bluuebunny/crossref_metadata_2025_split huggingface dataset:
Inequalities in Farm Sector Labour Force in India
Authors: Chakraborty Sonali 
Published: July 2020

The back bone of the rural economy in India is the farm sector or agricultural sector. It also contributes an overall economic and social development towards the nation. Farm activities include agriculture (crop production), plantation, animal husbandry (milk, meat, egg, etc.), forestry & logging, and fishing. In India, the lion share of the labor force is engaged in the farm sector(Pal and Dutta.Though the female labor force participation is typically low in our country, their share in agriculture is commendable and not decreasing as it has been noticed in all other sectors in the recent past. But whether this participation in true sense is in gain full economic activities is to be looked into. Wage discrimination, stereotyping of works, working hours are some inequalities that females are facing at the workplace. In this analysis, an attempt has been made to see the inequality in malefemale participation in farm sectors. Their wage differentials in rural-urban sectors, in different states, have been computed following NIC(National Industry Classification) and NCO(National Classification of occupation) using unit-level data of NSS(National Sample Survey,68th round 2011-12 and Periodiclabour force survey, 2017-18). From preliminary observations, it is noted that there is an increase of rural females as market-oriented crops producers or animal producers and related workers from 2011-12 to 2017-18. The NIC gives the industry-specific picture, where they mainly engaged in mixed farming, plant propagation, post-harvest activities along with perennial and non-perennial crop production. Reduction in a rural male in all these industries is noted as an opposite criterion. In both the rural and urban sectors, gender inequalities persist in wages in almost all NIC activities. Some exceptions like raising of cattle, supporting activities for crop production, fresh water aquaculture, growing of bush fruits and nuts where average earnings of females are a little bit higher than male workers working as either casual labor or regular waged salaried person.
A Study of the Decorations in the Four Minarets of Sultan Hussein Mirza School in Herat
Authors: Hassas Ghulam Hazrat 
Published: July 2020

Sultan Hussein Mirza School is one of the great and magnificent buildings of the Timurid period of Herat, which is located in the north of the old city of Herat. The school was once a place for scientists and scholars in the region, and historians have written extensively about it. The buildings and paintings of this famous school are collapsing and demolishing day by day. The purpose of writing this article is to examine the decorations in the four minarets of Sultan Hussein Mirza School. This article is conducted by Library and Field Research method. The Library Research is related to the history and process of the school building and its post excavations. In the Field Research section, the author himself has visited the school area and the four remaining minarets of Sultan Hussein’s school and wrote the observations of each minaret separately. The results show that all four minarets in school are decorated. Its decorations include geometric patterns, Arabesque motifs, Kufic inscriptions and Muqarnas.
Ghana Go Digital Agenda: The impact of Zipline Drone Technology on Digital Emergency Health Delivery in Ghana
Authors: Demuyakor John 
Published: July 2020

Ghana has deployed high-speed technology and digital initiatives for the daily management of all the sectors of the country under the theme ‘’Ghana Go Digital Agenda’’ policy initiative. These digital governance initiatives include the electronic or digital-health care systems, e-justice system paperless clearing of goods at port-banking, and other online services. Paramount among the many digital initiatives is the introduction of drones for emergency digital health delivery. Access to medical supplies in Ghana has been hindered by the difficulty of getting the supplies from the central points to other areas that are remotely located to enable the patients who need the services to get them. To overcome this challenge and deliver affordable and accessible health care services to the Ghanaian populace, the Government of Ghana engaged a US-based company Zipline Technology to use Drones in the supply of medical supplies for emergencies and hard-to-reach areas of the country. Since the introduction of this initiative in 2019, it has attracted mix-reactions from various stakeholders on the relevance of the drone technology project on health delivery in Ghana. This study used the Diffusion of Innovation (DOI) and Technology Acceptance Model (TAM) to assess drone technology’s impact on Ghana’s emergency health delivery system. The study utilized an online survey questionnaire to solicit data from participants. From the hundred (100) health facilities, located within the operational zone of the drone, twenty (20) were purposively sampled. Out of 550 questionnaires distributed, a total of 533 health workers (participants) validly responded to the online questionnaire. One key finding of our study indicates that the introduction of drone technology for medical supplies in Ghana has significantly impacted positively on the emergency health delivery system in Ghana.
Desnudando um corpo perturbador: a “bipedia compulsória” e o fetiche pela deficiência na Dança
Authors: Carmo Carlos Eduardo Oliveira do 
Published: July 2020

