Analysis of the Dose Commitments Resulting from Atmospheric Transport and Deposition from Nuclear Risk Sites in the Russian Far East

The purpose of this study was to estimate the worst-case case dose commitments and potential consequences of accidental releases at nuclear risk sites in the Russian Far East. The nuclear risk sites of concern are near Petropavlovsk (52055'N & 158030'E) and Vladivostok (42055'N & 132025'E). The region of interest includes the territories of the Russian Far East, China, Japan, North and South Korea, State of Alaska, the Aleutian Islands, Mongolia, Burma, Hong Kong, Laos, Taiwan, Thailand, and Vietnam. The transboundary region (i.e., that outside of Russia) is of primary interest because the largest doses resulting from hypothetical releases from these sites would reside in Russia and would be examined using site specific information and detailed models that were unavailable for this study. However, the transboundary region can be examined, in general, using existing information and models. The The methodology from the United Nations Scientific Committee on the Effects of Atomic Radiation (UNSCEAR) 1993 Report was used in this study to estimate effective dose commitments. It is recognized that this methodology is not the only acceptable manner to estimate such doses; the methodology was selected because it is independent, defensible, and, because it is based upon a multiplicative model, lends itself to a facile examination of parameter variation. The research tool used to generate the deposition data used as the basis of this study was a long-range transport model - the Danish Emergency Response Model of the Atmosphere (DERMA) which was used to simulate the 5-d atmospheric transport, dispersion and deposition of Cs-137 for a one-day release at a rate of 10Bq s-1 for a total "unit hypothetical release" of 8.64x10 14 Bq. The meteorological data from the European Center for Medium- Range Weather Forecasts (ECMWF, Reading, UK) based on the ECMWF global model forecast and analysis were used as input data for the model simulation. Using the DERMA model, the total Cs-137 depositions (i.e., sums of pertinent dry and wet deposition values) were computed for over 90% of the days in calendar year 2000. The necessary meteorological data was missing for the remaining days. In this report, Sr-90 and I-131 were radionuclides that might also have been of concern depending upon the conditions of the study. However, because of a lack of time and resources, the deposition values were not computed for these radionuclides for all calendar year 2000 days. There were Sr-90 and I-131 concentration and deposition data provided for selected days that were considered representative of the variation of the climactic condtions for the region for the year 2000. These data were used to generate simple, linear linear relationships between the unavailable Sr-90 and I-131 concentration and deposition data and the corresponding Cs-137 data. These relationships were found to be sufficiently accurate for the general examination undertaken in this report and were used to generate the necessary, unavailable data. From an examination of the appropriate source term information and deposition to dose transfer factors from both the UNSCEAR 1993 Report and the worst-case scenario, Cs-137 was determined to be the radionuclide of primary concern for this study. The Cs-137 deposition- to-dose transfer factor was dominated by the external exposure (to ground deposition) pathway. For the Petropavlovsk nuclear risk site, the maximum Cs-137 total deposition (locates in Russia) translated into a worst-case maximum effective dose commitment of 108 mSv per person for the maximum exposed individual (i.e., teen). For the transboundary region (i.e., that area outside of Russia), the maximum effective dose commitment was 5.0 mSv per teen. This maximum value was located in the State of Alaska; the maximum effective dose commitment for the Aleutian Islands was 3.3 mSv per teen. The maximum effective dose commitments in the effected U.S. territories were generally three to four times higher than those in Japan, the transboundary country with the next highest maximum dose commitments resulting from accidental releases from the Petropavlovsk risk site. For the Vladivostok nuclear risk site, the maximum Cs-137 137 total deposition (located again in Russia) translated into a worst-case maximum effective dose commitment of 102 mSv per teen. For the transboundary region, the maximum effective dose commitment for Cs-137 was 27 mSv per teen. These maximum values were located in China, which is proximate to the Vladivostok site. The maximum effective dose commitments for Japan and N. Korea are approximately the same (i.e., within a factor of two) as that for China. Note that the maximum effective dose commitments in the U.S. territories are generally more than a factor of 60 lower than those in China, the transboundary country with the highest maximum dose commitments resulting from accidental releases from the Vladivostok risk site. The maximum worst-case dose commitments corresponding to the potential Petropavlovsk and Vladivostok releases for both the regional and transboundary conditions were also compared to various annual reference levels (i.e., 0.15, 1.0, 10, and 100 mSv per person) discussed in the International Commission on Radiological Protection (ICRP) 82 Report pertaining to practices and interventions and the annual background radiation dose (i.e., 2.4 mSv per person) provided in the UNSCEAR 1993 Report. These comparisons were conservative because the effective dose commitments computed in this report are being compared to annual reference values and background doses. The worst-case maximum dose commitments from the Petropavlovsk site for the transboundary region on over 99% of all year 2000 days studied are less than the average annual background radiation dose. For the Vladivostok releases, the worst-case maximum dose commitments are less than the average annual background radiation dose for more than 44% of all year 2000 days studied. Furthermore, the maximum dose commitments corresponding to the Vladivostok releases for more than 90% of the year 2000 days studied are less than the annual 10 mSv per person level in which interventions are rarely justified and are all less than the annual 100 mSv per person level in which interventions are almost always justifiable according to ICRP 82. Therefore, the impacts from the adjusted Vladivostok releases would be, in general, more significant than those from Petropavlovsk (even though the Petropavlovsk releases translate into the maximum, worst-case dose commitment). The more significant impacts of the potential Vladivostok releases were compounded by the fact that many more people were impacted than from the corresponding hypothetical Petropavlovsk releases. However, the dose commitments from the potential Vladivostok releases could be considered negligible when compared to the 10 mSv per person level in which interventions are rarely justified. The maximum collective dose commitments corresponding to the worst-case dose commitments were also computed. The results indicate that even though the maximum effective dose commitments from the Petropavlovsk and Vladivostok releases were similar, the larger populations impacted by the Vladivostok releases generally resulted in significantly larger collective dose commitments and thus potential mortalities than those for the Petropavlovsk releases. For example, the maximum number of additional mortalities on a regional basis resulting from the worst-case Petropavlovsk scenario would be 355 with as many as 329 in Japan, 83 in China, 18 in the State of Alaska, and 10 in S. Korea. However, for the Vladivostok releases, there could be as many as 9771 additional mortalities on a regional basis, and the additional mortalities for Japan, China, N. Korea, S. Korea, Russia, and Taiwan would be 9501, 8575, 2485, 2436, 1614, and 318, respectively. The U.S. territories and Hong Kong might have an additional two mortalities each. However, even though these mortality numbers may appear large, it should be noted that none of the transboundary values exceed 9 mortalities per 100 000 persons, which is found in N. Korea resulting from the worst-case Vladivostok scenario. Because the aggregation of doses over large areas is contrary to the recommendation of the ICRP, a series of threshold values were imposed on the worst-case results to determine whether the conclusions would change dramatically. The impact on the maximum worst-case collective dose commitments for the Petropavlovsk releases would be significan. For example, if a threshold of 1 mSv per person is imposed on the collective dose computation, then the collective dose commitment for all transboundary areas except for the U.S. territories falls to zero (and this includes Japan, which had the largest collective dose commitment). However, the impact of imposing such thresholds on the collective dose commitments from the Vladivostok releases was much less profound than that for the corresponding Petropavlovsk dose commitments; in fact, the imposition of thresholds up to 1 mSv per person had little impact on the collective dose commitments for most countries in the region of interest. Even though the impact on the collective doses related to the Vladivostok releases was small, it remains true that the worst-case impacts of the effective dose commitments for the releases from both the Vladivostok and Petropavlovsk sites were negligible when compared to metrics such as the average annual background dose and other causes of death in the affected countries

