Sample records for INTERACCIONES ELECTROMAGNETICAS (electromagnetic interactions)
from WorldWideScience.org

Sample records 1 - 20 shown. Select sample records:



1

phi K+K- production in electron-positron annihilation

Gómez-Avila, S.; Napsuciale, Mauro; Oset, Eulogi
2009-02-18

Digital.CSIC (Spain)

2

Understanding open-charm mesons

Vijande, Javier; Fernández, F.; Valcarce, A.
2007-01-30

Digital.CSIC (Spain)

3

Three-body correlations in electromagnetic dissociation of Borromean nuclei: The He-6 case

Chulkov, L. V.; Simon, H.; Thompson, I. J.; Aumann, T.; García Borge, María José; Elze, Th. W.; Emling, H.; Geissel, H.; Grigorenko, L. V.; Hellström, M.; Jonson, B.; Kratz, J. W. V.; Kulessa, R.; Markenroth, K.; Meister, M.; Münzenberg, G.; Nickel, F.; Nilsson, T.; Nyman, G.; Pribora, V.; Richter, A.; Riisager, K.; Scheidenberger, C.; Schrieder, G.; Tengblad, Olof; Zhukov, M. V.
2005-06-13

Digital.CSIC (Spain)

4

The radiative decay of the Λ(1405) and its two-pole structure

Geng, Lisheng; Oset, Eulogi; Döring, Michael

11 pages, 9 figures.-- PACS nrs.: 13.40.Hq, 14.20.Jn, 13.75.-n, 25.20.Lj.-- ISI Article Identifier: 000247348200009.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ph/0702093 | We evaluate theoretically the radiative decay widths into γΛ and γΣ(0) of the two poles of the Λ(1405) found in c...

DRIVER (Spanish)

5

The radiative decay of the Λ(1405) and its two-pole structure

Geng, Li Sheng; Oset, Eulogi; Döring, Michael
2007-05-18

Digital.CSIC (Spain)

6

The Halo of 14Be

Labiche, M.; Orr, N. A.; Marqués, F. M.; Angélique, J. C.; Axelsson, L.; Benoit, B.; Bergmann, U. C.; García Borge, María José; Catford, W. N.; Chappell, S. P. G.; Clarke, N. M.; Costa, G.; Curtis, N.; D’Arrigo, A.; de Góes Brennand, E.; Dorvaux, O.; Fazio, G.; Freer, M.; Fulton, B. R.; Giardina, G.; Grévy, S.; Guillemaud-Mueller, D.; Hanappe, F.; Heusch, B.; Jones, K.L.; Jonson, B.; Le Brun, C.; Leenhardt, S.; Lewitowicz, M.; López, M. J.; Markenroth, K.; Mueller, A. C.; Nilsson, T.; Ninane, A.; Nyman, G.; de Oliveira, F.; Piqueras, I.; Riisager, K.; Saint-Laurent, M. G.; Sarazin, F.; Singer, S. M.; Sorlin, O.; Stuttgé, L.
2000-06-07

Digital.CSIC (Spain)

7

Substrate-enhanced infrared near-field spectroscopy

Aizpurúa, Javier; Taubner, Thomas; García de Abajo, F. Javier; Brehm, Markus; Hillenbrand, Rainer
2008-01-22

Digital.CSIC (Spain)

8

Search for the exotic Θ(+) resonance in the NOMAD experiment

Samoylov, O.; Naumov, D.; Cavasinni, V.; Astier, P.; Autiero, D.; Baldisseri, A.; Baldo-Ceolin, M.; Banner, M.

12 pages, 16 figures.-- PACS nrs.: 13.15.+g; 13.60.Le; 13.87.Fh; 14.40.Ev.-- ISI Article Identifier: 000243973100007.-- ArXiv pre-print available at: http://arxiv.org/abs/hep-ex/0612063 | Printed version published in Jan 2007. | A search for exotic Θ(+) baryon via Θ(+) -> p + K-S(0) decay mode in th...

DRIVER (Spanish)

9

Search for the exotic Θ(+) resonance in the NOMAD experiment

Cervera Villanueva, Anselmo; Gómez Cadenas, Juan José; Hernando, J.
2006-10-24

Digital.CSIC (Spain)

11

Quantum properties of tranverse pattern formation in second-harmonic generation

Bache, Morten; Scotto, Pierre; Zambrini, Roberta; San Miguel, Maxi; Saffman, Mark
2002-07-19

Digital.CSIC (Spain)

12

Polarization quantum properties in a type-II Optical Parametric Oscillator below threshold

Zambrini, Roberta; Gatti, Alessandra; Lugiato, Luigi A.; San Miguel, Maxi
2003-12-10

Digital.CSIC (Spain)

13

Performance of the prototype detector for the LHCf experiment

Sako, T.; Adriani, O.; Bonechi, L.; Bongi, M.; Faus, Ángeles; Haguenauer, M.; Itow, Y.; Kasahara, K.; Masuda, K.; Matsubara, Y.; Matsumoto, H.; Menjo, H.; Muraki, Y.; Obata, Y.; Tamura, T.; Tanaka, K.; Torii, S.; Turner, W. C.; Velasco, Jorge; Yoshida, K.
2007-07-21

