|
Author |
Title |
Year |
Publication |
Volume |
Pages |
Links |
|
Amerio, A.; Cuoco, A.; Fornengo, N. |
Extracting the gamma-ray source-count distribution below the Fermi-LAT detection limit with deep learning |
2023 |
Journal of Cosmology and Astroparticle Physics |
09 |
029 - 39pp |
|
|
Sierra, D.A.; De Romeri, V.; Flores, L.J.; Papoulias, D.K. |
Impact of COHERENT measurements, cross section uncertainties and new interactions on the neutrino floor |
2022 |
Journal of Cosmology and Astroparticle Physics |
01 |
055 - 26pp |
|
|
Molina, R.; Oset, E. |
Molecular picture for the X-0(2866) as a D*(K)over-bar* J(P)=0(+) state and related 1(+), 2(+) states |
2020 |
Physics Letters B |
811 |
135870 - 7pp |
|
|
Abreu, L.M.; Dai, L.R.; Oset, E. |
J/Psi decay to omega, phi, K*0 plus f0(1370), f0(1710), K0*(1430), f2(1270), f'2 (1525) and K2*(1430): Role of the D-wave for tensor production |
2023 |
Physics Letters B |
843 |
137999 - 10pp |
|
|
Bazzocchi, F.; Cerdeño, D.G.; Muñoz, C.; Valle, J.W.F. |
Calculable inverse-seesaw neutrino masses in supersymmetry |
2010 |
Physical Review D |
81 |
051701 - 5pp |
|
|
Husek, T.; Goudzovski, E.; Icampf, K. |
Precise Determination of the Branching Ratio of the Neutral-Pion Dalitz Decay |
2019 |
Physical Review Letters |
122 |
022003 - 6pp |
|
|
Bonilla, C.; Centelles Chulia, S.; Cepedello, R.; Peinado, E.; Srivastava, R. |
Dark matter stability and Dirac neutrinos using only standard model symmetries |
2020 |
Physical Review D |
101 |
033011 - 5pp |
|
|
Centelles Chulia, S.; Herrero-Brocal, A.; Vicente, A. |
The Type-I Seesaw family |
2024 |
Journal of High Energy Physics |
07 |
060 - 35pp |
|
|
Centelles Chulia, S.; Cepedello, R.; Peinado, E.; Srivastava, R. |
Systematic classification of two-loop d=4 Dirac neutrino mass models and the Diracness-dark matter stability connection |
2019 |
Journal of High Energy Physics |
10 |
093 - 33pp |
|
|
Motohashi, H.; Hu, W. |
Generalized slow roll in the unified effective field theory of inflation |
2017 |
Physical Review D |
96 |
023502 - 17pp |
|