Inflation Model Constrained from Astrophysics Observations

Particle Physics Inflation Model Constrained from Astrophysics Observations

The early Universe inflation [11] is well known as a promising theory to explain the origin of large scale structure of the Universe, a causal theory for the origin of primordial density fluctuations which may explain the observed density inhomogeneities and cosmic microwave fluctuations in the very early Universe, and to solve the early universe pressing problems for the standard hot big bang ...

Allowed parameter regions for a general inflation moded ∗

The early Universe inflation is well known as a promising theory to explain the origin of large scale structure of Universe and to solve the the early universe pressing problems [6]. For a resonable inflation model, the potential during inflation must be very flat in, at least, the direction of the inflaton. To construct the inflaton potential all the known related astrophysics observations sho...

Inflation and Output in a Cash Constrained Economy

 We examine permanent effects of monetary expansion in an economy where access to credit for financing consumption and investment is limited and consumers and firms are cash-constrained. The main difference between our model with those of Cooley-Hanson (1989) and Walsh (2003) is that investment, in addition to consumption, is subject to a cash-constraint. In this respect, our model is...

Seismology of solar spicules based on Hinode/SOT observations

Inflation model of Uzon caldera, Kamchatka, constrained by satellite radar interferometry observations

[1] We analyzed RADARSAT-1 synthetic aperture radar (SAR) data to compute interferometric SAR (InSAR) images of surface deformation at Uzon caldera, Kamchatka, Russia. From 2000 to 2003 approximately 0.15 m of inflation occurred at Uzon caldera, extending beneath adjacent Kikhpinych volcano. This contrasts with InSAR data showing no significant deformation during either the 1999 to 2000, or 200...