Aldo Romani
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Research Interests
Aldo Romani has a total of 1000 co-authors. Here are the top co-authors by number of shared publications:
- Fausto Ortica
Dipartimento di Chimica Biologia e Biotecnologie Università degli Studi e INFN 06123 Perugia Italy
121 shared publications - Albert Sotnikov
Joint Institute for Nuclear Research
98 shared publications - Alexander Derbin
St. Petersburg Nuclear Physics Institute NRC Kurchatov Institute
95 shared publications - Davide Franco
Université de Paris Cité
95 shared publications - Marco Pallavicini
Istituto Nazionale di Fisica Nucleare Sezione di Genova
88 shared publications - Oleg Smirnov
Department of Physics and Electronics Centre for Radio Astronomy Techniques and Technologies (RATT) Rhodes University 6140 Makhanda South Africa
88 shared publications
Latest Publications
- Open Access
- 1 September 2026
- Published by IOP Publishing in Journal of Instrumentation
- Vol. 21 (09) , P09046
Real-Time Wiener Deconvolution for feature reconstruction in JUNO
In particle physics, experiments generate substantial amounts of data that can be difficult to process without preliminary scaling. To avoid losing potentially crucial data, experimental collaborations are studying novel techniques for real-time data processing to extract features for further physics analysis. A common approach, especially in neutrino physics, is to use FPGAs for data acquisition and pre-processing. This paper presents an advanced Real-Time Wiener deconvolution algorithm designed to leverage the processing capabilities of the FPGA integrated into the readout boards of the Jiangmen Underground Neutrino Observatory (JUNO). The goal is to enable real-time reconstruction of the signal generated by photomultiplier tubes (PMTs) when neutrino interactions are detected. By exploiting online reconstruction of the signal generated by PMTs, we expect to improve the detection of low-energy depositions, such as those produced by transient astrophysical phenomena. These depositions are usually not saved because of the significant background that affects the low end of the energy spectrum, which would result in a large trigger rate, hence a large amount of data required for storage. This paper presents the features of the algorithm, including its ability to manage high-throughput data streams with minimal latency, adaptability, and resilience in discerning the characteristics of input data. Performance is evaluated on a JUNO electronic board. This study further demonstrates the potential of FPGA-based solutions for neutrino physics.
- 1 September 2026
- Published by IOP Publishing in Journal of Instrumentation
- Vol. 21 (09) , P09046
Open AccessReal-Time Wiener Deconvolution for feature reconstruction in JUNO
In particle physics, experiments generate substantial amounts of data that can be difficult to process without preliminary scaling. To avoid losing potentially crucial data, experimental collaborations are studying novel techniques for real-time data processing to extract features for further physics analysis. A common approach, especially in neutrino physics, is to use FPGAs for data acquisition and pre-processing. This paper presents an advanced Real-Time Wiener deconvolution algorithm designed to leverage the processing capabilities of the FPGA integrated into the readout boards of the Jiangmen Underground Neutrino Observatory (JUNO). The goal is to enable real-time reconstruction of the signal generated by photomultiplier tubes (PMTs) when neutrino interactions are detected. By exploiting online reconstruction of the signal generated by PMTs, we expect to improve the detection of low-energy depositions, such as those produced by transient astrophysical phenomena. These depositions are usually not saved because of the significant background that affects the low end of the energy spectrum, which would result in a large trigger rate, hence a large amount of data required for storage. This paper presents the features of the algorithm, including its ability to manage high-throughput data streams with minimal latency, adaptability, and resilience in discerning the characteristics of input data. Performance is evaluated on a JUNO electronic board. This study further demonstrates the potential of FPGA-based solutions for neutrino physics.
