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Welcome / Lopienski, Sebastian (speaker) (CERN) ; Ferreira, Pedro (speaker) (CERN) ; Gonzalez Labrador, Hugo (speaker) (CERN) ; Ragozina, Elizaveta (speaker) (Massachusetts Inst. of Technology (US))
2025 - 213. IT Lightning Talks (ITLT); IT Lightning Talks: session #26 External links: Talk details; Event details In : IT Lightning Talks: session #26

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Closing remarks / Mönnich, Adrian (speaker) (CERN) ; Ferreira, Pedro (speaker) (CERN)
2025 - 1373. Indico; Indico Workshop 2025 External links: Talk details; Event details In : Indico Workshop 2025

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Workshop kick-off / Ferreira, Pedro (speaker) (CERN)
2025 - 501. Indico; Indico Workshop 2025 External links: Talk details; Event details In : Indico Workshop 2025

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Radiative neutron capture cross section of $^{242}$Pu measured at n_TOF-EAR1 in the unresolved resonance region up to 600 keV / n_TOF Collaboration
The design of fast reactors burning MOX fuels requires accurate capture and fission cross sections. [...]
arXiv:2412.01332. - 20.
Fulltext

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The Stellar $^{72}$Ge(n, γ) Cross Section for weak s-process: A First Measurement at n_TOF / Dietz, M (Edinburgh U. ; Braunschweig, Phys. Tech. Bund.) ; Lederer-Woods, C (Edinburgh U.) ; Tattersall, A (Edinburgh U.) ; Battino, U (Edinburgh U.) ; Gunsing, F (IRFU, Saclay ; CERN) ; Heinitz, S (PSI, Villigen) ; Lerendegui-Marco, J (Seville U.) ; Krtička, M (Charles U. ; Seville U.) ; Reifarth, R (Frankfurt U.) ; Valenta, S (Charles U.) et al.
The slow neutron capture process (s-process) is responsible for producing about half of the elemental abundances heavier than iron in the universe. Neutron capture cross sections on stable isotopes are a key nuclear physics input for s-process studies. [...]
2023 - 4 p. - Published in : EPJ Web Conf. 284 (2023) 01017 Fulltext: PDF;
In : 15th International Conference on Nuclear Data for Science and Technology, Online, 21 - 29 Jul 2022, pp.01017

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Shedding Light on the Origin of Pb204, the Heaviest s-Process–Only Isotope in the Solar System / n_TOF Collaboration
Asymptotic giant branch stars are responsible for the production of most of the heavy isotopes beyond Sr observed in the solar system. Among them, isotopes shielded from the r-process contribution by their stable isobars are defined as s-only nuclei. [...]
2024 - 8 p. - Published in : Phys. Rev. Lett. 133 (2024) 052702 Fulltext: PDF;

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Top quark at the new physics frontier / Yazgan, Efe ; Ferreira da Silva, Pedro (ed.)
Basel : MDPI, 2024. - 257 p.

10.3390/books978-3-7258-0614-0

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HHH Whitepaper / Abouabid, Hamza (Abdelmalek Essaadi U.) ; Arhrib, Abdesslam (Abdelmalek Essaadi U.) ; Arnold, Hannah (Stony Brook U.) ; Azevedo, Duarte (KIT, Karlsruhe, TP) ; Brigljevic, Vuko (Boskovic Inst., Zagreb) ; Chen, Maggie (Oxford U., Theor. Phys.) ; Diaz, Daniel (San Diego State U.) ; Duarte, Javier (San Diego State U.) ; du Pree, Tristan (NIKHEF, Amsterdam ; Twente U., Enschede) ; Falaki, Jaouad El (Ibn Zohr U., Agadir) et al.
We here report on the progress of the HHH Workshop, that took place in Dubrovnik in July 2023. After the discovery of a particle that complies with the properties of the Higgs boson of the Standard Model, all Standard Model (SM) parameters are in principle determined [...]
arXiv:2407.03015.- 2024-11-19 - 117 p. - Published in : 10.1140/epjc/s10052-024-13376-3 Fulltext: 2407.03015 - PDF; document - PDF;

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Euclid. I. Overview of the Euclid mission / Euclid Collaboration
The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Euclid is a medium-class mission in the Cosmic Vision 2015-2025 programme of the European Space Agency (ESA) that will provide high-resolution optical imaging, as well as near-infrared imaging and spectroscopy, over about 14,000 deg^2 of extragalactic sky. [...]
arXiv:2405.13491.- 2025-04 - 94 p. - Published in : Astron. Astrophys. 697 (2025) A1 Fulltext: 2405.13491 - PDF; publication - PDF;

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10.

Measurement of the prompt fission $\gamma $-rays from slow neutron-induced fission of $^{235}$U with STEFF / n_TOF Collaboration
The average energy and multiplicity of prompt $\gamma $-rays from slow neutron-induced fission of $^{235}$U have been measured using the STEFF spectrometer at the neutron time-of-flight facility n_TOF. The individual responses from 11 NaI scintillators were corrected for multiple $\gamma $-ray interactions, prompt fission neutrons and background counts before being deconvolved to estimate the emitted spectrum of prompt fission $\gamma $-rays. [...]
2024 - 11 p. - Published in : Eur. Phys. J. A 60 (2024) 70 Fulltext: PDF;

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Se också: liknande författarnamn
108	FERREIRA, Pedro
76	Ferreira, P
1	Ferreira, P A L
1	Ferreira, P B
1	Ferreira, P C
12	Ferreira, P Castelo
63	Ferreira, P G
2	Ferreira, P J S G
4	Ferreira, P L
65	Ferreira, P M
2	Ferreira, P M M
12	Ferreira, P.G.
1	Ferreira, P.M.
3	Ferreira, Paulo
1	Ferreira, Paulo J S G
108	Ferreira, Pedro
3	Ferreira, Pedro C
68	Ferreira, Pedro G
5	Ferreira, Pedro G.
1	Ferreira, Pedro M
1	Ferreira, Pedro M.
1	Ferreira, Pedro. M.
1	Ferreira, Prof. Pedro G.
1	Ferreira, Professor Pedro
1	Ferreira, Professor Pedro G.

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