Este artigo apresenta a “bipedia compulsória”, conceito em desenvolvimento pelo autor, como uma estrutura social, política, econômica e cultural que determina padrões excludentes pautados na normatividade do corpo, subjugando e inferiorizando as potencialidades da pessoa com deficiência, tomadas por incapazes e inaptas. Estabelece diálogos com autores da Teoria Crip, que compreende a deficiência em seus aspectos históricos e culturais, em contraposição ao modelo social. Observa o fenômeno da “bipedia compulsória” pelo viés da Dança, trazendo uma análise dos espetáculos “Striptease-Bicho” e “O Corpo Perturbador”, que abordam o devoteísmo – fetiche pela deficiência – associando-o a determinados comportamentos hierárquicos recorrentes na Dança e nas relações sociais estabelecidas com as pessoas com deficiência. Entende tais relações pautadas pelo pensamento abissal (SANTOS, 2010), que determina diferenciações entre corpos aptos ou não para dançar.
PENGEMBANGAN KOMIK DIGITAL SEBAGAI MEDIA EDUKASI PENANGGULANGAN BENCANA ALAM
Authors: Ratnasari Dine Trio , Ginanjar Ajeng 
Published: July 2020

Penelitian ini bertujuan untuk merancang dan mengembangkan media pembelajaran atau bahan ajar komik digital. Media pembelajaran/ bahan ajar komik digital yaitu model pembelajaran yang merupakan salah satu alternatif yang dapat digunakan dalam pembelajaran Ilmu Pengetahuan Sosial (IPS), selain untuk meningkatkan motivasi dan hasil belajar siswa, mengoptimalkan pembagian kerja dalam kelompok, model ini dikembangkan untuk menghindari terjadinya berpikir abstrak, suatu kesan negatif yang dibiarkan terjadi sejak mereka masih kecil, yang pada akhirnya hingga dewasa kesan negatif tersebut, yang menyatakan bahwa pembelajaran IPS itu membosankan dan membuat siswa menjadi jenuh. Metode yang digunakan dalam penelitian ini adalah R & D (Research and Development). Hasil penelitian adalah bahan ajar e-book dan media pembelajaran komik digital untuk menghindari berpikir abstrak pada pembelajaran IPS sehingga memberikan pengalaman dan kesan negatif siswa terhadap pelajaran IPS. Desain dan implementasi dari penelitian ini diharapkan menjadi salah satu referensi di sekolah-sekolah yang masih minim dalam penggunaan media pembelajaran. Khususnya di kabupaten Lebak-Banten.
Late Morbidity Among Survivors of Childhood Cancers; Experience at Tertiary Care Cancer Hospital
Authors: Shaheen Najma , Jan Mir Rooh , Khan Saghir , Riaz Shazia 
Published: July 2020

Background: Long-term survivors of childhood malignancies are at increased risk of experiencing treatment-related morbidities. Survival into late adulthood in these children provides ample time for the acquisition of long-term sequelae. This study aimed to determine late adverse effects among long-term survivors of childhood cancer from a low-income country perspective. Methods: Data were retrospectively collected from review of charts of patients aged under 18 years at the time of their primary diagnosis between January 1, 1995, to December 31, 2008, and who survived for at least 5 years after completion of their treatment. Analyzed data included demographics, cancer type, treatment modality, types of chemotherapy agents administered and specific late morbidities including frequency of azoospermia, oligospermia, endocrine abnormalities, hearing and pulmonary function impairment, and cardiac dysfunction among the long-term survivors of cancer. Results: The total number of patients was 300 with a mean age of 18 ± 2 years. The male to female ratio was 2.7:1. Median follow up duration was 18 years (range: 5-25 years). Seventy-seven percent of patients were from Punjab, 20% were from Khyber Pakhtunkhwa and 3% were from other provinces. Fifty percent had a diagnosis of Hodgkin Lymphoma, 17% Acute Lymphoblastic Leukemia, 13% Non-Hodgkin Lymphoma, 10% Germ cell tumors and 10% had other tumors. Fifty-seven percent received chemotherapy, 23% chemotherapy and radiotherapy, 15% chemotherapy and surgery, 3% chemotherapy, surgery and radiotherapy and 2% had only surgery. Notable long-term documented sequelae were; azoospermia/oligospermia in 64%, endocrine abnormalities in 25% with hypothyroidism in 13.5% and follicle-stimulating hormone and luteinizing hormone abnormalities in 11.5%, ototoxicity in 6.5%, impaired pulmonary function tests in 4.6%, cardiotoxicity in 2.4% and second malignancies (acute myeloid Leukemia and myelodysplastic syndrome) in 1%. Conclusion: Childhood cancer survivors are at increased risk of adverse treatment-related sequelae and a long-term follow-up plan should be in place in centers where they receive treatment for their primary disease.
Biotremology in arthropods
Authors: Cividini Sofia , Montesanto Giuseppe 
Published: July 2020

