5 citations · 5 across the 7 of their papers we have counts for
7 papers
Cross-sections and experimental signatures for detection of a well-defined dark matter WIMP
Bailey Tallman, Jehu Martinez, Rohan Shankar +2
We report the following calculations for a recently proposed bosonic dark matter WIMP with well-defined interactions: (1)~the mass as determined by fitting to the relic abundance;…
Experimental signatures of an alternative supersymmetry
Roland E. Allen
There are at least three physical arguments for some form of supersymmetry, based on experiment and observation, but conventional supersymmetry (SUSY) has not been observed up to s…
The cosmological constant, dark matter, and other unsolved problems from a fresh perspective
Roland E. Allen
Quantum theory, general relativity, the standard model of particle physics, and the CDM model of cosmology have all been spectacularly successful within their respective regimes…
Potential for definitive discovery of a 70 GeV dark matter WIMP with only second-order gauge couplings
Bailey Tallman, Alexandra Boone, Adhithya Vijayakumar +4
As astronomical observations and their interpretation improve, the case for cold dark matter (CDM) becomes increasingly persuasive. A particularly appealing version of CDM is a wea…
Indirect detection, direct detection, and collider detection cross-sections for a 70 GeV dark matter WIMP
Bailey Tallman, Alexandra Boone, Caden LaFontaine +9
Assuming a dark matter fraction and a reduced Hubble constant , we obtain a value of 70 GeV/c for the mass of the dark matter WIMP we have previously…
The Vacuum Energy from a New Perspective
A. R. Mondragon, R. E. Allen
It is commonly believed that the vacuum energy problem points to the need for (1) a radically new formulation of gravitational physics and (2) a new principle which forces the vacu…
Four Testable Predictions of Instanton Cosmology
R. E. Allen
A new cosmological model makes the following predictions: (1) The deceleration parameter is approximately zero. (2) The mass density parameter is less than 1. (3) T…