A systematic linear analysis of the perturbations induced by cosmic strings in cold dark matter is presented. The power spectrum is calculated and it is found that the strings produce a great deal of power on small scales. It is shown that the perturbations on interesting scales are the result of many uncorrelated string motions, which indicates a much more Gaussian distribution than was previously supposed
We study the effects of cosmic strings on structure formation in open universes. We calculate the po...
We investigate the non-gaussian properties of cosmic-string-seeded linear density perturbations with...
We investigate the contribution made by small loops from a cosmic string network as seeds for large-...
We describe a detailed study of string-seeded structure formation using high resolution numerical si...
We describe a detailed study of string-seeded structure formation using high resolution numerical si...
We describe the detailed study and results of high-resolution numerical simulations of string-induce...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
A systematic analysis is challenging popular ideas about perturbation from cosmic strings. One way i...
The Zeldovich approximation is applied to study the accretion of hot and cold dark matter onto movin...
The clustering of baryons and cold dark matter induced by a single moving string is analyzed numeric...
We compute the power spectra in the cosmic microwave background and cold dark matter (CDM) fluctuati...
A broad class of models that describe physics beyond the Standard Model of ParticlePhysics predicts ...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
We investigate the non-Gaussian properties of cosmic string-seeded linear density perturbations with...
We study the effects of cosmic strings on structure formation in open universes. We calculate the po...
We investigate the non-gaussian properties of cosmic-string-seeded linear density perturbations with...
We investigate the contribution made by small loops from a cosmic string network as seeds for large-...
We describe a detailed study of string-seeded structure formation using high resolution numerical si...
We describe a detailed study of string-seeded structure formation using high resolution numerical si...
We describe the detailed study and results of high-resolution numerical simulations of string-induce...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
A systematic analysis is challenging popular ideas about perturbation from cosmic strings. One way i...
The Zeldovich approximation is applied to study the accretion of hot and cold dark matter onto movin...
The clustering of baryons and cold dark matter induced by a single moving string is analyzed numeric...
We compute the power spectra in the cosmic microwave background and cold dark matter (CDM) fluctuati...
A broad class of models that describe physics beyond the Standard Model of ParticlePhysics predicts ...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
We describe the results of high-resolution numerical simulations of string-induced structure formati...
We investigate the non-Gaussian properties of cosmic string-seeded linear density perturbations with...
We study the effects of cosmic strings on structure formation in open universes. We calculate the po...
We investigate the non-gaussian properties of cosmic-string-seeded linear density perturbations with...
We investigate the contribution made by small loops from a cosmic string network as seeds for large-...