216 research outputs found

    Inert Doublet Dark Matter with an additional scalar singlet and 125 GeV Higgs Boson

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    In this work we consider a model for particle dark matter where an extra inert Higgs doublet and an additional scalar singlet is added to the Standard Model (SM) Lagrangian. The dark matter candidate is obtained from only the inert doublet. The stability of this one component dark matter is ensured by imposing a Z2Z_2 symmetry on this additional inert doublet. The additional singlet scalar has a vacuum expectation value (VEV) and mixes with the Standard Model Higgs doublet resulting in two CP even scalars h1h_1 and h2h_2. We treat one of these scalars, h1h_1, to be consistent with the SM Higgs like boson of mass around 125 GeV reported by the LHC experiment. These two CP even scalars affect the annihilation cross-section of this inert doublet dark matter resulting in a larger dark matter mass region that satisfies the observed relic density. We also investigate the h1→γγh_1 \rightarrow \gamma\gamma and h1→γZh_1 \rightarrow \gamma Z processes and compared these with LHC results. This is also used to constrain the dark matter parameter space in the present model. We find that the dark matter candidate in the mass region m12<mH<mW\frac {m_1} {2} < m_H < m_W GeV (m1=125m_1 = 125 GeV, mass of h1h_1) satisfies the recent bound from LUX direct detection experiment.Comment: 21 Pages, 5 Figures, 1 Tabl

    Extension of Minimal Fermionic Dark Matter Model : A Study with Two Higgs Doublet Model

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    We explore a fermionic dark matter model with a possible extension of Standard Model (SM) of particle physics into two Higgs doublet model. Higgs doublets couple to the singlet fermionic dark matter (FDM) through a non renormalisable coupling providing a new physics scale. We explore the viability of such dark matter candidate and constrain the model parameter space by collider serach, relic density of DM, direct detection measurements of DM-nucleon scattreing cross-section and with the experimentally obtained results from indirect search of dark matter.Comment: 22 pages, 17 new png figures, Title changed, new references added, major revisio

    Low Energy Gamma Ray Excess Confronting a Singlet Scalar Extended Inert Doublet Dark Matter Model

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    Recent study of gamma rays originating from the region of galactic centre has confirmed an anomalous γ\gamma-ray excess within the energy range 1-3 GeV. This can be explained as the consequence of pair annihilation of a 31-40 GeV dark matter into bbˉb \bar b with thermal annihilation cross-section σv∼1.4−2.0×10−26 cm3/s\sigma v \sim 1.4-2.0 \times 10^{-26}~\rm{cm^3/s}. In this work we revisit the Inert Doublet Model (IDM) in order to explain this gamma ray excess. Taking the lightest inert particle (LIP) as a stable DM candidate we show that a 31-40 GeV dark matter derived from IDM will fail to satisfy experimental limits on dark matter direct detection cross-section obtained from ongoing direct detection experiments and is also inconsistent with LHC findings. We show that a singlet extended inert doublet model can easily explain the reported γ\gamma-ray excess which is as well in agreement with Higgs search results at LHC and other observed results like DM relic density and direct detection constraints.Comment: 17 pages, 4 figure

    Possible explanation of indirect gamma ray signatures from hidden sector fermionic dark matter

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    We propose the existence of a hidden or dark sector besides the standard model (SM) of particle physics, whose members (both fermionic and bosonic) obey a local SU(2)H_{\rm H} gauge symmetry while behaving like a singlet under the SM gauge group. However, the fermiomic fields of the dark sector also possess another global U(1)H_{\rm H} symmetry which remains unbroken. The local SU(2)H_{\rm H} invariance of the dark sector is broken spontaneously when a scalar field in this sector acquires a vacuum expectation value (VEV) and thereby generating masses to the dark gauge bosons and dark fermions charged under the SU(2)H_{\rm H}. The lightest fermion in this dark SU(2)H_{\rm H} sector can be a potential dark matter candidate. We first examine the viability of the model and constrain the model parameter space by theoretical constraints such as vacuum stability and by the experimental constraints such as PLANCK limit on relic density, LHC data, limits on spin independent scattering cross-section from dark matter direct search experiments etc. We then investigate the gamma rays from the pair annihilation of the proposed dark matter candidate at the Galactic Centre region. We also extend our calculations of gamma rays flux for the case of dwarf galaxies and compare the signatures of gamma rays obtained from these astrophysical sites.Comment: 33 pages, 16 figures, title changed, major revisio

    Two component WIMP-FImP dark matter model with singlet fermion, scalar and pseudo scalar

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    We explore a two component dark matter model with a fermion and a scalar. In this scenario the Standard Model (SM) is extended by a fermion, a scalar and an additional pseudo scalar. The fermionic component is assumed to have a global U(1)DM{\rm U(1)}_{\rm DM} and interacts with the pseudo scalar via Yukawa interaction while a Z2\mathbb{Z}_2 symmetry is imposed on the other component -- the scalar. These ensure the stability of both the dark matter components. Although the Lagrangian of the present model is CP conserving, however the CP symmetry breaks spontaneously when the pseudo scalar acquires a vacuum expectation value (VEV). The scalar component of the dark matter in the present model also develops a VEV on spontaneous breaking of the Z2\mathbb{Z}_2 symmetry. Thus the various interactions of the dark sector and the SM sector are progressed through the mixing of the SM like Higgs boson, the pseudo scalar Higgs like boson and the singlet scalar boson. We show that the observed gamma ray excess from the Galactic Centre, self-interaction of dark matter from colliding clusters as well as the 3.55 keV X-ray line from Perseus, Andromeda etc. can be simultaneously explained in the present two component dark matter model.Comment: 35 pages, 5 figure

    Toward a framework for mitigating object detection decision making bias in driverless cars

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    Bias in machine learning is a significant problem that demands industry-wide attention, and in the case of driverless vehicles, life and death are at stake. The debate is whether autonomous vehicles are safe, yet more likely to strike a pedestrian of color than a person of white skin color. It is essential to obtain a greater understanding of the algorithmic bias that occurs during driving-centric object recognition. Major automakers plan to develop cars with a degree of autonomy between Level 4 and Level 5 within the next decade. At Level 5, the system is meant to behave similarly to a human driver; it can drive anyplace lawful and can make independent decisions (SAE International 2016)
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