Khachatur V. Manukyan
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Khachatur V. Manukyan has a total of 320 co-authors. Here are the top co-authors by number of shared publications:
Ani Aprahamian
15 shared publications- Richard James Deboer
University of Notre Dame
14 shared publications - Michael Wiescher
University of Notre Dame
13 shared publications J. Görres
10 shared publications- Alexander S. Mukasyan
Department of Chemical and Biomolecular Engineering, University of Notre Dame, Notre Dame, IN 46556, USA
8 shared publications - Wanpeng Tan
University of Notre Dame
7 shared publications
Latest Publications
- Open Access
- 9 October 2026
- Published by Elsevier in Progress in Materials Science
- Vol. 165
Next-generation materials and devices by combustion processes
- 9 October 2026
- Published by Elsevier in Progress in Materials Science
- Vol. 165
Open AccessNext-generation materials and devices by combustion processes
- Open Access
- 5 October 2026
- Published by Elsevier in SSRN Electronic Journal
Retrainable physics-integrated neural differentiable modeling of sintering across material systems
Sintering is widely used to manufacture ceramics for structural, electronic, and energy applications, but coupled densification and grain growth, material-dependent kinetics, and sparse measurements complicate predictive modeling and process design. Without reliable simulation, processing schedules are commonly developed through repeated furnace trials and post-process characterization. Here, we present Sinter-PiNDiff, a retrainable sintering physics-integrated neural differentiable framework for predicting density and grain-size evolution across ceramic systems. Two neural networks learn material-dependent densification and grain-growth coefficients within coupled sintering rate equations, while a smooth density-saturation factor attenuates densification as theoretical density is approached. The common governing structure, network architecture, and training procedure were fitted independently to published measurements for MgO, Al-doped ZnO, and CaO-doped ThO₂. Condition-wise held-out tests evaluate predictions at unseen temperatures and compositions. Sinter-PiNDiff achieved the lowest mean error in all twelve material–metric comparisons with multilayer-perceptron and residual-network baselines. For MgO, Al-doped ZnO, and CaO-doped ThO₂, respectively, density normalized root-mean-square errors were 14.6%, 10.8%, and 14.4%, and grain-size normalized root-mean-square errors were 8.6%, 12.1%, and 19.3%. Removing the evolving density from both neural-network inputs increased both density and grain-size trajectory errors in all three systems and increased ten of the twelve aggregate errors examined, supporting density-dependent kinetic feedback. Deep ensembles estimated model disagreement, although empirical coverage showed that the resulting bands were not calibrated and did not capture all model–data discrepancies. These results establish Sinter-PiNDiff as a retrainable framework for sparse-data prediction and uncertainty-informed selection of sintering conditions.
- 5 October 2026
- Published by Elsevier in SSRN Electronic Journal
Open AccessRetrainable physics-integrated neural differentiable modeling of sintering across material systems
Sintering is widely used to manufacture ceramics for structural, electronic, and energy applications, but coupled densification and grain growth, material-dependent kinetics, and sparse measurements complicate predictive modeling and process design. Without reliable simulation, processing schedules are commonly developed through repeated furnace trials and post-process characterization. Here, we present Sinter-PiNDiff, a retrainable sintering physics-integrated neural differentiable framework for predicting density and grain-size evolution across ceramic systems. Two neural networks learn material-dependent densification and grain-growth coefficients within coupled sintering rate equations, while a smooth density-saturation factor attenuates densification as theoretical density is approached. The common governing structure, network architecture, and training procedure were fitted independently to published measurements for MgO, Al-doped ZnO, and CaO-doped ThO₂. Condition-wise held-out tests evaluate predictions at unseen temperatures and compositions. Sinter-PiNDiff achieved the lowest mean error in all twelve material–metric comparisons with multilayer-perceptron and residual-network baselines. For MgO, Al-doped ZnO, and CaO-doped ThO₂, respectively, density normalized root-mean-square errors were 14.6%, 10.8%, and 14.4%, and grain-size normalized root-mean-square errors were 8.6%, 12.1%, and 19.3%. Removing the evolving density from both neural-network inputs increased both density and grain-size trajectory errors in all three systems and increased ten of the twelve aggregate errors examined, supporting density-dependent kinetic feedback. Deep ensembles estimated model disagreement, although empirical coverage showed that the resulting bands were not calibrated and did not capture all model–data discrepancies. These results establish Sinter-PiNDiff as a retrainable framework for sparse-data prediction and uncertainty-informed selection of sintering conditions.