- Open Access
- 9 May 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (5)
Ultra-trace analysis of U and Th in organic liquid scintillators with high sensitivity
Rare event searches demand extremely low background levels, necessitating ever-advancing screening techniques to enhance sensitivity. Liquid scintillators are highly attractive as detector media due to their inherent radiopurity and scalability in mass. In this work, we present a screening procedure to measure ultra-trace concentrations of natural contaminants – $$^{238}$$ U and $$^{232}$$ Th – with sensitivities at the $${10}^{-15}$$ g/g level. Our method combines neutron activation analysis with radiochemical techniques, followed by $$\beta $$ / $$\gamma $$ coincidence spectroscopy to minimize interference backgrounds. This approach achieves sensitivities of $$0.65 \cdot 10^{-15}$$ g/g for $$^{238}$$ U and $$1.9 \cdot 10^{-15}$$ g/g for $$^{232}$$ Th, among the best reported worldwide. Potential pathways for further sensitivity improvements are outlined in the conclusions.- 9 May 2026
- Published by Springer Nature in The European Physical Journal C
- Vol. 86 (5)
Open AccessUltra-trace analysis of U and Th in organic liquid scintillators with high sensitivity
Rare event searches demand extremely low background levels, necessitating ever-advancing screening techniques to enhance sensitivity. Liquid scintillators are highly attractive as detector media due to their inherent radiopurity and scalability in mass. In this work, we present a screening procedure to measure ultra-trace concentrations of natural contaminants – $$^{238}$$ U and $$^{232}$$ Th – with sensitivities at the $${10}^{-15}$$ g/g level. Our method combines neutron activation analysis with radiochemical techniques, followed by $$\beta $$ / $$\gamma $$ coincidence spectroscopy to minimize interference backgrounds. This approach achieves sensitivities of $$0.65 \cdot 10^{-15}$$ g/g for $$^{238}$$ U and $$1.9 \cdot 10^{-15}$$ g/g for $$^{232}$$ Th, among the best reported worldwide. Potential pathways for further sensitivity improvements are outlined in the conclusions. - Open Access
- 21 November 2025
- Published by American Association for the Advancement of Science (AAAS) in Science Advances
- Vol. 11 (47) , eady1807
Discovering the dual degradation pathway of emerald green in oil paints: The effects of light and humidity
Emerald green, a copper acetoarsenite pigment, enriched the 19th-century and 20th-century artists’ palettes and caused darkening and fragilities in paintings. The accepted alteration mechanism involves the oxidation of triarsenite ions [(As 3 O 6 ) 3− ] to arsenates (AsO 4 3− ), although questions about the promoting factors and the origin of the oxidized arsenic remain unanswered. This study investigates the primary environmental parameters inducing alteration in the oil binder and elucidates the associated degradation pathways through a multiscale analytical approach, including noninvasive spectroscopic techniques and synchrotron radiation–based x-ray methods. By combining results from a historical oil painting by James Ensor (1860 to 1949) and artificially aged paint mock-ups, we identified ultraviolet A–visible light and humidity (relative humidity ≥ 95%) as key driving factors, inducing a dual degradation pathway: Light promotes surface-stratified arsenic oxidation (As 3+ → As 5+ ) resulting in amorphous As 5+ -rich compounds, whereas a dark, high moisture environment favors arsenolite (As 2 O 3 ) crystallization. In addition, a noninvasive analytical strategy is proposed for monitoring the conservation state of emerald green paints in historical artworks.
- 21 November 2025
- Published by American Association for the Advancement of Science (AAAS) in Science Advances
- Vol. 11 (47) , eady1807
Open AccessDiscovering the dual degradation pathway of emerald green in oil paints: The effects of light and humidity
Emerald green, a copper acetoarsenite pigment, enriched the 19th-century and 20th-century artists’ palettes and caused darkening and fragilities in paintings. The accepted alteration mechanism involves the oxidation of triarsenite ions [(As 3 O 6 ) 3− ] to arsenates (AsO 4 3− ), although questions about the promoting factors and the origin of the oxidized arsenic remain unanswered. This study investigates the primary environmental parameters inducing alteration in the oil binder and elucidates the associated degradation pathways through a multiscale analytical approach, including noninvasive spectroscopic techniques and synchrotron radiation–based x-ray methods. By combining results from a historical oil painting by James Ensor (1860 to 1949) and artificially aged paint mock-ups, we identified ultraviolet A–visible light and humidity (relative humidity ≥ 95%) as key driving factors, inducing a dual degradation pathway: Light promotes surface-stratified arsenic oxidation (As 3+ → As 5+ ) resulting in amorphous As 5+ -rich compounds, whereas a dark, high moisture environment favors arsenolite (As 2 O 3 ) crystallization. In addition, a noninvasive analytical strategy is proposed for monitoring the conservation state of emerald green paints in historical artworks.
