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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    International journal of legal medicine 111 (1998), S. 299-304 
    ISSN: 1437-1596
    Keywords: Key words Postmortem cooling ; Radiation energy loss ; Stefan-Boltzmann law ; Single exponential model ; Skin ; temperature
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine , Law
    Notes: Abstract Conduction and convection are assumed to account for most of the energy loss from the dead body to the (cooler) environment. There are no quantitative estimations in the literature for the contribution of radiation to heat loss. The aim of the present paper was to estimate the radiation energy loss in postmortem cooling. The Stefan-Boltzmann law is used and combined with a single-exponential model for the cooling process of the skin derived from experimental data of Lyle and Cleveland (1956). The influence of various factors (e.g. skin temperature, environmental temperature, body mass and body height) on the amount of radiation emitted was investigated. The radiation energy is quantitatively described as a function of time. The radiation energy loss ranged from approximately 200 kJ in small (165 cm) and lean (50 kg) bodies at room temperature (20 °C) to approximately 600 kJ in tall (185 cm) and over-weight (100 kg) bodies at outdoor temperature (5 °C) in the first hour postmortem.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    International journal of legal medicine 112 (1999), S. 233-240 
    ISSN: 1437-1596
    Keywords: Key words Postmortem cooling ; Radiation ; Conduction ; Convection ; Thermal energy ; Supravital ; activity ; Time since death
    Source: Springer Online Journal Archives 1860-2000
    Topics: Medicine , Law
    Notes: Abstract With the help of the law of Stefan and Boltzmann and a model for the cooling of exposed skin derived from the data of Lyle and Cleveland [7], the radiation energy loss ER can be calculated according to the following formula: where ɛ represents the emissivity of the skin (0.98), σ the Stefan-Boltzmann constant, AR the radiating surface area, TS(0) the skin temperature at death, TE the environmental temperature and Z′ = 0.1017 the gradient of the skin temperature curve. Additionally, an energy loss due to conduction and convection EC has to be taken into account. Comparing the energy losses due to radiation, conduction and convection with the decrease ET of the thermal energy in the body, calculated from mean heat capacity (3.45 kJ/(kg °K)), body mass and decrease of mean body temperature, there is a surplus of energy in the very early postmortem period, which can be explained only by an internal source of energy EI. Alltogether the following balance equation can be formulated: Since the body temperature decreases in the early postmortem period, EI can be estimated by: EI(t) ≥ max (ER(t) – ET(t), 0). The values obtained range up to 500 kJ for a medium sized (175 cm), medium weight (75 kg) body at an environmental temperature of 5 °C and are compatible with estimations of Lundquist [6] for supravital energy production by breakdown of glycogen.
    Type of Medium: Electronic Resource
    Library Location Call Number Volume/Issue/Year Availability
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