Are cosmological data sets consistent with each other within theΛcold dark matter model?
نویسندگان
چکیده
منابع مشابه
Linearizing sets: each other
It is has been well known since Fiengo and Lasnik (1973) and Langendoen (1978) that each other presents a high degree of contextual variability. In a tradition that goes back to Langendoen (1978) and later to Dalrymple et al. (1998), theoreticians have tried to list different truth conditions and to establish a criterion for determining which one holds in which particular context. Along the lin...
متن کاملSupersymmetric dark matter with a cosmological constant
Recent measurements of cosmological parameters from the microwave background radiation, type Ia supernovae, and the age of globular clusters help determine the relic matter density in the universe. It is first shown with mild cosmological assumptions that the relic matter density satisfies ΩMh 2 < 0.6 independent of the cosmological constant and independent of the SNIa data. Including the SNIa ...
متن کاملCosmological dark matter and ensoulment
Allocortical structures such as hippocampal formation and amygdala are involved in the emotions and memory, and regarded as the seat of personhood. Human body is a composite of a biological organism and an intellective soul. It was suggested that cerebral allocortex is the main region harboring the soul and the beginning of a human person as an individual living organism is at the 13 week of de...
متن کاملA New Cosmological Model of Quintessence and Dark Matter
We propose a new class of quintessence models in which late times oscillations of a scalar field give rise to an effective equation of state which can be negative and hence drive the observed acceleration of the universe. Our ansatz provides a unified picture of quintessence and a new form of dark matter we call Frustrated Cold Dark Matter (FCDM). FCDM inhibits gravitational clustering on small...
متن کاملAre the H 1 and ZEUS “ High Q 2 Anomalies ” Consistent with Each Other ?
Both ZEUS and H1 have recently reported an excess of events at high Q and high Bjorken–x. However, the x distributions differ considerably; moreover, H1 sees more events with lower luminosity. Taken separately, the x distributions and the number of observed events are consistent between the two experiments at the few percent level. However, when combined it becomes clear that the results of H1 ...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physical Review D
سال: 2016
ISSN: 2470-0010,2470-0029
DOI: 10.1103/physrevd.93.043522