Author |
Title |
Year |
Publication |
Volume |
Pages |
Calefice, L.; Hennequin, A.; Henry, L.; Jashal, B.K.; Mendoza, D.; Oyanguren, A.; Sanderswood, I.; Sierra, C.V.; Zhuo, J.H. |
Effect of the high-level trigger for detecting long-lived particles at LHCb |
2022 |
Frontiers in Big Data |
5 |
1008737 - 13pp |
Alonso, I. et al; Bernabeu, J. |
Cold atoms in space: community workshop summary and proposed road-map |
2022 |
EPJ Quantum Technology |
9 |
30 - 55pp |
Dai, L.R.; Molina, R.; Oset, E. |
The (B)over-bar(0)-> D*+ (D)over-bar*K-0(-) reaction to detect the I=0, J(P)=1+ partner of the X-0(2866) |
2022 |
Physics Letters B |
832 |
137219 - 5pp |
Aguilar, A.C.; Ferreira, M.N.; Oliveira, B.M.; Papavassiliou, J. |
Schwinger-Dyson truncations in the all-soft limit: a case study |
2022 |
European Physical Journal C |
82 |
1068 - 15pp |
Ji, T.; Dong, X.K.; Albaladejo, M.; Du, M.L.; Guo, F.K.; Nieves, J. |
Establishing the heavy quark spin and light flavor molecular multiplets of the X(3872), Z(c)(3900), and X(3960) br |
2022 |
Physical Review D |
106 |
094002 - 13pp |
Ramalho, M.; Suhonen, J.; Kostensalo, J.; Alcala, G.A.; Algora, A.; Fallot, M.; Porta, A.; Zakari-Issoufou, A.A. |
Analysis of the total beta-electron spectrum of( 92)Rb: Implications for the reactor flux anomalies |
2022 |
Physical Review C |
106 |
024315 - 7pp |
Ikeno, N.; Liang, W.H.; Toledo, G.; Oset, E. |
Interpretation of the Omega(c) -> pi(+) Omega(2012) -> pi(+) ((K)over-bar Xi) relative to Omega(c) -> pi(+) (K)over-bar Xi from the Omega (2012) molecular perspective |
2022 |
Physical Review D |
106 |
034022 - 10pp |
Bernabeu, J.; Di Domenico, A. |
Can future observation of the living partner post-tag the past decayed state in entangled neutral K mesons? |
2022 |
Physical Review D |
105 |
116004 - 8pp |
Navarro-Salas, J.; Pla, S. |
Particle Creation and the Schwinger Model |
2022 |
Symmetry-Basel |
14 |
2435 - 9pp |
Ackermann, M. et al; Garcia Soto, A. |
High-energy and ultra-high-energy neutrinos: A Snowmass white paper |
2022 |
Journal of High Energy Astrophysics |
36 |
55-110 |