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It is our great honor to invite you to the 7th Fermi Asian Network Workshop (FAN7), which will be held during Dec 7-11, 2017, in Lijiang, China. The FAN was established in 2010 to promote collaboratio...
It is our great honor to invite you to the 7th Fermi Asian Network Workshop (FAN7), which will be held during Dec 7-11, 2017, in Lijiang, China. The FAN was established in 2010 to promote collaboratio...
FERMI ACCELERATION     FERMI ACCELERATION  particle       2015/9/29
Fermi acceleration is a mechanism, first suggested by Enrico Fermi in 1949, to explain heating of particles in cosmic rays.
Two approaches for the efficient rational approximation of the Fermi-Dirac function are discussed: one uses the contour integral representation and conformal mapping, and the other is based on a versi...
There is a mass very huge star in Milky Way Galactic disk center, known as Milky Way "Nuclear-Star". Nuclear-Star mass exceeds solar mass 9 trillion times. Nuclear-Star center temperature exceed solar...
Spin-echo experiments are reported for 3He-4He solutions under extremely high B/T conditions, B=14.75  T and T≥1.73  mK. The 3He concentration x3 was adjusted close to the valu...
We simulate the dilute attractive Fermi–Hubbard model in the unitarity regime using a diagrammatic determinant Monte Carlo (MC) algorithm with worm-type updates. We obtain the dependence of the critic...
The viscosity is measured for a Fermi liquid, a dilute 3He-4He mixture, under extremely high magnetic field/temperature conditions (B≤14.8  T, T≥1.5  mK). The spin-splitting en...
We use the diagrammatic Monte Carlo approach to solve the problem of a single spin-down fermion resonantly interacting with a Fermi gas of spin-up particles. Our solution is important for understandin...
Fermi卫星于2008.6正式发射升空并取得了一系列令人瞩目的观测上的重大突破。2011.12我国的暗物质粒子探测卫星项目得以正式启动。为给暗物质粒子卫星将来的数据处理培养青年骨干,我们将于2013.1-2013.2在南京组织一个小规模的Fermi数据处理workshop(由于场地所限,学员仅限于对暗物质项目很感兴趣的博士生/博士后或低年级硕士生,总不超过10人;旁听不超过5人),对爆发性点源、...
Finding the ground state of a fermionic Hamiltonian using quantum Monte Carlo is a very difficult problem, due to the Fermi sign problem. While still scaling exponentially, full configuration-interact...
We investigate single-particle properties of a one-component Fermi gas with a tunable p-wave interaction. Including pairing fluctuations associated with this anisotropic interaction within a $T$-matri...
The gamma-ray sky >100 MeV is dominated by the diffuse emissions from interactions of cosmic rays with the interstellar gas and radiation fields of the Milky Way. Observations of these diffuse emissio...
The F-GAMMA program is a coordinated effort to investigate the physics of Active Galactic Nuclei (AGNs) via multi-frequency monitoring of Fermi blazars. In the current study we show and discuss the ev...
Recent detections of GeV photons in a few GRBs by Fermi-LAT imply huge bulk Lorentz factors to avoid a large gamma gamma optical depth at high energy. Estimates can be as high as Gamma ~ 1000 in the m...

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