We use a set of numerical N -body simulations to study the large-scale behavior of the reduced bispectrum of dark matter and compare the results with the second-order perturbation theory and the halo models for different halo mass functions. We find that the second-order perturbation theory (PT2) agrees with the simulations fairly well on large scales of k < 0.05 hMpc, but it shows a signature ...

[1] Many broadside coronal mass ejections (CMEs) propagate almost radially beyond the first couple of solar radii, and their angular widths remain nearly constant while propagating through the corona. Assuming that these characteristics hold true for halo CMEs that originate far from solar limbs, some useful geometric and kinematic properties of halo CMEs may be reproduced using a simple geomet...

Circadian variations of organ specific and lethal toxicities were investigated in female C3H mice following intraperitoneal injection(s) of 5-fluorouracil (5-FU) and/or cis-platinum (CDDP) with different doses at one of the four equidistant time points, viz., 3, 9, 15 and 21 HALO (Hours After Light On). Lethality, peripheral WBC count, spleen size, femoral bone marrow cell population and change...

We study the dependence of the galaxy contents within halos on the halo formation time using two galaxy formation models, one being a semianalytic model utilizing the halo assembly history from a high resolution N-body simulation and the other being a smoothed particle hydrodynamics simulation including radiative cooling, star formation, and energy feedback from galactic winds. We confirm the f...

We study the dependence of galaxy contents within halos on halo formation time using two galaxy formation models, one being a semi-analytic model utilizing halo assembly history from a high resolution N-body simulation and the other being a smoothed particle hydrodynamics simulation including radiative cooling, star formation, and energy feedback from galactic winds. We confirm the finding by G...