- Open Access
- 30 September 2025
- Published by Springer Nature in The European Physical Journal C
- Vol. 85 (9) , 1-21
Simulation of the background from $^{13}$C$(\alpha ,\,n)^{16}$O reaction in the JUNO scintillatorLarge-scale organic liquid scintillator detectors are highly efficient in the detection of MeV-scale electron antineutrinos. These signal events can be detected through inverse beta decay on protons, which produce a positron accompanied by a neutron. A noteworthy background for antineutrinos coming from nuclear power reactors and from the depths of the Earth (geoneutrinos) is generated by ( $$\alpha ,\,n$$ ) reactions. In organic liquid scintillator detectors, $$\alpha $$ particles emitted from intrinsic contaminants such as $$^{238}$$ U, $$^{232}$$ Th, and $$^{210}$$ Pb/ $$^{210}$$ Po, can be captured on $$^{13}$$ C nuclei, followed by the emission of a MeV-scale neutron. Three distinct interaction mechanisms can produce prompt energy depositions preceding the delayed neutron capture, leading to a pair of events correlated in space and time within the detector. Thus, ( $$\alpha ,\,n$$ ) reactions represent an indistinguishable background in liquid scintillator-based antineutrino detectors, where their expected rate and energy spectrum are typically evaluated via Monte Carlo simulations. This work presents results from the open-source SaG4n software, used to calculate the expected energy depositions from the neutron and any associated de-excitation products. Also simulated is a detailed detector response to these interactions, using a dedicated Geant4-based simulation software from the JUNO experiment. An expected measurable $$^{13}$$ C $$(\alpha ,\,n)^{16}$$ O event rate and reconstructed prompt energy spectrum with associated uncertainties, are presented in the context of JUNO, however, the methods and results are applicable and relevant to other organic liquid scintillator neutrino detectors.- 30 September 2025
- Published by Springer Nature in The European Physical Journal C
- Vol. 85 (9) , 1-21
Open AccessSimulation of the background from $^{13}$C$(\alpha ,\,n)^{16}$O reaction in the JUNO scintillatorLarge-scale organic liquid scintillator detectors are highly efficient in the detection of MeV-scale electron antineutrinos. These signal events can be detected through inverse beta decay on protons, which produce a positron accompanied by a neutron. A noteworthy background for antineutrinos coming from nuclear power reactors and from the depths of the Earth (geoneutrinos) is generated by ( $$\alpha ,\,n$$ ) reactions. In organic liquid scintillator detectors, $$\alpha $$ particles emitted from intrinsic contaminants such as $$^{238}$$ U, $$^{232}$$ Th, and $$^{210}$$ Pb/ $$^{210}$$ Po, can be captured on $$^{13}$$ C nuclei, followed by the emission of a MeV-scale neutron. Three distinct interaction mechanisms can produce prompt energy depositions preceding the delayed neutron capture, leading to a pair of events correlated in space and time within the detector. Thus, ( $$\alpha ,\,n$$ ) reactions represent an indistinguishable background in liquid scintillator-based antineutrino detectors, where their expected rate and energy spectrum are typically evaluated via Monte Carlo simulations. This work presents results from the open-source SaG4n software, used to calculate the expected energy depositions from the neutron and any associated de-excitation products. Also simulated is a detailed detector response to these interactions, using a dedicated Geant4-based simulation software from the JUNO experiment. An expected measurable $$^{13}$$ C $$(\alpha ,\,n)^{16}$$ O event rate and reconstructed prompt energy spectrum with associated uncertainties, are presented in the context of JUNO, however, the methods and results are applicable and relevant to other organic liquid scintillator neutrino detectors. - Open Access
- 9 July 2025
- Published by IOP Publishing in Journal of Physics: Photonics
- Vol. 7 (3) , 035020
Light source classification and colour change modelling for understanding and predicting pigments discolouration
In this study, we introduce a simple but effective model, combined with a classification system for light sources based on their spectral profile approximated by the relative power distribution in the red, green and blue regions, which successfully fits experimental data of pigment colour changes in an oil binder under various lighting conditions. This model is experimentally validated by artificial ageing tests on two sets of model samples made of historical pigments (strontium yellow and Prussian blue mixed with lead white) using three white light sources (two WLEDs and a xenon light source). The model accurately fits colour shifts by analysing changes in International Commission on Illumination L*a*b* values. The results highlight that integrating the spectral classification of the light sources with the colour change model provides deeper insights into the causes of paint colour changes than traditional methods that rely solely on total irradiance. This combined approach enables precise prediction of long-term colour changes by exploiting the spectral characteristics of light sources.
- 9 July 2025
- Published by IOP Publishing in Journal of Physics: Photonics
- Vol. 7 (3) , 035020
Open AccessLight source classification and colour change modelling for understanding and predicting pigments discolouration
In this study, we introduce a simple but effective model, combined with a classification system for light sources based on their spectral profile approximated by the relative power distribution in the red, green and blue regions, which successfully fits experimental data of pigment colour changes in an oil binder under various lighting conditions. This model is experimentally validated by artificial ageing tests on two sets of model samples made of historical pigments (strontium yellow and Prussian blue mixed with lead white) using three white light sources (two WLEDs and a xenon light source). The model accurately fits colour shifts by analysing changes in International Commission on Illumination L*a*b* values. The results highlight that integrating the spectral classification of the light sources with the colour change model provides deeper insights into the causes of paint colour changes than traditional methods that rely solely on total irradiance. This combined approach enables precise prediction of long-term colour changes by exploiting the spectral characteristics of light sources.
- 19 March 2025
- Published by Springer Nature
- p. 195-214
Fluorescence of Binders and Varnishes Used in Paintings
- 19 March 2025
- Published by Springer Nature
- p. 195-214
Fluorescence of Binders and Varnishes Used in Paintings
- 13 November 2024
- Published by Springer Nature
- p. 353-364
Fluorescence of Pigments in Late Nineteenth- to Twentieth-Century Paintings by Edvard Munch and Gerardo Dottori
- 13 November 2024
- Published by Springer Nature
- p. 353-364
Fluorescence of Pigments in Late Nineteenth- to Twentieth-Century Paintings by Edvard Munch and Gerardo Dottori