[PDF] Top 20 La enseñanza de la pronunciación en clase de francés como lengua extranjera
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Dark Matter indirect detection:Some anomalies and many constraints
... four anomalies are: 1) the positron and electron excesses, first soundly detected by Pamela in 2008 in the positron fraction and then corroborated by many results from Fermi, Hess and recently Ams-02; 2) ... See full document
8
Less-simplified models of dark matter for direct detection and the LHC
... . Dark matter SMS based on vector mediators of this kind where studied, ...DD constraints and the results of the next sections will remain ...possible anomalies are canceled by new heavy ... See full document
61
Indirect Dark Matter search with the ANTARES Deep-Sea Cherenkov detector
... the detection of the Cherenkov light induced by the propagation of rela- tivistic muons generated by neutrino interactions in transparent media like ...the detection of up-going muons as a signature of a ... See full document
5
Perspectives on the detection of supersymmetric Dark Matter
... of matter in our Galaxy it is easier to search for antimatter particles from DM ...visible matter and sharply peaking in the ...the indirect DM searches are best performed with satellites outside the ... See full document
10
Atomki anomaly and the Secluded Dark Sector
... direct/indirect dark matter searches. The projected direct detection bounds by the XENON1T and the LZ experiments are shown with the blue dotted ...the dark matter satisfies the ... See full document
5
The XENON project for dark matter direct detection at LNGS
... XENON100 is the first dual-phase TPC operated stably for long-enough period to allow performing a study of annual modulation [13]. The study is performed again on the events belonging to the electronic recoil band in ... See full document
11
Dark Matter Production after Inflation and Constraints
... Furthermore, many other puzzles lack satis- factory explanations within the SCM framework, such as the observed large-scale homogeneity, isotropy and spatial flatness of the ... See full document
89
Astrophysical Constraints on Dark Matter
... of dark matter (DM) into standard model particles, a phenomenon which could be a significant source of photons in the gamma-ray ...an indirect signature of DM ...extended dark matter ... See full document
26
On the Nature of Dark Matter and Dark Energy
... It is worth noting that the experiments for the scanning the celestial sphere by the pulsed plasma generator [22,31] to detect some directions in space, where energy is more than the average value, are the final ... See full document
257
Nature of Dark Matter and Dark Energy
... so many places (including those located on the Earth-on its surface, above and below its surface, in the depths of rivers, lakes, seas and oceans) sometimes touch and even slightly immerse into each ... See full document
228
Dark Energy as a Property of Dark Matter
... A main problem in astrophysics is the discovery, about two decades ago, that our Universe expansion is acceler- ating, instead of slowing down as predicted by the Big Bang theory [1] Scientists hypothesize the existence ... See full document
106
Universe, Dark Energy and Dark Matter
... . (1) It has been found recently that the law (1) is not ful- filled for groups of satellites of our Galaxy, Andromeda nebula and some other galaxies. Every time the velocities of the satellites at distances of ... See full document
46
The Nature of Dark Matter and of Dark Energy
... round matter fields, confining them by the Higgs me- chanism, giving inertial mass to the elementary particles, that is, giving them mechanical ...of matter and the propagation of light and hence is the ... See full document
76
Non-minimal dark matter search in dark matter colliders
... Dark matter (DM) is a key element constituting our universe with energy density about five times larger than that of the Standard Model (SM) ...the dark sector may be also flavorful containing ... See full document
26
Dark Matter and Dark Energy in the Universe
... a matter dominated phase when the field oscillates at the minimum of the ...% matter is responsible for the late phase expansion and 23 % matter called Dark Matter is responsible for a ... See full document
22
Dark Matter Particle Detection System SQUID - Magnetic Calorimeter
... G = × − TeV − is the gravitational constant in the four-dimensional space-time world. A new TeV scale of the interaction unification proposed in certain recent publication includes gravitation [18-21]. Such a ‘premature’ ... See full document
19
Hadronic Dark Matter
... In this consideration, the most of estimations (for instance, the value of new hadron mass and annihilation cross-section) are fulfilled as rough approximations which give an order of value. So, it should be done more ... See full document
21
Search for invisible axion dark matter with the Axion Dark Matter Experiment
... This Letter reports the results from a haloscope search for dark matter axions with masses between 2.66 and 2 . 81 μeV. The search excludes the range of axion-photon couplings predicted by plausible models ... See full document
38
Explanation of Dark Matter, Dark Energy and Dark Space: Discovery of Invisible Universes
... Secondly, many theories developed in physics up to date, in- cluding the theory of relativity and quantum mechanics, are not actually com- pletely accurate and require correction in accordance with the principle ... See full document
81
Calculation of Dark Energy and Dark Matter
... Oscillations are fundamental oscillations of the cosmic space [1, pg.15]. THOMAS GÖRNITZ says: „Structural quanta emerge from a quantum-theoretical description of „oscillation states“ of a system around its ground state. ... See full document
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