AbstractEffective communication is essential in animal life to allow fundamental behavioral processes and survival. Communicating by surface-borne vibrations is likely the most ancient mode of getting and exchanging information in both invertebrates and vertebrates. In this review, we concentrate on the use of vibrational communication in arthropods as a form of intraspecific and interspecific signaling, with a focus on the newest discoveries from our research group in terrestrial isopods (Crustacea: Isopoda: Oniscidea), a taxon never investigated before in this context. After getting little attention in the past, biotremology is now an emerging field of study in animal communication, and it is receiving increased interest from the scientific community dealing with these behavioral processes. In what follows, we illustrate the general principles and mechanisms on which biotremology is based, using definitions, examples, and insights from the literature in arthropods. Vibrational communication in arthropods has mainly been studied in insects and arachnids. For these taxa, much evidence of its use as a source of information from the surrounding environment exists, as well as its involvement in many behavioral roles, such as courtship and mating, conspecific recognition, competition, foraging, parental care, and danger perception. Recently, and for the first time, communication through surface-borne waves has been studied in terrestrial isopods, using a common Mediterranean species of the Armadillidae family as a pilot species,Armadillo officinalisDuméril, 1816. Mainly, for this species, we describe typical behavioral processes, such as turn alternation, aggregation, and stridulation, where vibrational communication appears to be involved.
Sample-size determination for the Bayesian t test and Welch’s test using the approximate adjusted fractional Bayes factor
Authors: Fu Qianrao , Hoijtink Herbert , Moerbeek Mirjam 
Published: July 2020

AbstractWhen two independent means μ1 and μ2 are compared, H0 : μ1 = μ2, H1 : μ1≠μ2, and H2 : μ1 > μ2 are the hypotheses of interest. This paper introduces the package , which can be used to determine the sample size needed to evaluate these hypotheses using the approximate adjusted fractional Bayes factor (AAFBF) implemented in the package . Both the Bayesian t test and the Bayesian Welch’s test are available in this package. The sample size required will be calculated such that the probability that the Bayes factor is larger than a threshold value is at least η if either the null or alternative hypothesis is true. Using the package and/or the tables provided in this paper, psychological researchers can easily determine the required sample size for their experiments.
Existence results for a perturbed Dirichlet problem without sign condition in Orlicz spaces
Authors: Moussa H. , Rhoudaf M. , Sabiki H. 
Published: July 2020

UDC 517.5
We deal with the existence result for nonlinear elliptic equations related to the form

<
b
r
>
A
u
+
g

(
x
,
u
,
∇
u
)

=
f
,
<
b
r
>

where the term

-

ⅆ
i
v

(
a
(
x
,
u
,
∇
u
)
)

is a Leray–Lions operator from a subset of

W
0
1

L
M

(
Ω
)

into its dual. The growth and coercivity conditions on the monotone vector field

a

are prescribed by an

N

-function

M

which does not have to satisfy a

Δ
2

-condition. Therefore we use Orlicz–Sobolev spaces which are not necessarily reflexive and assume that the nonlinearity

g

(
x
,
u
,
∇
u
)

is a Carathéodory function satisfying only a growth condition with no sign condition. The right-hand side~

f

belongs to

W
-1

E

M
¯

(
Ω
)

.
A classification of conformal vector fields on the tangent bundle
Authors: Raei Zohre , Latifi Dariush 
Published: July 2020

UDC 514.7
Let

(
M
,
g
)

be a Riemannian manifold and

T
M

be its tangent bundle equipped with a Riemannian (or pseudo-Riemannian) lift metric derived from

g
.