Meditation-induced bliss viewed as release from conditioned neural (thought) patterns that block reward signals in the brain pleasure center

The nucleus accumbens orchestrates processes related to reward and pleasure, including the addictive consequences of repeated reward (e.g., drug addiction and compulsive gambling) and the accompanying feelings of craving and anhedonia. The neurotransmitters dopamine and endogenous opiates play interactive roles in these processes. They are released by natural rewards (i.e., food, water, sex, money, play, etc.) and are released or mimicked by drugs of abuse. Repeated drug use induces conditioned down-regulation of these neurotransmitters, thus causing painful suppression of everyday pleasure. As with many spiritual traditions, Buddhism provides strong advice against the pursuit of worldly pleasures to attain the ‘‘good life.’’ In contrast, many forms of meditation give rise to an immense and abiding joy. Most of these practices involve ‘‘stilling the mind,’’ whereby all content-laden thought (e.g., fantasies, daydreams, plans) ceases, and the mind enters a state of openness, formlessness, clarity, and bliss. This can be explained by the Buddhist suggestion that almost all of our everyday thoughts are a form of addiction. It follows that if we turn off this internal ‘‘gossip of ego,’’ we will find relief from the biochemical dopamine/opiate down-regulation, which is, perhaps, the perpetual concomitant of our daily rumination

