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Title Observation of collective photoswitching in free-standing TATA-based azobenzenes on Au(111) Author info Talina R. Rusch, Alexander Schlimm ... [et al.] Author Rusch Talina R. (11%)
Co-authors Schlimm Alexander (11%)
Krekiehn Nicolai R. (11%)
Tellkamp Tobias (11%)
Budzák Šimon 1982- (11%) UMBFP08 - Katedra chémie
Jacquemin Denis (11%)
Tuczek Felix (11%)
Herges Rainer (11%)
Magnussen Olaf M. (12%)
Source document Angewandte Chemie : international edition. Vol. 59, no. 39 (2020), pp. 17192-17196. - Weinheim : John Wiley & Sons, 2020 Keywords pozorovanie - observation mikroskopia - microscopy excitations Form. Descr. články - journal articles Language English Country Germany URL Link na plný text Public work category ADC No. of Archival Copy 48518 Catal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Database xpca - PUBLIKAČNÁ ČINNOSŤ References PERIODIKÁ-Súborný záznam periodika 
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Title Contribution of the massive photon decay channel to neutrino cooling of neutron stars Author info D. N. Voskresensky, Evgeni E. Kolomeitsev, B. Kämpfer Author Voskresensky Dmitri (34%)
Co-authors Kolomeitsev Evgeni E. 1970- (33%)
Kämpfer B. (33%)
Source document Journal of experimental and theoretical physics. Vol. 87, no. 2 (1998), pp. 211-217. - Woofbury : American Institute of Physics, 1998 Keywords luminosity matter excitations Language English Country United States of America systematics 539.1 Annotation We consider massive photon decay reactions via intermediate states of electron-electron-holes and proton-proton-holes into neutrino-antineutrino pairs in the course of neutron star cooling. These reactions may become operative in hot neutron stars in the region of proton pairing where the photon due to the Higgs-Meissner effect acquires an effective mass m(gamma) that is small compared to the corresponding plasma frequency. The contribution of these reactions to neutrino emissivity is calculated; it varies with the temperature and the photon mass as T(3/2)m(gamma)(7/2) exp(-m(gamma)/T) for T < m(gamma). Estimates show that these processes appear as extra efficient cooling channels of neutron stars at temperatures T =10(9)-10(10) K. (C) 1998 American Institute of Physics. Public work category ADC No. of Archival Copy 26369 Catal.org. BB301 - Univerzitná knižnica Univerzity Mateja Bela v Banskej Bystrici Database xpca - PUBLIKAČNÁ ČINNOSŤ unrecognised