We give a classification of infinitesimal fibre-preserving conformal transformations on the tangent bundle.
О

σ

-субнормальных подгруппах конечных 3'-групп
Authors: Kamornikov S. F. , Tyutyanov V. N. 
Published: July 2020

УДК 512.542
Для любого разбиения

σ

множества всех простых чисел доказывается, что каждое полное холлово множество типа

σ

конечной 3'-группы

G

редуцируется в некоторую подгруппу

H

группы

G

, то подгруппа

H

является

σ

-субнормальной в

G

.
Bounds for the right spectral radius of quaternionicmatrices
Authors: Ali I. 
Published: July 2020

UDC 517.5
In this paper we present bounds for the sum of the moduli of right eigenvalues of a quaternionic matrix. As a consequence, we obtain bounds for the right spectral radius of a quaternionic matrix. We also present a minimal ball in 4D spaces which contains all the Gersgorin balls of a quaternionic matrix. As an application, we introduce the estimation for the right ˇ eigenvalues of quaternionic matrices in the minimal ball. Finally, we suggest some numerical examples to illustrate of our results.
La transformación del índex en el cine en la era digital: análisis de la cinematografía de las películas The Matrix y The Matrix Reloaded
Authors: Castellanos Cerda Vicente 
Published: July 2020

Regularmente, los debates acerca del estatuto de la imagen cinematográfica y su relación con el mundo representado, siempre han iniciado con un detallado estudio de la fotografía, pues como afirmó en 1945 André Bazin “la fotografía y el cine son invenciones que satisfacen definitivamente y en su esencia misma la obsesión del realismo” (Bazin, 2001,p 26). Un realismo vinculado al registro de la huella luminosa del que resulta el efecto de realidad de la imagen cinematográfica.
Este estudio pretende incorporar al debate de la comprensión del fenómeno cinematográfico un punto de vista semiológico, estético y comunicativo que tiene una triple condición sígnica: sonora, visual y técnica.
The ALMA Spectroscopic Survey in the HUDF: Deep 1.2 mm Continuum Number Counts
Authors: González-López Jorge , Novak Mladen , Decarli Roberto , Walter Fabian , Aravena Manuel , Carilli Chris , Boogaard Leindert , Popping Gergö , Weiss Axel , Assef Roberto J. , Bauer Franz Erik , Bouwens Rychard , Cortes Paulo C. , Cox Pierre , Daddi Emanuele , Cunha Elisabete da , Díaz-Santos Tanio , Ivison Rob , Magnelli Benjamin , Riechers Dominik , Smail Ian , Werf Paul van der , Wagg Jeff 
Published: July 2020

Abstract
We present the results from the 1.2 mm continuum image obtained as part of the Atacama Large Millimeter/submillimeter Array Spectroscopic Survey in the Hubble Ultra Deep Field. The 1.2 mm continuum image has a size of 2.9 (4.2) arcmin2 within a primary beam response of 50% (10%) and an rms value of

. We detect 35 sources at high significance (Fidelity ≥0.5); 32 have well-characterized near-infrared Hubble Space Telescope counterparts. We estimate the 1.2 mm number counts to flux levels of

in two different ways: we first use the detected sources to constrain the number counts and find a significant flattening of the counts below S

ν
∼ 0.1 mJy. In a second approach, we constrain the number counts using a probability of deflection statistics (P(D)) analysis. For this latter approach, we describe new methods to accurately measure the noise in interferometric imaging (employing jackknifing in the cube and in the visibility plane). This independent measurement confirms the flattening of the number counts. Our analysis of the differential number counts shows that we are detecting ∼93% (∼100% if we include the lower fidelity detections) of the total continuum dust emission associated with galaxies in the Hubble Ultra Deep Field. The ancillary data allow us to study the dependence of the 1.2 mm number counts on redshift (z = 0−4), galaxy dust mass (

