SOUVENIR ALL INDIA COORDINATED RESEARCH PROJECT FOR DRYLAND AGRICULTURE CRIDA, HYDERABAD XV Working Group Meeting (24th-27th December, 2015) BISWANATH CHARIALI CENTRE ASSAM AGRICULTURAL UNIVERSITY

Not AvailableIt is my proud privilege to express heartfelt thanks to the entire AICRPDA family for giving me the responsibility of bringing out a souvenir to commemorate the occasion of XVth Working Group Meeting of AICRPDA at Biswanath Chariali Centre, BNCA, Assam Agricultural University. I, on behalf of the editorial board do extend a warm welcome to all delegate scientists and dignitaries coming from different parts of our country to this holy historic place of Biswanath, popularly known as ‘Gupta Kanshi’. Holding such a mega event of national importance for the first time at a place like Biswanath Chariali at the far east of the country amidst the bounty of natural resources and an area being almost entirely rainfed is of great significance. In view of the aim of realizing the dream of another green revolution that is envisaged from the rainfed areas of the country particularly the eastern and north eastern parts; this workshop is expected to march ahead further for achieving the goal. The vast ‘Gene’ resource of the North East India offers plenty of scope for their utilization to cope up the challenges of rainfed agriculture. This is a challenging task of converting these ‘Gene’ resources into viable ‘Seed Resources’ for their commercial exploitation keeping the very natural resource base and integrity unaltered. A holistic effort with all modern technological interventions is the need of the hour to bring into sustainable utilization of the natural resource base of the region. The idea of bringing out the souvenir in its present form came with the realization of the need of accumulating the multitude of the concepts required for framing the objectives of rainfed area research particularly for the North Eastern part of India. I am fortunate to have the wholehearted response from many luminaries from several ICAR institutes including CRIDA and number dignified scientists from the Assam Agricultural University contributing their valuable articles. I, do express gratitude and thankfulness from my inner core of the heart to all of them for their valuable contributions. I am extremely grateful to the Honorable Vice Chancellor, AAU, Dr. Kamalmalla Bujarbaruah sir, for his constant inspiration and suggestions all along the organization of the workshop. I would also like to express my sincere gratitude to Dr. Srinivasa Rao, Director, CRIDA, Dr. G. N. Hazarika, Director of Research (Agri), AAU, Dr.G.Rabindra Charry, PC, AICRPDA, Dr. T.C. Baruah, Associate Dean, BNCA, Dr. P.K. Sarma, CS, AICRPDA and all associated scientists for their encouragement, moral support and valuable suggestions. Last but not the least, all the Research Associates working under AICRPDA, BNCA, do deserve due share of thanks for their all round helps in bringing out the souvenir.Not Availabl

Search for low-mass dark matter with CDMSlite using a profile likelihood fit

The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) searches for interactions between dark matter particles and germanium nuclei in cryogenic detectors. The experiment has achieved a low energy threshold with improved sensitivity to low-mass (/c2) dark matter particles. We present an analysis of the final CDMSlite data set, taken with a different detector than was used for the two previous CDMSlite data sets. This analysis includes a data salting method to protect against bias, improved noise discrimination, background modeling, and the use of profile likelihood methods to search for a dark matter signal in the presence of backgrounds. We achieve an energy threshold of 70 eV and significantly improve the sensitivity for dark matter particles with masses between 2.5 and 10 GeV/c2 compared to previous analyses. We set an upper limit on the dark matter-nucleon scattering cross section in germanium of 5.4×10−42 cm2 at 5 GeV/c2, a factor of ∼2.5 improvement over the previous CDMSlite result

Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

This article presents an analysis and the resulting limits on light dark matter inelastically scattering off of electrons, and on dark photon and axionlike particle absorption, using a second-generation SuperCDMS high-voltage eV-resolution detector. The 0.93 g Si detector achieved a 3 eV phonon energy resolution; for a detector bias of 100 V, this corresponds to a charge resolution of 3% of a single electron-hole pair. The energy spectrum is reported from a blind analysis with 1.2 g-days of exposure acquired in an above-ground laboratory. With charge carrier trapping and impact ionization effects incorporated into the dark matter signal models, the dark matter-electron cross section ¯ is constrained for dark matter masses from 0.5 to 104  MeV/2; in the mass range from 1.2 to 50  eV/2 the dark photon kinetic mixing parameter and the axioelectric coupling constant ⁢ are constrained. The minimum 90% confidence-level upper limits within the above-mentioned mass ranges are ¯=8.7×10−34  cm2, =3.3×10−14, and ⁢=1.0×10−9

Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated Above Ground

We present limits on spin-independent dark matter-nucleon interactions using a $10.6$ $\mathrm{g}$ Si athermal phonon detector with a baseline energy resolution of $\sigma_E=3.86 \pm 0.04$ $(\mathrm{stat.})^{+0.19}_{-0.00}$ $(\mathrm{syst.})$ $\mathrm{eV}$. This exclusion analysis sets the most stringent dark matter-nucleon scattering cross-section limits achieved by a cryogenic detector for dark matter particle masses from $93$ to $140$ $\mathrm{MeV}/c^2$, with a raw exposure of $9.9$ $\mathrm{g}\cdot\mathrm{d}$ acquired at an above-ground facility. This work illustrates the scientific potential of detectors with athermal phonon sensors with eV-scale energy resolution for future dark matter searches.Comment: 7 pages, 4 figures, this version includes ancillary files from official data releas

Light dark matter constraints from SuperCDMS HVeV detectors operated underground with an anticoincidence event selection

This article presents constraints on dark-matter-electron interactions obtained from the first underground data-taking campaign with multiple SuperCDMS HVeV detectors operated in the same housing. An exposure of 7.63  g−days is used to set upper limits on the dark-matter-electron scattering cross section for dark matter masses between 0.5 and 1000  MeV/2, as well as upper limits on dark photon kinetic mixing and axionlike particle axioelectric coupling for masses between 1.2 and 23.3  eV/2. Compared to an earlier HVeV search, sensitivity was improved as a result of an increased overburden of 225 meters of water equivalent, an anticoincidence event selection, and better pile-up rejection. In the case of dark-matter-electron scattering via a heavy mediator, an improvement by up to a factor of 25 in cross section sensitivity was achieved

Constraints on low-mass, relic dark matter candidates from a surface-operated SuperCDMS single-charge sensitive detector

This article presents an analysis and the resulting limits on light dark matter inelastically scattering off of electrons, and on dark photon and axionlike particle absorption, using a second-generation SuperCDMS high-voltage eV-resolution detector. The 0.93 g Si detector achieved a 3 eV phonon energy resolution; for a detector bias of 100 V, this corresponds to a charge resolution of 3% of a single electron-hole pair. The energy spectrum is reported from a blind analysis with 1.2 g-days of exposure acquired in an above-ground laboratory. With charge carrier trapping and impact ionization effects incorporated into the dark matter signal models, the dark matter-electron cross section σ_e is constrained for dark matter masses from 0.5 to 10⁴  MeV/c²; in the mass range from 1.2 to 50  eV/c² the dark photon kinetic mixing parameter ϵ and the axioelectric coupling constant gae are constrained. The minimum 90% confidence-level upper limits within the above-mentioned mass ranges are σ_e = 8.7×10⁻³⁴ cm², ϵ = 3.3×10⁻¹⁴, and g_(ae) = 1.0×10⁻⁹

Light dark matter constraints from SuperCDMS HVeV detectors operated underground with an anticoincidence event selection

This article presents constraints on dark-matter-electron interactions obtained from the first underground data-taking campaign with multiple SuperCDMS HVeV detectors operated in the same housing. An exposure of 7.63  g−days is used to set upper limits on the dark-matter-electron scattering cross section for dark matter masses between 0.5 and 1000  MeV/2, as well as upper limits on dark photon kinetic mixing and axionlike particle axioelectric coupling for masses between 1.2 and 23.3  eV/2. Compared to an earlier HVeV search, sensitivity was improved as a result of an increased overburden of 225 meters of water equivalent, an anticoincidence event selection, and better pile-up rejection. In the case of dark-matter-electron scattering via a heavy mediator, an improvement by up to a factor of 25 in cross section sensitivity was achieved