Lorenzo Ubaldi, Ph.D.
Affiliations: | 2011 | University of California, Santa Cruz, Santa Cruz, CA, United States |
Area:
Elementary Particles and High Energy Physics, Astronomy and AstrophysicsGoogle:
"Lorenzo Ubaldi"Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Stefano Profumo | grad student | UC Santa Cruz | ||
| Michael Dine | grad student | 2011 | UC Santa Cruz | |
| (Lights in the dark.) | ||||
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Publications
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| Colucci S, Ubaldi L, Dreiner HK. (2019) The Supersymmetric R-Parity Violating Dine-Fischler-Srednicki-Zhitnitsky Axion Model Physical Review D. 99 |
| Bastero-Gil M, Santiago J, Ubaldi L, et al. (2019) Vector dark matter production at the end of inflation Journal of Cosmology and Astroparticle Physics. 2019: 15-15 |
| Azatov A, Barducci D, Ghosh D, et al. (2018) Combined explanations of B-physics anomalies: the sterile neutrino solution Journal of High Energy Physics. 2018: 92 |
| Tangarife W, Tobioka K, Ubaldi L, et al. (2018) Dynamics of relaxed inflation Journal of High Energy Physics. 2018 |
| Staub F, Athron P, Basso L, et al. (2016) Precision tools and models to narrow in on the 750 GeV diphoton resonance European Physical Journal C. 76: 516 |
| Gupta RS, Komargodski Z, Perez G, et al. (2016) Is the relaxion an axion? Journal of High Energy Physics. 2016: 1-14 |
| Festuccia G, Opferkuch T, Ubaldi L. (2015) Dynamical Generation of the Peccei-Quinn Scale in Gauge Mediation Physical Review D. 92: 15020 |
| Colucci S, Dreiner HK, Staub F, et al. (2015) Heavy concerns about the light axino explanation of the 3.5 keV X-ray line Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 750: 107-111 |
| Feng L, Profumo S, Ubaldi L. (2015) Closing in on singlet scalar dark matter: LUX, invisible Higgs decays and gamma-ray lines Journal of High Energy Physics. 2015: 1-13 |
| Dreiner HK, Staub F, Ubaldi L. (2014) From the unification scale to the weak scale: A self consistent supersymmetric Dine-Fischler-Srednicki-Zhitnitsky axion model Physical Review D. 90: 55016 |