- 24 September 2026
- Published by American Physical Society (APS) in Physical Review C
- Vol. 114 (3) , 035807
First strength measurements of low-energy resonances in the Sc 45 ( p , γ ) Ti 46 reaction and its astrophysical implications
The $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction plays an important role in both hydrostatic and explosive nucleosynthesis. During hydrostatic oxygen and silicon burning in massive stars, including dynamic processes such as convective carbon-oxygen (C-O) shell mergers, it acts as a bottleneck that regulates the reaction flow in the Sc-Ti mass region. In oxygen-neon (ONe) novae, the ejecta indicate the production of elements up to the Fe group, as observed in V1974 Cygni, and the $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction links nuclei above Ca to the Fe region. In core-collapse supernovae (CCSNe), it influences the production of the radioactive isotope $^{47}\mathrm{Sc}$. At present, the thermonuclear reaction rate is based on statistical model calculations. In this work, we report on measurements of the $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction performed using the 5 MV accelerator at the Nuclear Science Laboratory, University of Notre Dame, over a laboratory proton energy range of 526--1275 keV. We present the first direct measurements of the resonance strengths for six resonances at ${E}_{\mathrm{R}}^{\mathrm{lab}}=917.4$, 1026.0, 1031.1, 1049.7, 1059.4, and 1257.5 keV, together with integrated resonance strengths at ${E}^{\mathrm{lab}}=555$, 630, 700, 761, and 871 keV. For resonance energies below the lowest directly measured energy, available transfer-reaction data were used to estimate the resonance strengths. An updated thermonuclear reaction rate is derived, and its astrophysical implications are discussed.- 24 September 2026
- Published by American Physical Society (APS) in Physical Review C
- Vol. 114 (3) , 035807
First strength measurements of low-energy resonances in the Sc 45 ( p , γ ) Ti 46 reaction and its astrophysical implications
The $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction plays an important role in both hydrostatic and explosive nucleosynthesis. During hydrostatic oxygen and silicon burning in massive stars, including dynamic processes such as convective carbon-oxygen (C-O) shell mergers, it acts as a bottleneck that regulates the reaction flow in the Sc-Ti mass region. In oxygen-neon (ONe) novae, the ejecta indicate the production of elements up to the Fe group, as observed in V1974 Cygni, and the $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction links nuclei above Ca to the Fe region. In core-collapse supernovae (CCSNe), it influences the production of the radioactive isotope $^{47}\mathrm{Sc}$. At present, the thermonuclear reaction rate is based on statistical model calculations. In this work, we report on measurements of the $^{45}\mathrm{Sc}(p,\ensuremath{\gamma})^{46}\mathrm{Ti}$ reaction performed using the 5 MV accelerator at the Nuclear Science Laboratory, University of Notre Dame, over a laboratory proton energy range of 526--1275 keV. We present the first direct measurements of the resonance strengths for six resonances at ${E}_{\mathrm{R}}^{\mathrm{lab}}=917.4$, 1026.0, 1031.1, 1049.7, 1059.4, and 1257.5 keV, together with integrated resonance strengths at ${E}^{\mathrm{lab}}=555$, 630, 700, 761, and 871 keV. For resonance energies below the lowest directly measured energy, available transfer-reaction data were used to estimate the resonance strengths. An updated thermonuclear reaction rate is derived, and its astrophysical implications are discussed.- Open Access
- 11 September 2026
- Published by Elsevier in Journal of the European Ceramic Society
- Vol. 47 (2)
Diffusion bonding of alumina-alumina via in-situ Ti5Si3 interlayers formed by self-propagating high-temperature synthesis in spark plasma sintering
- 11 September 2026
- Published by Elsevier in Journal of the European Ceramic Society
- Vol. 47 (2)
Open AccessDiffusion bonding of alumina-alumina via in-situ Ti5Si3 interlayers formed by self-propagating high-temperature synthesis in spark plasma sintering
- Open Access
Fabrication and characterization of self-supporting natural and isotopically pure samarium targets
- Open Access
- 27 April 2026
- Published by Elsevier in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
- Vol. 1090
Combustion-assisted ink-jet printing of nuclear targets
- 27 April 2026
- Published by Elsevier in Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
- Vol. 1090
Open AccessCombustion-assisted ink-jet printing of nuclear targets
- 19 March 2026
- Published by American Physical Society (APS) in Physical Review C
