Effects of high-energy astrophysical events on habitable planets

2012 ◽  
Vol 11 (4) ◽  
pp. 279-286 ◽  
Author(s):  
Jorge E. Horvath ◽  
Douglas Galante

AbstractWith the possible exception of meteor impacts, high-energy astrophysical events such as supernovae, gamma-ray bursts (GRB) and flares are usually not taken into account for biological and evolutionary studies due to their low rates of occurrence. We show that a class of these events may occur at distances and time scales in which their biological effects are non-negligible, maybe more frequent than the impacts of large asteroids. We review the effects of four transient astrophysical sources of ionizing radiation on biospheres – stellar flares, giant flares from soft gamma repeaters (SGR), supernovae and GRB. The main damaging features of them are briefly discussed and illustrated. We point out some open problems and ongoing work.

2018 ◽  
Vol 189 (08) ◽  
pp. 785-802 ◽  
Author(s):  
Rafail L. Aptekar ◽  
Andrei M. Bykov ◽  
Sergei V. Golenetskii ◽  
Dmitrii D. Frederiks ◽  
Dmitry S. Svinkin ◽  
...  

2012 ◽  
Vol 754 (2) ◽  
pp. 121 ◽  
Author(s):  
◽  
M. Ackermann ◽  
M. Ajello ◽  
L. Baldini ◽  
G. Barbiellini ◽  
...  

2012 ◽  
Vol 547 ◽  
pp. A95 ◽  
Author(s):  
F. Longo ◽  
E. Moretti ◽  
L. Nava ◽  
R. Desiante ◽  
M. Olivo ◽  
...  

Author(s):  
M. Merck ◽  
D. L. Bertsch ◽  
B. L. Dingus ◽  
C. E. Fichtel ◽  
R. C. Hartman ◽  
...  

1995 ◽  
Vol 231 (1-2) ◽  
pp. 339-341 ◽  
Author(s):  
M. Ostrowski ◽  
A. A. Zdziarski

2011 ◽  
Author(s):  
J. Chiang ◽  
J. L. Racusin ◽  
J. E. McEnery ◽  
J. L. Racusin ◽  
N. Gehrels ◽  
...  

2019 ◽  
Vol 22 ◽  
pp. 88
Author(s):  
K. Balasi ◽  
C. Markou ◽  
K. Tzamarioudaki ◽  
P. Rapidis ◽  
E. Drakopoulou ◽  
...  

The response of an underwater neutrino detector is discussed for investigating its performance to the detection of muons and high energy neutrinos. The afformentioned telescope consists of an autonomous battery operated detector string to a central 4-floor tower. In this aim, we utilised a fast detector simulation program, SIRENE, to simulate the hits from Cherenkov photons at ultra high energies (as high as 1020 eV). In order to optimize the detector, analytical studies for different configurations and characteristics of the photo-multiplier tubes inside the optical modules of the telescope was also examined.


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