Review of Zwinger et al.

Adhikari, Surendra

doi:10.5194/gmd-2019-270-rc3

Cited by 37 publications

(74 citation statements)

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“…The study shows that women younger and older than the age range of this study has a bigger risk for having unintended pregnancy than women aging 20-35 years. This is in-line with previous study which stated that the older the women, the higher their chance of having unintended pregnancy [10,11]. Pregnancy in younger age (<20 years old) or older age (>35 years old) has a high risk on maternal and child health [12].…”

Section: Resultssupporting

confidence: 91%

“…This study states that women who are illiterate about KB method have lower risk of having unintended pregnancy rather than literate women. It was not in-line with the previous study which stated the literate women have lower risk of having unintended pregnancy than women who are illiterate about KB method [11]. The lack of knowledge in service providers and acceptors of KB indicates the lack of basic information about all of the KB methods, this misinformation could cause low usage of KB and affect the unintended pregnancy [12].…”

Section: Resultsmentioning

confidence: 53%

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Trends and Determinants of Unintended Pregnancy Occurrence Among Married Women Aged 15–49 Years in Indonesia

Andini¹,

Mutahar²,

Yeni³

2020

Proceedings of the 4th International Symposium on Health Research (ISHR 2019)

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Complications resulting from unsafe abortion are among the major complications which account for nearly 75% of all maternal deaths. Unsafe abortion is risky for women with an unintended pregnancy. Unintended pregnancy is one of the important issues in public health because there is a negative relationship with the health and social impacts for both mother and children. This study aims to determine trends and analyses the determinants of unintended pregnancy in married woman aged 15-49 in Indonesia. The secondary data used in this study are Indonesia Demographic and Health Survey (IDHS) 2002/03, 2007, and 2012 to display the trends and IDHS 2012 to analyze factors associated with unintended pregnancy. This study is a quantitative study using cross sectional design with married woman aged 15-49 years who had pregnancy/birth and currently pregnant at the time of survey as the study population. Data analysis was done with complex sample from univariate, bivariate by using chi square analysis, and multivariate by using multiple logistic regression analysis. The results shows the increase and decrease of unintended pregnancy based on IDHS 2002/03, 2007, and 2012 (17,1%, 20,3%, 14,7%). The result of the study based on IDHS 2012 shows that the variables significant associated to the incidence of unintended pregnancy included the use of planning methods (PR=1,91), knowledge of contraception methods (PR=0,73), age (PR=1,97), parity (PR=3,25), birth spacing (PR=0,76), residents (PR =1,29), age at first marriage (PR=1,33), knowledge of ovulation cycle (PR=1,31), woman participation in household decision making (PR=1,52). Parity is the most dominantly influencing variable with unintended pregnancy incidence after other variables control (PR=2,33). Contraception program for fertile couples is important to reduce the unintended pregnancy issue by focusing on the effectivity of KB or birth control method, ideal pregnancy planning, and related mother-infant health program so that the welfare of the family can be maintained and improved, decreasing the fertility rate, unsafe abortion and maternal mortality.

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Section: Resultssupporting

confidence: 91%

Section: Resultsmentioning

confidence: 53%

Trends and Determinants of Unintended Pregnancy Occurrence Among Married Women Aged 15–49 Years in Indonesia

Andini¹,

Mutahar²,

Yeni³

2020

Proceedings of the 4th International Symposium on Health Research (ISHR 2019)

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“…As is well-known, the DAMA/Libra experiment [20] observes a yearly modulation in scattering events with a peak date in June [21]. This signal is also compatible with the initial modulation analysis of the COSINE-100 experiment [22], though the results have nearly equal preference for the null (i.e., no dark matter signal) hypothesis. Assuming the SHM or a smooth halo profile derived from simulation, it is difficult to interpret the DAMA/Libra signal as dark matter, given the negative results from other experiments, for both spin-independent (SI) and spin-dependent (SD) interactions [23][24][25][26][27][28].…”

Section: Introductionsupporting

confidence: 83%

Direct detection anomalies in light of GAIA data

2019

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Measurements from the Gaia satellite have greatly increased our knowledge of the dark matter velocity distributions in the Solar neighborhood. There is evidence for multiple cold structures nearby, including a high-velocity stream counterrotating relative to the Sun. This stream could significantly alter the spectrum of recoil energies and increase the annual modulation of dark matter in direct detection experiments such as DAMA/Libra. We reanalyze the experimental limits from Xenon1T, CDMSlite, PICO-60 and COSINE-100, and compare them to the results of the DAMA/Libra experiment. While we find that this new component of the dark matter velocity distribution can greatly improve the fit to the DAMA/Libra data, both spin-independent and spindependent interpretations of the DAMA/Libra signal with elastic and inelastic scattering continue to be ruled out by the null results of other experiments, in particular Xenon1T.

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“…After the submission of the present paper COSINE-100 has released its first annual modulation analysis, consistent at 68.3% C.L. with both a null hypothesis and DAMA/LIBRA's 2-6 keVee best-fit value [65].…”

Section: Acknowledgmentsmentioning

confidence: 73%

Probing DAMA/LIBRA data in the full parameter space of WIMP effective models of inelastic scattering

2019

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We discuss the compatibility of the combined annual modulation effect measured by DAMA/LIBRA-phase1 and DAMA/LIBRA-phase2 with an explanation in terms of inelastic scattering events induced by the most general Galilean-invariant effective contact interaction of a Weakly Interacting Massive Particle (WIMP) dark matter particle of spin 0, 1/2 or 1. We take into account all the possible interferences among operators by studying the intersections among the ellipsoidal surfaces of constant signal of DAMA and other experiments in the space of the coupling constants of the effective theory. In our analysis we assume a standard Maxwellian velocity distribution in the Galaxy. We find that, compared to the elastic case, inelastic scattering partially relieves but does not eliminate the existing tension between the DAMA effect and the constraints from the null results of other experiments. Such tension is very large in all the parameter space with the exception of a small region for WIMP mass m χ ≃ 10 GeV and mass splitting δ > ∼ 20 keV, where it is partially, but not completely relieved. In such region the bounds from fluorine targets are evaded in a kinematic way because the minimal WIMP incoming speed required to trigger upscatters off fluorine exceeds the maximal WIMP velocity in the Galaxy, or is very close to it. As a consequence, we also find that the residual tension between DAMA and other results is considerably more sensitive on the astrophysical parameters compared to the elastic case. We find that the configurations with the smallest tension can produce enough yearly modulation in some of the DAMA bins in compliance with the constraints from other experiments, but the ensuing shape of the modulation spectrum is too steep compared to the measured one. For such configurations the recent COSINE-100 bound is evaded in a natural way due to their large expected modulation fractions.

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Review of Zwinger et al.

Cited by 37 publications

References 0 publications

Trends and Determinants of Unintended Pregnancy Occurrence Among Married Women Aged 15–49 Years in Indonesia

Trends and Determinants of Unintended Pregnancy Occurrence Among Married Women Aged 15–49 Years in Indonesia

Direct detection anomalies in light of GAIA data

Probing DAMA/LIBRA data in the full parameter space of WIMP effective models of inelastic scattering

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