via the increased scattering, impeding their movement. The reflected phonons from the z20 interface influence faster heating on the GaN side of the z20 interface, increasing scattering rates, reducing thermal conductivity, and producing a positive feedback temperature loop. As phonons are reflected, the hot spot temperature increases. Phonons generated in the hot region are more likely to scatter, and with each scattering, the velocity randomizes, delaying their movement toward the z12 interface and necessitating analysis at later times.
To allow for a longer simulation time, we switched to the analysis with the 8 nm3 cell size. Fig. 8a and b display the temperature profiles at 100 ps and 200 ps, respectively, where the interfacial effects are even more profound with more drastic temperature drops than the short runtimes (Fig. 7). Fig. 8c shows the temperature profile along the x = 0 line at various times. The hot spot temperature increases with time and starts to plateau at 200 ps. The maximum temperature is observed at the interface. The z20 interfacial temperature drop is also on the order of ∼100 K, with a comparable temperature drop in the GaN layer from the max temperature zone not seen until around 20 nm away from the z20 interface. Unlike the linear temperature profile one would expect within the GaN layer from Fourier's law, the nonlinearity in Fig. 8c highlights the complex nature of varying thermal conductivity with temperature, constant heat flux input, and transient conditions, combined with the influence of the interfaces.
The hot spot size continues to grow compared to the 1 nm3 case at shorter times, as expected. Between 100 ps and 200 ps, the central hot spot area (>400 K) extends marginally, with the outside area expanding ∼10 nm. At the z12 interface, we observe a local maximum via secondary heating events influenced by the reflection effects of the z12 interface. The area between the hot spot and the z12 interface experiences a relatively even temperature distribution due to a balancing effect from the hot spot phonons and the reflected z12 phonons. This secondary heating zone is not observed at all if there is no interface.
The maximum temperature within this hot spot is 430 K, representing a ∼80 K increase from the TCAD-determined conditions. This area primarily encompasses a 30 nm × 5 nm area on the GaN side of the z20 interface. Surrounding this is a region of 400 K that encapsulates a 40 nm × 10 nm area, which leads to the 10 K–100 K excitation region extending down to the z20 boundary.
For a more direct comparison of the effect of size and temperature effects within MC to the TCAD simulations, the MC simulation was run without the frequency-based statistical transmittance of the material interfaces. All phonons that reach interfaces (with velocity vectors pointing across the interfaces) are allowed to cross over and adopt the dynamics of the new material. Fig. 9 shows the temperature distribution at two timesteps with our 1 nm resolution. A maximum temperature of 380 K is obtained from this simulation with no indication of dominant interfacial resistance or secondary heating zones, with more even heating occurring above and below the central hot spot region and a slightly quicker drop seen at z20 due to the higher AlN thermal conductivity. This represents a ∼30 K increase in maximum temperature compared to the TCAD simulation and a decrease of ∼50 K compared to the MC with interfaces. This increase in temperature compared to the TCAD case is only due to the size and temperature effects and allows us to isolate the influence of interfaces on the thermal evolution within the multilayered architecture. When combined, these interfacial, size and temperature-dependent effects build upon each other, resulting in an 80 K increase in temperature for the MC case with interfaces.
Another TCAD case and MC simulation were run with a 6 V drain voltage, producing a maximum TCAD temperature of 387 K and the corresponding maximum MC temperature of 480 K. Figures outlining these results are included in the SI (Fig. S4) and show a similar secondary heating zone at the lower interface with higher temperatures in the MC case.
The consolidation of the probabilistic methods utilized to capture both intra- and inter-material phonon movement within this MC simulation provides significant insight into the effect of interfaces on the temporal and spatial propagation of various phonon frequencies. Our framework preserves the accuracy of ab initio calculations and the statistical methods typically seen in MC simulations while allowing isolation of the interfacial effects, allowing us to directly observe the resultant differences in temperature evolution and distribution, the importance of temperature-dependent thermal effects within thermal analysis and the influence of material interfaces on all these effects.
Supplementary information (SI) is available. See DOI: https://doi.org/10.1039/d5nr03065j.
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