Implications of collider experiments for detecting cold dark matter

By investigating the space of parameters of the minimal supersymmetric extension of the Standard Model, it is shown that an observation of at least one supersymmetric particle in high-energy experiments would increase considerably the importance of highly sensitive low-energy experiments aimed at detecting cold-dark-matter particles assumed to be neutralinos, the lightest supersymmetric particles, which are stable. On the other hand, nonobservation of direct signals from dark matter in such experiments can have a pronounced effect on the strategy of high-energy searches for the light charged Higgs boson.     

Search for particles of cold nonbarion dark matter in the EDELWEISS-II experiment

The EDELWEISS-II experiment is aimed at direct detection of weakly interacting massive particles (WIMP) considered as main candidates for the role of nonbarion dark matter. In the experiment, a search for rare WIMP-Ge scattering events is performed using HPGe-detectors-bolometers at a temperature of 20 mK. Because of different ionization losses of recoil nuclei and electrons, the use of detectors allowing simultaneous measurement of phonon and ionization signals enables background events to be suppressed very efficiently. To suppress actively the remained source of events simulating the WIMP signature, namely, the surface events with incomplete charge collection, detectors with coplanar ring electrodes have been developed for the EDELWEISS-II facility. The experimental coefficient of suppression of all EDELWEISS-II background components with the help of calibration measurements allows 3500 kg⋅day statistics to be accumulated with the expected zero level of the background events in the region of search for the WIMP. This enables the spinindependent WIMP-nucleon scattering events to be registered given that their cross section is greater than 10^-45 cm² (10^-9 pb) predicted by a wide class of the SUSY models.     

Constraints from the Wilkinson microwave anisotropy probe on decaying cold dark matter

We reformulate cosmological perturbations in the decaying cold dark matter model, and calculate cosmological microwave background anisotropies. By comparing our predictions with data from the Wilkinson Microwave Anisotropy Probe, we derive a new bound on the abundance and lifetime of decaying dark matter particles. The lifetime is constrained to Gamma(- 1)> or =123 Gyr at 68% C.L. (52 Gyr at 95.4% C.L.) when cold dark matter consists only of such decaying particles. We also consider a more general case and show that the constraint generalizes to Omega(DDM )h2 less, similar -0.5(Gamma (-1)/1 Gyr) (-1)+0.12 for Gamma(- 1)> or =5 Gyr at 95.4% C.L.     

Model for cold dark matter

We present a model for cold dark matter based upon continuum bound states of thee ⁺ e ^– system. These continuum bound states, referred to as photonium states to distinguish them from the well-known bound states of positronium, are shown to have cross sections and lifetime properties consistent with abundant production in the early universe and survival to the present time. Thus photonium can easily account for more than 90% of the total mass of the universe.The authors have benefitted from discussions with Charles J. Benesh. This work was supported in part by the US DOE grant no. DE-FG02-87ER40371, Division of High Energy and Nuclear Physics and by contract no. W-7405-ENG-82.     

Annihilating cold dark matter

Structure formation with cold dark matter (CDM) predicts halos with a central density cusp, which are observationally disfavored. If CDM particles have an annihilation cross section sigmav approximately 10(-29)(m/GeV) cm(2), then annihilations will soften the cusps. We discuss plausible scenarios for avoiding the early Universe annihilation catastrophe that could result from such a large cross section. The predicted scaling of core density with halo mass depends upon the velocity dependence of sigmav, and s-wave annihilation leads to a core density nearly independent of halo mass, which seems consistent with observations.     

Observational evidence for self-interacting cold dark matter

Cosmological models with cold dark matter composed of weakly interacting particles predict overly dense cores in the centers of galaxies and clusters and an overly large number of halos within the Local Group compared to actual observations. We propose that the conflict can be resolved if the cold dark matter particles are self-interacting with a large scattering cross section but negligible annihilation or dissipation. In this scenario, astronomical observations may enable us to study dark matter properties that are inaccessible in the laboratory.     

Planck-mass-rotons cold dark matter hypothesis

Sakharov's conjecture that the vacuum is densely occupied with Planck-mass maximons is taken as a model to explain the missing mass as rotons of a superfluid made up from the Planck-mass maximons. Because rotons require a finite excitation energy, they not only can account for the missing mass but, in addition, can mimic a small, positive cosmological constant. According to Sakharov, the large vacuum energy of the Planck-mass maximons is compensated by ghost particles. In the proposed superfluid vacuum model, we assume that the compensation is done by a large, negative cosmological constant instead.     

DBI models for the unification of dark matter and dark energy

We propose a model based on a DBI action for the unification of dark matter and dark energy. This is supported by the results of the study of its background behavior at early and late times, and reinforced by the analysis of the evolution of perturbations. We also perform a Bayesian analysis to set observational constraints on the parameters of the model using type Ia SN, CMB shift and BAO data. Finally, to complete the study we investigate its kinematics aspects, such as the effective equation of state parameter, acceleration parameter and transition redshift. Particularizing those parameters for the best fit one appreciates that an effective phantom is preferred.     

Messenger sneutrinos as cold dark matter

In models where supersymmetry breaking is communicated into the visible sector via gauge interactions the lightest supersymmetric particle is typically the gravitino which is too light to account for cold dark matter. We point out that the lightest messenger sneutrinos with mass in the range of one to three TeV may serve as cold dark matter over most of the parameter space due to one-loop electroweak radiative corrections. However, in the minimal model this mass range has been excluded by the direct dark matter searches. We propose a solution to this problem by introducing terms that explicitly violate the messenger number. This results in low detection rate for both direct and indirect searches and allows messenger sneutrinos to be a valid dark matter candidate in a wide region of SUSY parameter space.     

EDELWEISS experiment: Direct search for dark matter

The EDELWEISS experiment is aimed at direct searches for nonbaryonic cold dark matter by means of cryogenic germanium detectors. It is deployed at the LSM underground laboratory in the Frejus tunnel, which connects France and Italy. The results of the experimentmade it possible to set a limit on the spin-independent cross section for the scattering of weak-interacting massive particles (WIMP) at a level of 10^?6 pb. Data from 21 detectors of total mass about 7 kg are being accumulated at the present time.     

直接探测暗物质和中国暗物质实验

The nature of dark matter in our universe is one of the most challenging problems in science today. A most probable class of dark matter is the weakly interacting massive particles (WIMPs), which exhibit a wide range of features. Current experiments searching for dark matter aim for direct detection via the elastic scattering off ordinary matter in terrestrial detectors. This paper will present the main methods, status and roadmap for the direct detection of dark matter. The world's deepest laboratory, China Jinping underground laboratory and its extension, will also be described. Finally, we will give a detailed introduction to the research history, detection technologies, current results, and future prospects of China dark matter experiment (CDEX).     

Axion as a cold dark matter candidate

Here we generally prove that the axion as a coherently oscillating scalar field acts as a cold dark matter in nearly all cosmologically relevant scales. The proof is made in the linear perturbation order. Compared with our previous proof based on solutions, here we compare the equations in the axion with the ones in the cold dark matter, thus expanding the valid range of the proof. Deviation from purely pressureless medium appears in very small scale where axion reveals a peculiar equation of state. Our analysis is made in the presence of the cosmological constant, and our conclusions are valid in the presence of other fluid and field components.