The Impact of Medicaid Reimbursement on Rates of Postpartum LARC Uptake [27J]

2020 ◽  
Vol 135 ◽  
pp. 110s
Author(s):  
Amy Addante ◽  
Susannah Koch ◽  
Allison Brubaker ◽  
Duckham Hillary ◽  
Melissa Tepe ◽  
...  
2016 ◽  
Vol 3 (3) ◽  
pp. 175-179
Author(s):  
Bradley C. Gill ◽  
Hans C. Arora ◽  
James C. Ulchaker ◽  
Sandip P. Vasavada

PEDIATRICS ◽  
1991 ◽  
Vol 87 (6) ◽  
pp. 909-920
Author(s):  
Margaret McManus ◽  
Rebecca Kelly ◽  
Samuel Flint

This article examines 1989 Medicaid physician reimbursement for pediatric care in 47 states and the District of Columbia. To assess the adequacy of payment, several state reimbursement policies were analyzed, including physician payment methods, frequency of payment updates, and fee data for five common evaluation and management codes and two Early and Periodic Screening, Diagnosis, and Treatment visit categories. Physician payment rates were evaluated to determine overall state and regional patterns of Medicaid reimbursement. They were also compared with regional private market fee data and average national Medicare fees to assess their adequacy. The majority of state Medicaid programs used fixed fee schedules as their physician reimbursement method. Nearly one fourth of states that update their fees overall by physician specialty have not adjusted their rates since 1985 or before. Medicaid reimbursement rates for five commonly used evaluation and management Physicians' Current Procedural Terminalogy (4th ed) office visit codes and Early and Periodic Screening, Diagnosis, and Treatment screening and follow-up examinations varied substantially across states and among regions. States in the West paid the highest rates for most office visits, while Northeastern states generally paid the least. A comparison of Medicaid payment rates with private market fee data revealed that Medicaid payments for established patients averaged less than two thirds of market rates for pediatricians, family physicians, and general practitioners. New patient care is reimbursed somewhat better. Regional variations are substantial. In addition, a comparison of Medicaid payment rates with 1988 Medicare fee data showed that average Medicaid reimbursement rates were less than four fifths of average allowed Medicare charges. Policy implications include the need to increase Medicaid rates so that they are much closer to private insurance and Medicare rates, particularly in the Northeast and in selected states, in order to increase participation by pediatric providers in Medicaid. In addition, efforts to evaluate reimbursement relative to level of service, as used in Medicare's resource-based relative value scales, deserve further research. Finally, comparable access to comprehensive pediatric care especially in underserved urban areas will require not only improvements in physician reimbursement but also more deliberate efforts to affect the maldistribution of mainstream medical care. Approaches to measure the impact of enhanced reimbursement on access to care by Medicaid-eligible children are discussed.


Medical Care ◽  
1989 ◽  
Vol 27 (1) ◽  
pp. 25-33 ◽  
Author(s):  
Andrew F. Coburn ◽  
Richard H. Fortinsky ◽  
Catherine A. McGuire

1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


1962 ◽  
Vol 14 ◽  
pp. 169-257 ◽  
Author(s):  
J. Green

The term geo-sciences has been used here to include the disciplines geology, geophysics and geochemistry. However, in order to apply geophysics and geochemistry effectively one must begin with a geological model. Therefore, the science of geology should be used as the basis for lunar exploration. From an astronomical point of view, a lunar terrain heavily impacted with meteors appears the more reasonable; although from a geological standpoint, volcanism seems the more probable mechanism. A surface liberally marked with volcanic features has been advocated by such geologists as Bülow, Dana, Suess, von Wolff, Shaler, Spurr, and Kuno. In this paper, both the impact and volcanic hypotheses are considered in the application of the geo-sciences to manned lunar exploration. However, more emphasis is placed on the volcanic, or more correctly the defluidization, hypothesis to account for lunar surface features.


1997 ◽  
Vol 161 ◽  
pp. 197-201 ◽  
Author(s):  
Duncan Steel

AbstractWhilst lithopanspermia depends upon massive impacts occurring at a speed above some limit, the intact delivery of organic chemicals or other volatiles to a planet requires the impact speed to be below some other limit such that a significant fraction of that material escapes destruction. Thus the two opposite ends of the impact speed distributions are the regions of interest in the bioastronomical context, whereas much modelling work on impacts delivers, or makes use of, only the mean speed. Here the probability distributions of impact speeds upon Mars are calculated for (i) the orbital distribution of known asteroids; and (ii) the expected distribution of near-parabolic cometary orbits. It is found that cometary impacts are far more likely to eject rocks from Mars (over 99 percent of the cometary impacts are at speeds above 20 km/sec, but at most 5 percent of the asteroidal impacts); paradoxically, the objects impacting at speeds low enough to make organic/volatile survival possible (the asteroids) are those which are depleted in such species.


1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.


Author(s):  
Lucien F. Trueb

Crushed and statically compressed Madagascar graphite that was explosively shocked at 425 kb by means of a planar flyer-plate is characterized by a black zone extending for 2 to 3 nun below the impact plane of the driver. Beyond this point, the material assumes the normal gray color of graphite. The thickness of the black zone is identical with the distance taken by the relaxation wave to overtake the compression wave.The main mechanical characteristic of the black material is its great hardness; steel scalpels and razor blades are readily blunted during attempts to cut it. An average microhardness value of 95-3 DPHN was obtained with a 10 kg load. This figure is a minimum because the indentations were usually cracked; 14.8 DPHN was measured in the gray zone.


Author(s):  
Sarah A. Luse

In the mid-nineteenth century Virchow revolutionized pathology by introduction of the concept of “cellular pathology”. Today, a century later, this term has increasing significance in health and disease. We now are in the beginning of a new era in pathology, one which might well be termed “organelle pathology” or “subcellular pathology”. The impact of lysosomal diseases on clinical medicine exemplifies this role of pathology of organelles in elucidation of disease today.Another aspect of cell organelles of prime importance is their pathologic alteration by drugs, toxins, hormones and malnutrition. The sensitivity of cell organelles to minute alterations in their environment offers an accurate evaluation of the site of action of drugs in the study of both function and toxicity. Examples of mitochondrial lesions include the effect of DDD on the adrenal cortex, riboflavin deficiency on liver cells, elevated blood ammonia on the neuron and some 8-aminoquinolines on myocardium.


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