Protection against neonatal rotavirus infection by breast milk antibodies and trypsin inhibitors

The role of breast milk antirotavirus immunoglobulin A (IgA) and trypsin inhibitors in limiting the acquisition of rotavirus infection during the initial 5 days of life was evaluated among 42 exclusively breast-fed hospital-born infants, 22 of whom experienced rotavirus infection. The mean concentrations of antirotavirus IgA (ELISA Units) in the breast milk of mothers of the 22 rotavirus-infected neonates was 130.4 +/- 46.4; the corresponding value in 20 noninfected neonates was 384.3 +/- 328.3 (P less than 0.001). Similarly, the trypsin inhibitory capacity (mumols/mt/ml) of breast milk in the rotavirus-infected group was significantly lower (0.109 +/- 0.095) than that in the noninfected group (0.376 +/- 0.191; P less than 0.001). The trypsin inhibitory capacity of milk showed an inverse correlation with infant stool tryptic activity (P less than 0.01). Our results indicate that the acquisition of rotavirus infection during the early neonatal period depends on the concentrations of antirotavirus IgA and trypsin inhibitors in human milk and that protection is mediated by high levels of these antiviral factors.

Role of enteric adenoviruses and rotaviruses in mild and severe acute enteritis

The role of enteric-type adenoviruses and rotaviruses in mild and severe acute gastroenteritis was investigated among children younger than 5 years of age seeking treatment at an urban hospital (UH) and at a rural health center (RHC) in India. There were 330 children at the UH and 340 at the RHC; 319 and 315 age matched nondiarrheal children served as controls for the respective groups. Rotavirus was detected in 15.2% of 330 cases and 1.9% of 319 controls at the UH (P less than 0.001) and in 16.5% of 340 cases and 2.9% of 315 controls at the RHC (P less than 0.001). RV excretion was 3- to 5-fold more common in severe compared with mild diarrhea at the UH and at the RHC (P less than 0.001). The detection rate for enteric-type adenoviruses was similar in patients and controls, respectively, at the UH (0.9%; 2.5%) and RHC (3.8%; 2.5%). At the RHC adenovirus types other than 40 and 41 were excreted by 8.8% of the patients and by only 1.0% of the controls (P less than 0.001). It is possible that the diarrheagenic role of adenoviruses may not be restricted to types 40 and 41.

Neonatal rotavirus infection and its relation to cord blood antibodies

Among 274 neonates born at the maternity services of an urban hospital in India, 36.1% of the infants shed rotavirus in feces (as detected by ELISA) by 72 h of life. The excretion rate increased to 70.3% among the 120 infants who stayed for 5 days or more at the hospital. Diarrhoeal symptoms of mild and self-limited nature were observed only in 19.2% of the rotavirus excretors, the remaining being asymptomatic. Among the 98 infants who received supplement feeds, 49% acquired rotavirus infection as against 24.7% of the 150 exclusively breast fed infants (p less than 0.001). Viral RNA in the feces of all rota positive infants showed the same electropherotype, indicating infection from a common source. The mean percentage rotavirus inhibitory activity of cord sera in the infected and non-infected infants was 50.2 +/- 21.7 and 56.6 +/- 19.2 respectively (p greater than 0.05), suggesting that cord blood antibodies do not offer significant protection against neonatal rotavirus infection.

Secular Variations in the Abundances of Heavy Nuclei in Cosmic Rays

The ratios of fluxes of heavy cosmic-ray nuclei [(30 </= Z </= 40)/(20 < Z </= 28), where Z is the atomic number], based on studies of meteorites and lunar samples, show little variation with time, distance in the solar system (1 to 3 astronomical units), or kinetic energy (30 to 2000 megaelectron volts per nucleon). Samples exposed for time intervals of 10(3) to 10(8) years show that the variations in the flux of 30 </= Z </= 40 nuclei relative to that of the iron group nuclei (20 < Z </= 28) have remained within the range of (1.3 +/- 0.6) x 10(-3) during the last billions of years, thus indicating a remarkable similarity in the elemental composition of sources responsible for these nuclei in the cosmic radiation.