Search Publications

Probing Space-Time in the Solar System:. from Cassini to Bepicolombo
DOI: 10.1142/S0218271807011449 Bibcode: 2007IJMPD..16.2117I

Iess, Luciano; Asmar, Sami

Spacecraft radio science techniques can be used for precision solar system tests of relativistic gravity, as was demonstrated by the measurement of the Doppler shift of radio signals with the Cassini mission. Similar experiments are planned for the BepiColombo mission to Mercury. Recent theoretical developments based on string theory and inflation…

2007 International Journal of Modern Physics D
Cassini 23
Do Recent Supernovae ia Observations Tend to Rule Out all the Cosmologies?
DOI: 10.1142/S0218271807011036 Bibcode: 2007IJMPD..16.1641V

Vishwakarma, Ram Gopal

Dark energy and the accelerated expansion of the universe have been the direct predictions of the distant supernovae Ia observations which are also supported, indirectly, by the observations of the CMB anisotropies, gravitational lensing and the studies of galaxy clusters. Today these results are accommodated in what has become the concordance cos…

2007 International Journal of Modern Physics D
eHST 12
Light Superconducting Strings in the Galaxy
DOI: 10.1142/S0218271807011802 Bibcode: 2007IJMPD..16.2399F

Ferrer, Francesc; Vachaspati, Tanmay

Observations of the Milky Way by the SPI/INTEGRAL satellite have confirmed the presence of a strong 511 keV gamma ray line emission from the bulge, which requires an intense source of positrons in the galactic center. These observations are hard to account for by conventional astrophysical scenarios, whereas other proposals, such as light DM, face…

2007 International Journal of Modern Physics D
INTEGRAL 8
Constraints on Simplified Quartessence Cosmology from the Latest Observational Data
DOI: 10.1142/S0218271807011085 Bibcode: 2007IJMPD..16.1783W

Wu, Puxun; Dong, Sumei

The simplified generalized Chaplygin gas (GCG) model as a candidate of UDME is studied in this paper. By using the latest 162 ESSENCE type Ia supernovae (Sne Ia) data, 30 high red shift Sne Ia data and the distance ratio from z = 0.35 to z = 1089 (the red shift of decoupling), we obtain Ω k = 0.076-0.077+0.093 and …

2007 International Journal of Modern Physics D
eHST 0