Results 111 to 120 of about 150,777 (255)
Luminosity Studies for the Cool Copper Collider [PDF]
Achieving high instantaneous luminosity while managing the beaminduced background (BIB) is critical for the successful operation of any future electron-positron (e+e−) collider.
Ntounis Dimitris +2 more
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Desenvolvimento de Mudas de Nim Indiano sob Diferentes Níveis de Sombreamento
Este estudo teve como objetivo avaliar o efeito de níveis de sombreamento na produção de mudas de nim indiano (Azadirachta indica), visando a obtenção de mudas com maior padrão de qualidade. Foram adotados quatro tratamentos (pleno sol, 30%, 50% e 70% de
Glauce Taís de Oliveira Sousa Azevedo +3 more
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REMARKS ON H. D. CURTIS' PAPER ON STELLAR LUMINOSITIES [PDF]
W. J. Luyten
openalex +1 more source
On the Masses, Luminosities, and Surface-Temperatures of the Stars.: (Final Note.) [PDF]
James Jeans
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O objetivo deste estudo foi avaliar a adição de concentrações de carvão ativado em meio de cultura ½ MS (com metade da concentração dos macronutrientes) sob dois espectros luminosos para a obtenção de plântulas in vitro de Cattleya loddigesii.
Renato Fernandes Galdiano Júnior +3 more
doaj
Optimizing integrated luminosity of future hadron colliders
The integrated luminosity, a key figure of merit for any particle-physics collider, is closely linked to the peak luminosity and to the beam lifetime. The instantaneous peak luminosity of a collider is constrained by a number of boundary conditions, such
Michael Benedikt +2 more
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Luminosities of AGB Variables [PDF]
8 pages, 2 figure, to be published in Mass-Losing Pulsating Stars and their Circumstellar Matter, Y. Nakada & M.
openaire +3 more sources
The Moeller luminosity factor [PDF]
LBNL-53553, CBP Note-543 The Moller Luminosity Factor ∗ M. A. Furman † Center for Beam Physics Lawrence Berkeley National Laboratory, Bldg. 71R0259 1 Cyclotron Rd. Berkeley, CA 94720-8211 (Dated: September 24, 2003) Consider two bunches of particles with densities ρ 1 (x, t) and ρ 2 (x, t) normalized such that d 3 x ρ i (x, t) = N i , i = 1, 2 where N ...
openaire +4 more sources