- Vol. 113 (3)
Low-energy measurement of the Mg 25 ( α , n ) Si 28 reaction via neutron spectroscopy
- 19 March 2026
- Published by American Physical Society (APS) in Physical Review C
- Vol. 113 (3)
Low-energy measurement of the Mg 25 ( α , n ) Si 28 reaction via neutron spectroscopy
- 9 February 2026
- Published by American Chemical Society (ACS) in ACS Applied Materials & Interfaces
- Vol. 18 (6) , 9645-9654
Irradiation Driven Restructuring of Nanocrystalline ThO 2 and Th 1– x U x O 2 Thin Films
Irradiation induced structural changes of actinide oxide materials is a key consideration in their development and use as nuclear fuels. This study reported on the synthesis of ThO2 and Th1-xUxO2 (x = 0.15, 0.50) thin films, fabricated using electrospray-assisted solution combustion synthesis, and their responses to ion irradiation. Krypton ion irradiations, up to a fluence of 1 × 1016 ions/cm2, were carried out to simulate radiation damage induced by fission products in a reactor environment. Structural and chemical changes induced by irradiation were analyzed using high-resolution scanning transmission electron microscopy (STEM), energy-dispersive X-ray spectroscopy (EDS), and electron energy-loss spectroscopy (EELS). It was determined that the extent and nature of irradiation-induced damage are strongly correlated with the uranium content. ThO2 films were most susceptible to radiation-induced damage, with significant cavity formation and delamination from the substrate at high fluence. Of the compositions studied, Th0.85U0.15O2 films showed the highest stability, characterized by moderate grain growth and the absence of voids or severe defect structures. In contrast, Th0.5U0.5O2 films accumulated extensive damage, including the formation of a nanocrystalline central region. EELS analysis indicated that oxygen displacement is the primary driver of structural degradation in Th0.5U0.5O2 films. α-particle spectroscopy confirmed minimal actinide loss across all compositions, underscoring the mechanical robustness of the films. These findings provide insight into the irradiation-induced damage mechanisms in ThO2 and Th1-xUxO2 systems, supporting their development as potential materials for nuclear fuels and irradiation-tolerant thin film targets in nuclear physics measurements.
- 9 February 2026
- Published by American Chemical Society (ACS) in ACS Applied Materials & Interfaces
- Vol. 18 (6) , 9645-9654
Irradiation Driven Restructuring of Nanocrystalline ThO 2 and Th 1– x U x O 2 Thin Films
Irradiation induced structural changes of actinide oxide materials is a key consideration in their development and use as nuclear fuels. This study reported on the synthesis of ThO2 and Th1-xUxO2 (x = 0.15, 0.50) thin films, fabricated using electrospray-assisted solution combustion synthesis, and their responses to ion irradiation. Krypton ion irradiations, up to a fluence of 1 × 1016 ions/cm2, were carried out to simulate radiation damage induced by fission products in a reactor environment. Structural and chemical changes induced by irradiation were analyzed using high-resolution scanning transmission electron microscopy (STEM), energy-dispersive X-ray spectroscopy (EDS), and electron energy-loss spectroscopy (EELS). It was determined that the extent and nature of irradiation-induced damage are strongly correlated with the uranium content. ThO2 films were most susceptible to radiation-induced damage, with significant cavity formation and delamination from the substrate at high fluence. Of the compositions studied, Th0.85U0.15O2 films showed the highest stability, characterized by moderate grain growth and the absence of voids or severe defect structures. In contrast, Th0.5U0.5O2 films accumulated extensive damage, including the formation of a nanocrystalline central region. EELS analysis indicated that oxygen displacement is the primary driver of structural degradation in Th0.5U0.5O2 films. α-particle spectroscopy confirmed minimal actinide loss across all compositions, underscoring the mechanical robustness of the films. These findings provide insight into the irradiation-induced damage mechanisms in ThO2 and Th1-xUxO2 systems, supporting their development as potential materials for nuclear fuels and irradiation-tolerant thin film targets in nuclear physics measurements.
- Open Access
- 29 October 2025
- Published by Elsevier in Physics Letters B
- Vol. 871
Alpha-decay width of a near proton-threshold resonance in the 7Li(α, α) channel
- 29 October 2025
- Published by Elsevier in Physics Letters B
- Vol. 871
Open AccessAlpha-decay width of a near proton-threshold resonance in the 7Li(α, α) channel