Digital.CSIC (Spain)

14

Neutrino flux prediction at MiniBooNE

Sorel, Michel; Aguilar-Arevalo, A. A.; Anderson, C. E.; Bazarko, A. O.; Brice, S. J.; Brown, B. C.; Bugel, L.; Cao, J.; Coney, L.; Conrad, J. M.; Cox, D. C.; Curioni, A.; Djurcic, Z.; Finley, D. A.; Fleming, B. T.; Ford, R.; Garcia, F. G.; Garvey, G. T.; Green, C.; Green, J. A.; Hart, T. L.; Hawker, E.; Imlay, R.; Johnson, R. A.; Karagiorgi, G.; Kasper, P.; Katori, T.; Kobilarcik, T.; Kourbanis, I.; Koutsoliotas, S.; Laird, E. M.; Linden, S. K.; Link, J. M.; Liu, Y.; Louis, W. C.; Mahn, K. B. M.; Marsh, W.; Martin, P. S.; McGregor, G.; Metcalf, W.; Meyers, P. D.; Mills, F.; Mills, G. B.; Monroe, J.; Moore, C. D.; Nelson, R. H.; Nguyen, V. T.; Nienaber, P.; Nowak, J. A.; Ouedraogo, S.; Patterson, R. B.; Perevalov, D.; Polly, C. C.; Prebys, E.; Raaf, J. L.; Ray, H.; Roe, B. P.; Russell, A. D.; Sandberg, V.; Schirato, R.; Schmitz, D.; Shaevitz, M. H.; Shoemaker, F. C.; Smith, D.; Soderberg, M.; Spentzouris, P.; Stancu, I.; Stefanski, R. J.; Sung, M.; Tanaka, H. A.; Tayloe, R.; Tzanov, M.; Van de Water, R.; Wascko, M. O.; White, D. H.; Wilking, M. J.; Yang, H. J.; Zeller, G. P.; Zimmerman, E. D.; MiniBooNE Collaboration
2009-04-15

Digital.CSIC (Spain)

18

Interacciones de las radiaciones electromagnéticas y especies reactivas del oxígeno sobre la piel/ Interactions of electromagnetic radiations and reactive oxygen species on skin

Ferramola de Sancovich, A M; Sancovich, H A
2006-06-01

Resumen en español La energía radiante abarca todo el espectro electromagnético y proviene de la fusión en el sol, de 4 núcleos de hidrógeno en uno de helio. Las radiaciones electromagnéticas tienen características de ondas, con la velocidad de la luz (c) y difieren en sus longitudes de ondas (λ). La energía lumínica es transmitida en unidades individuales o fotones: E = h c/λ así, los fotones de menores λs son los de mayor energía. Las radiaciones ultravioletas (U (mas) V) (λs de 200 - 400 nm) pueden dividirse: UVA (λs 315 - 400 nm); UVB (λs 280 - 315 nm) y UVC (λs Resumen en inglés The energy of electromagnetic radiation is derived from the fusion in the sun of four hydrogen nuclei to form a helium nucleus. The sun radiates energy representing the entire electromagnetic spectrum. Light is a form of electromagnetic radiation. All electromagnetic radiation has wave characteristics and travels at the same speed (c: speed of light). But radiations differ in wavelength (λ). Light energy is transmitted not in a continuum stream but only in individual (mas) units or photons: E = h c/λ. Short wave light is more energetic than photons of light of longer wavelength. Ultraviolet radiations (UV) (λs 200 - 400 nm) can be classified in UVA (λs 315 - 400 nm.); UVB (λs 280 - 315 nm) and UVC (λs

Scientific Electronic Library Online (Spanish)

19

Identification of photon-tagged jets in the ALICE experiment

Conesa, Gustavo; Delagrange, H.; Díaz Medina, José; Kharlov, Y. V.; Schutz, Y.
2007-11-15

Digital.CSIC (Spain)

20

Global restrictions to the Mixing Angle W

Calixto Molina, Manuel; Aldaya Valverde, Víctor; Guerrero García, Julio

In spite of its firm hold in particle physics, the gauge group SU(2)⊗U(1)Y proves not to be the most appropriate to describe the unification of weak and electromagneticinteractions. In fact, a look at the structure of SU(2)⊗U(1)Y tells us that both, the electric charge generator Q and its correspon...

DRIVER (Spanish)

23

Entanglement swapping between spacelike-separated atoms

León García, Juan José; Sabín, Carlos
2008-11-10

Digital.CSIC (Spain)

24

Electromagnetism in nonleptonic weak interactions

Ecker, Gerhard; Isidori, Gino; Müller, G.; Neufeld, Helmut; Pich, Antonio
2000-12-18

Digital.CSIC (Spain)

25
26

Electromagnetic decays of heavy baryons

Bañuls, M. C.; Pich, Antonio; Scimemi, Ignazio
2000-01-01

Digital.CSIC (Spain)

27
29

Angular momentum of multimode and polarization patterns

Zambrini, Roberta; Barnett, Stephen M.
2007-09-11

Digital.CSIC (Spain)