), stellar mass (

), and star formation rate (

). In an accompanying paper we show that the number counts are crucial to constrain galaxy evolution models and the understanding of star-forming galaxies at high redshift.
Using Stereoscopic Observations of Cometary Plasma Tails to Infer Solar Wind Speed
Authors: Cheng Long , Zhang Quanhao , Wang Yuming , Li Xiaolei , Liu Rui 
Published: July 2020

Abstract
Detection of the solar wind speed near the Sun is significant in understanding the heating and acceleration of the solar wind. Cometary plasma tails have long been used as natural probes for solar wind speed; previous solar wind speed estimates via plasma tails, however, were based on comet images from a single viewpoint, and the projection effect may influence the result. Using stereoscopic observations from the Solar Terrestrial Relations Observatory and the Solar and Heliospheric Observatory, we three-dimensionally reconstruct the plasma tails of three comets C/2012 S1 (ISON), C/2010 E6, and C/2011 W3 (Lovejoy) and infer the ambient solar wind speed. The first comet is located between 3.5 and 6 solar radii (Rs) away from the Sun at high latitudes; the estimated solar wind speed is about 300–500 km s−1. The second comet is located within 10 Rs and about 20° away from the ecliptic; the estimated solar wind speed is about 200–320 km s−1. The third comet is also located at low latitudes but farther (>20 Rs) away from the Sun; the estimated solar wind speed is about 100–600 km s−1. For comets near the ecliptic, our results are close to those predicted by MHD models, whereas for the comet at high latitudes, the deviation between our estimate and the model results is notable. This consistency and difference could be used to constrain and improve solar wind models. We will seek opportunities to apply the method to comet 322P, whose tail may sweep the Parker Solar Probe.
Dynamical Evolution of Cosmic Supermassive Binary Black Holes and Their Gravitational-wave Radiation
Authors: Chen Yunfeng , Yu Qingjuan , Lu Youjun 
Published: July 2020

Abstract
We investigate the evolution of supermassive binary black holes (BBHs) in galaxies with realistic property distributions and the gravitational-wave (GW) radiation from the cosmic population of these BBHs. We incorporate a comprehensive treatment of the dynamical interactions of the BBHs with their environments by including the effects of galaxy triaxial shapes and inner stellar distributions, and generate a large number of BBH evolution tracks. By combining these BBH evolution tracks, galaxy mass functions, galaxy merger rates, and supermassive black hole–host galaxy relations into our model, we obtain statistical distributions of surviving BBHs, BBH coalescence rates, the strength of their GW radiation, and the stochastic GW background (GWB) contributed by the cosmic BBH population. About ∼1%–3% (or

) of supermassive BHs at nearby galactic centers are expected to be binaries with mass ratio

(or

). The characteristic strain amplitude of the GWB at frequency

is estimated to be

, and the upper bound of its results obtained with the different BH–host galaxy relations can be up to

, which await testing by future experiments (e.g., the Square Kilometer Array, FAST, Next-Generation Very Large Array). The turnover frequency of the GWB spectrum is at

. The uncertainties on the above estimates and prospects for detecting individual sources are also discussed. The application of the cosmic BBH population to the Laser Interferometer Space Antenna (LISA) band provides a lower limit to the detection rate of BBHs by LISA,

.
Testing General Relativity with the Stellar-mass Black Hole in LMC X-1 Using the Continuum-fitting Method
Authors: Tripathi Ashutosh , Zhou Menglei , Abdikamalov Askar B. , Ayzenberg Dimitry , Bambi Cosimo , Gou Lijun , Grinberg Victoria , Liu Honghui , Steiner James F. 
Published: July 2020

Abstract
The iron-line and continuum-fitting methods are currently the two leading techniques for measuring black-hole spins with electromagnetic radiation. They can be naturally extended for probing the spacetime geometry around black holes and testing general relativity in the strong field regime. In the past couple of years, there has been significant work to use the iron-line method to test the nature of black holes. Here we use the continuum-fitting method and we show its capability of constraining the spacetime geometry around black holes by analyzing 17 Rossi X-ray Timing Explorer data of the X-ray binary LMC X-1.