What is the impact of primary dental avulsion injuries on the permanent dentition?

2021 ◽  
Vol 22 (4) ◽  
pp. 136-137
Author(s):  
Rachel Osborne
2021 ◽  
Vol 31 (1) ◽  
pp. 19-25
Author(s):  
ME Villa-Gualpa ◽  
◽  
MN Jiménez-Romero ◽  

Objective: To determine the prevalence of dentoalveolartrauma in the urban parish of San Sebastián, Cuenca (Ecuador), in the year 2019. Methods: A descriptive study was carried out retrospectively, 316 people from the San Sebastián parish were included. The lifting of the information was made through a survey. The dependent variable was the prevalence of dentoalveolar trauma. The independent variables wereage, sex, dental arch, teeth affected, etiological agent and avulsion. The Chi square statistic was used with α= 0.05 and used the statistical program SPSS V25. Results: 48.4% were men and 51.6% women, between 1 and 92 years. The prevalence of dentoalveolar trauma was 3.2%, with 10 people dentoalveolar trauma, 7 women and 3 men; 7 people ages 18 and 56years; 5 people with an affected tooth; 3 people with dental avulsion due to trauma. The upper dental arch was the most affected and it was found that the impact with the objects was the main cause. Conclusion: The prevalence of dentoalveolar trauma in the population of San Sebastián was low;there was no significant relationship between sex, age and prevalence. The clash with objects and the upper jaw were the most affected


2018 ◽  
Vol 23 (2) ◽  
Author(s):  
Dorota Olczak-Kowalczyk ◽  
Anna Turska-Szybka ◽  
Dariusz Gozdowski ◽  
Urszula Kaczmarek

Introduction. There has been a lack of current epidemiological data regarding the prevalence of developmental defects of enamel in Polish adolescents. Aim. To evaluate the prevalence of developmental defect of enamel in the permanent dentition in the population of adolescents aged 18 years old, including the impact of selected sociodemographic factors. Material and methods. A cross-sectional study conducted in 2017 covered adolescents aged 18 years old attending schools in 16 Polish voivodeships, selected by stratified sampling. Sociodemographic factors such as sex, place of residence, parents’ education level and subjective economic status were collected with a survey. The condition of enamel was assessed with the use of DDE Index modified by Clarkson and Dean’s Indicator by dentists specially trained and calibrated for this study. Prior to its initiation, the study was approved by the Bioethics Committee of the Medical University in Warsaw (Ref. No.: KB/134/217 of 6.06.217). Results. A total of 1611 adolescents were examined (with 52.6% female and 50.5% were residents of rural areas). Developmental defects of enamel were identified in 16.3% of the participants of the study, most frequently in the form of demarcated opacities (10.4%). In 2.7%, they were classified as fluorosis, most frequently questionable. Maxillary central incisors and first premolars were most frequently affected. In 2.5% of the examined adolescents, the defects involved single teeth, whereas in 0.6% the defects were generalised. Defects not classified as fluorosis were more commonly identified in males. There were statistically significant differences in the prevalence between voivodeships, with defects most commonly observed in participants from southern voivodeships. No other sociodemographic factors, however, were identified as significant. Conclusions. The highest prevalence of demarcated opacities suggests the significance of local factors in the aetiology of developmental enamel defects of permanent dentition in Poland. Fluorosis is a rarely encountered entity. The lack of the significance of sociodemographic factors and the regional differences in the prevalence of developmental defects of enamel suggest the need for further research, aimed at identifying geographical risk factors.


2018 ◽  
Vol 34 (3) ◽  
pp. 158-163 ◽  
Author(s):  
Josiane P. Soares ◽  
Jéssica C. Barasuol ◽  
Fernanda M. Torres ◽  
Angela Giacomin ◽  
Bruna M. Gonçalves ◽  
...  

2021 ◽  
pp. 238008442110035
Author(s):  
L. Tanner ◽  
D. Craig ◽  
R. Holmes ◽  
L. Catinella ◽  
P. Moynihan

Introduction: A systematic review of the evidence on the impact of dental caries on malnutrition risk in children was conducted. Objectives: To systematically review published evidence pertaining to the effect of dental caries severity and prevalence on risk of wasting or stunting in children. Methods: Four questions relating to caries of the permanent dentition, primary dentition, early childhood caries (ECC), and severe ECC as a risk factor for undernutrition were set. The target population was children aged 0 to 18 y from any country. Data sources included MEDLINE and Embase. All human epidemiological studies were included. Quality assessment excluded lowest-quality studies. Evidence synthesis by vote counting was depicted using harvest plots. A best available evidence approach was applied to narrative synthesis. The review was conducted in accordance with the Preferred Reporting Items for Systematic Reviews and Meta-Analyses statement. Results: Of the 2,690 studies identified, 447 were screened in duplicate; of these, 117 underwent quality assessment, resulting in 46 included studies, of which 38 were included in vote counting (3 quasi-experimental, 1 cohort, 1 case control, and 33 cross-sectional studies). For the permanent dentition, findings were mixed; the balance of data showed no association between caries prevalence (7/11 studies) or severity (8/17 studies) with wasting. For the primary dentition, the balance of data showed a positive association between caries prevalence (10/15 studies) and severity (12/15 studies) with wasting, as well as between-caries prevalence (4/5 studies) and severity (6/6 studies) with stunting. Considering ECC only did not alter this pattern of findings. Conclusion: The balance of evidence suggests that dental caries in the primary dentition is associated with undernutrition. There is a need for well-designed trials on the impact of caries rehabilitation on growth trajectories of children from low- and middle-income countries and for prospective studies of the impact of caries severity on both stunting and wasting to confirm causality. Knowledge Transfer Statement: The results of this study can be used by policy makers when considering the importance of oral health in addressing the United Nations Sustainable Development Goal to end all forms of malnutrition. The findings suggest that dental caries in the primary dentition may impair children’s healthy weight gain. The findings indicate that higher-quality data are required to confirm a causal relationship and thus inform funding bodies of the need for research, especially in low- and middle-income countries, to substantiate the current knowledge and inform clear and accurate policy statements.


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.


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