Search for giant planets in M67 - III. Excess of hot Jupiters in dense
... has a well-established solar metallicity and abundance pattern (Randich et al. 2005). The hypothesis that the high frequency of HJs in M67 or in OCs in general originates from the higher mass of the host star can be also excluded: the stars hosting HJs in M67 all have masses around one solar mass, w ...
... has a well-established solar metallicity and abundance pattern (Randich et al. 2005). The hypothesis that the high frequency of HJs in M67 or in OCs in general originates from the higher mass of the host star can be also excluded: the stars hosting HJs in M67 all have masses around one solar mass, w ...
Breaks in gamma-ray spectra of distant blazars and transparency of
... of VHE photon production along the path from the source to the observer feeds the photon flux which is, in parallel, absorbed in the usual way. These additional photons may be created in interactions of ultra-high-energy cosmic protons, which are assumed, in this model, to be produced in the very sa ...
... of VHE photon production along the path from the source to the observer feeds the photon flux which is, in parallel, absorbed in the usual way. These additional photons may be created in interactions of ultra-high-energy cosmic protons, which are assumed, in this model, to be produced in the very sa ...
Light on Dark Matter with Weak Gravitational Lensing
... Taylor series approximation of the distortion operator, given by the lens equation, can be done : ...
... Taylor series approximation of the distortion operator, given by the lens equation, can be done : ...
View/Open - NuSpace Home - National University of Science and
... theories can be ruled out unless sufficient observations are available to act up as the arbiter thus pressure is put on the need for more refined observations. Should these observations became available, there is hope that only the correct theory will stand the test as the fine tuning of these theor ...
... theories can be ruled out unless sufficient observations are available to act up as the arbiter thus pressure is put on the need for more refined observations. Should these observations became available, there is hope that only the correct theory will stand the test as the fine tuning of these theor ...
Ion dynamics in electron beam–plasma interaction: particle-in
... 1985). In this resonant three-wave interaction the frequency of the ion acoustic mode is very small against the plasma frequency which makes it very difficult to resolve separated peaks in the plasma frame. However, the resonance conditions require a significant difference in the wave numbers of the ...
... 1985). In this resonant three-wave interaction the frequency of the ion acoustic mode is very small against the plasma frequency which makes it very difficult to resolve separated peaks in the plasma frame. However, the resonance conditions require a significant difference in the wave numbers of the ...
08 Waves Chapters 8_-_waves_combined
... tells a friend out in the hall, “Mr. Gunderson just bought a sports car, I think he got a Ferrari.” The Physics Kahuna supposes that this is possible. Anyway, two hours later one of the students in the Kahuna Physics Institute tells the Physics Kahuna, “Hey, Mr. Gunderson just got a Ferrari.” This s ...
... tells a friend out in the hall, “Mr. Gunderson just bought a sports car, I think he got a Ferrari.” The Physics Kahuna supposes that this is possible. Anyway, two hours later one of the students in the Kahuna Physics Institute tells the Physics Kahuna, “Hey, Mr. Gunderson just got a Ferrari.” This s ...
Recent Developments in Physics Beyond the Standard
... relations, because the right-handed neutrinos are SU (5) singlets. An interesting alternative [5] is that the large mixings reside instead in the left-handed neutrinos. This is compatible with SU (5) if the Yukawa coupling matrices are highly asymmetric. Indeed, the SU(5) relation between the charge ...
... relations, because the right-handed neutrinos are SU (5) singlets. An interesting alternative [5] is that the large mixings reside instead in the left-handed neutrinos. This is compatible with SU (5) if the Yukawa coupling matrices are highly asymmetric. Indeed, the SU(5) relation between the charge ...
Schutz A First Course in General Relativity(Second Edition).
... The first part of the book, up to Ch. 8, introduces the theory in a sequence that is typical of many treatments: a review of special relativity, development of tensor analysis and continuum physics in special relativity, study of tensor calculus in curvilinear coordinates in Euclidean and Minkowski ...
... The first part of the book, up to Ch. 8, introduces the theory in a sequence that is typical of many treatments: a review of special relativity, development of tensor analysis and continuum physics in special relativity, study of tensor calculus in curvilinear coordinates in Euclidean and Minkowski ...
On the anomalous secular increase of the eccentricity of the orbit of
... modeling the tidal dissipation in both the Earth and the Moon was given. Later, Williams & Dickey (2003), relying upon Williams et al. (2001), yielded an anomalous eccentricity rate as large as ėmeas = (1.6 ± 0.5) × 10−11 yr−1 . Anderson & Nieto (2010) commented that eq. (1) is not compatible with ...
... modeling the tidal dissipation in both the Earth and the Moon was given. Later, Williams & Dickey (2003), relying upon Williams et al. (2001), yielded an anomalous eccentricity rate as large as ėmeas = (1.6 ± 0.5) × 10−11 yr−1 . Anderson & Nieto (2010) commented that eq. (1) is not compatible with ...