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b

We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC-2020 March 27 17:00 UTC). We conduct two independent searches: A generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate. © 2022. The Author(s). Published by the American Astronomical Society

Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run

Isolated neutron stars that are asymmetric with respect to their spin axis are possible sources of detectable continuous gravitational waves. This paper presents a fully coherent search for such signals from eighteen pulsars in data from LIGO and Virgo's third observing run (O3). For known pulsars, efficient and sensitive matched-filter searches can be carried out if one assumes the gravitational radiation is phase-locked to the electromagnetic emission. In the search presented here, we relax this assumption and allow both the frequency and the time derivative of the frequency of the gravitational waves to vary in a small range around those inferred from electromagnetic observations. We find no evidence for continuous gravitational waves, and set upper limits on the strain amplitude for each target. These limits are more constraining for seven of the targets than the spin-down limit defined by ascribing all rotational energy loss to gravitational radiation. In an additional search, we look in O3 data for long-duration (hours-months) transient gravitational waves in the aftermath of pulsar glitches for six targets with a total of nine glitches. We report two marginal outliers from this search, but find no clear evidence for such emission either. The resulting duration-dependent strain upper limits do not surpass indirect energy constraints for any of these targets. © 2022. The Author(s). Published by the American Astronomical Society

Open data from the third observing run of LIGO, Virgo, KAGRA, and GEO

The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org. The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages

A joint Fermi-GBM and Swift-BAT analysis of gravitational-wave candidates from the third gravitational-wave observing run

We present Fermi Gamma-ray Burst Monitor (Fermi-GBM) and Swift Burst Alert Telescope (Swift-BAT) searches for gamma-ray/X-ray counterparts to gravitational-wave (GW) candidate events identified during the third observing run of the Advanced LIGO and Advanced Virgo detectors. Using Fermi-GBM onboard triggers and subthreshold gamma-ray burst (GRB) candidates found in the Fermi-GBM ground analyses, the Targeted Search and the Untargeted Search, we investigate whether there are any coincident GRBs associated with the GWs. We also search the Swift-BAT rate data around the GW times to determine whether a GRB counterpart is present. No counterparts are found. Using both the Fermi-GBM Targeted Search and the Swift-BAT search, we calculate flux upper limits and present joint upper limits on the gamma-ray luminosity of each GW. Given these limits, we constrain theoretical models for the emission of gamma rays from binary black hole mergers

Constraints on the cosmic expansion history from GWTC–3

We use 47 gravitational wave sources from the Third LIGO–Virgo–Kamioka Gravitational Wave Detector Gravitational Wave Transient Catalog (GWTC–3) to estimate the Hubble parameter H(z), including its current value, the Hubble constant H0. Each gravitational wave (GW) signal provides the luminosity distance to the source, and we estimate the corresponding redshift using two methods: the redshifted masses and a galaxy catalog. Using the binary black hole (BBH) redshifted masses, we simultaneously infer the source mass distribution and H(z). The source mass distribution displays a peak around 34 M⊙, followed by a drop-off. Assuming this mass scale does not evolve with the redshift results in a H(z) measurement, yielding ${H}_{0}={68}_{-8}^{+12}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ (68% credible interval) when combined with the H0 measurement from GW170817 and its electromagnetic counterpart. This represents an improvement of 17% with respect to the H0 estimate from GWTC–1. The second method associates each GW event with its probable host galaxy in the catalog GLADE+, statistically marginalizing over the redshifts of each event's potential hosts. Assuming a fixed BBH population, we estimate a value of ${H}_{0}={68}_{-6}^{+8}\,\mathrm{km}\ \,\ {{\rm{s}}}^{-1}\,{\mathrm{Mpc}}^{-1}$ with the galaxy catalog method, an improvement of 42% with respect to our GWTC–1 result and 20% with respect to recent H0 studies using GWTC–2 events. However, we show that this result is strongly impacted by assumptions about the BBH source mass distribution; the only event which is not strongly impacted by such assumptions (and is thus informative about H0) is the well-localized event GW190814