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Galaxies
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41by Dibert, Karia Radh“... dark matter, which serves as an alternative to collisionless cold dark matter, may be useful...”
Published 2019
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42by Lee Jae-Weon“... matter acts like cold dark matter, while below the scale quantum pressure from the uncertainty principle...”
Published 2018-01-01
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43by Schewtschenko, Jascha Alexander“...-cold dark matter component. We focus in the first case on models with a non-vanishing interaction cross...”
Published 2016
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45by Felipe Andrade Oliveira“... and cold dark matter. The nonexistence of a dark energy component implies that our scenario is based on a...”
Published 2010
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46by Oliveira, Felipe Andrade“... and cold dark matter. The nonexistence of a dark energy component implies that our scenario is based on a...”
Published 2010
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47by Ahmad Borzou“... that the standard model (SM) neutrinos can be the cold dark matter (CDM) because (1.) the expansion of the universe...”
Published 2018-08-01
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48by Makhathini, Sphesihle.“... with that of cold dark matter. We show that we can sufficiently describe the VCG cosmology from decoupling to today...”
Published 2013
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49by Sergey Paston“... of embedding matter turns out to be slow enough so that it can play the role of cold dark matter. The non...”
Published 2020-09-01
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50by Kaboth, Asher C. (Asher Cunningham)“..., and directional detection of cold dark matter. The cosmic neutrino background is investigated through the KATRIN...”
Published 2013
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52“... can not only have the same large-scale success of cold dark matter but also alleviates the ”small...”
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53by Dolle, Ethan Michael“...Cosmological observations have precisely measured the amount of cold dark matter (CDM...”
Published 2009
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54“... level; moreover, the new scalar bosons involved in the loop corrections play a role as stable cold dark...”
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55by Hall, Jonathan“... if it contributes to cold dark matter and this means that tan(β) cannot be too large. A new variant of the E6SSM...”
Published 2011
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56by Dodds, Stephen James“...-space distortion is required, Ω<SUP>0.6</SUP>/<I>b<SUB>IRAS</SUB></I> = 1.0±0.2. A Cold Dark Matter...”
Published 1996
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58by Abhik Kumar Sanyal“..., in the presence of background cold dark matter. Such crossing is a sufficiently late time transient phenomenon...”
Published 2009-01-01
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59by Ratcliffe, Andrew“... detection of large scale power above and beyond that of the standard cold dark matter cosmological model...”
Published 1996
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60by Choi, Jun-Hwan“... processes of satellite disruption in cold dark matter host halos using idealized N-body simulations...”
Published 2007
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