Design and Implementation of the ABRACADABRA-10 cm Axion Dark Matter Search

The past few years have seen a renewed interest in the search for light particle dark matter. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, $10^{-12}\lesssim m_a\lesssim10^{-6}$ eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to QCD axion couplings. In this paper, we present the details of the design, construction, and data analysis for the first axion dark matter search with the ABRACADABRA-10 cm detector. We include a detailed discussion of the statistical techniques used to extract the limit from the first result with an emphasis on creating a robust statistical footing for interpreting those limits.Comment: 12 pages, 8 figure

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Multi-messenger Observations of a Binary Neutron Star Merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ∼ 1.7 {{s}} with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of {40}-8+8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 {M}ȯ . An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ∼ 40 {{Mpc}}) less than 11 hours after the merger by the One-Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ∼10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ∼ 9 and ∼ 16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC 4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.</p

Next generation MDM-the new 360 view

If your priority is to establish best in class customer-centricity principles in your business, then please join us for a review of how relationship centric MDM is the newest and most effective way to take command of your customer data and deliver business value faster. In this session you will hear how Pitney Bowes Software is assisting the University of Wollongong in expanding their vision of using Information Management to improve research outcomes, commercial partnerships and student learning experiences. This session will examine the: • Utilisation of Master Data principles and Relationship Analysis in understanding and exploring the current state of the University of Wollongong\u27s collaborations and to facilitate improvement • Importance of visualisation to translate master data into meaningful information that assists decision makers • Lessons learned and experience gained from the successful proof of concept • Future directions for the application using these techniques within the Universit

ABRACADABRA, A Search for Low-Mass Axion Dark Matter

ABRACADABRA is a proposed experiment to search for ultralight ($10^{-14} - 10^{-6}\mathrm{eV}$) axion dark matter. When ultralight axion dark matter encounters a static magnetic field, it sources an effective electric current that follows the magnetic field lines and oscillates at the axion Compton frequency. In the presence of axion dark matter, a large toroidal magnet will act like an oscillating current ring, whose induced magnetic flux can be measured by an external pickup loop inductively coupled to a SQUID magnetometer. Both broadband and resonant readout circuits are considered. ABRACADABRA is fielding a 10-cm prototype in 2017 with the intention of scaling to a 1 m$^3$ experiment. The long term goal is to probe QCD axions at the GUT-scale

First Results from ABRACADABRA-10 cm: A Search for Sub-μeV Axion Dark Matter

The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axionlike particle dark matter is relatively unexplored, particularly at masses m_{a}≲1  μeV. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, 10^{-12}≲m_{a}≲10^{-6}  eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between g_{aγγ}<1.4×10^{-10} and g_{aγγ}<3.3×10^{-9}  GeV^{-1} over the mass range 3.1×10^{-10}–8.3×10^{-9}  eV. These results are competitive with the most stringent astrophysical constraints in this mass range

Foundation economy: the infrastructure of everyday life

Privatisation, market choice, outsourcing: these are the watchwords that have shaped policy in numerous democratic states in the last generation. The end result is the degradation of the foundational economy. The foundational economy encompasses the material infrastructure at the foundation of civilised life - things like water pipes and sewers - and the providential services like education, health care and care for the old which are at the base of any civilised life. This book shows how these services were built up in the century between 1880 and 1980 so that they were collectively paid for, collectively delivered and collectively consumed. This system of provision has been undermined in the age of privatisation and outsourcing. The book describes the principles that should guide renewal of the foundational economy and the initiatives which could begin to put these principles into practice

Foundation economy: the infrastructure of everyday life

Privatisation, market choice, outsourcing: these are the watchwords that have shaped policy in numerous democratic states in the last generation. The end result is the degradation of the foundational economy. The foundational economy encompasses the material infrastructure at the foundation of civilised life - things like water pipes and sewers - and the providential services like education, health care and care for the old which are at the base of any civilised life. This book shows how these services were built up in the century between 1880 and 1980 so that they were collectively paid for, collectively delivered and collectively consumed. This system of provision has been undermined in the age of privatisation and outsourcing. The book describes the principles that should guide renewal of the foundational economy and the initiatives which could begin to put these principles into practice