نتایج جستجو برای: 15 to 30 mmin

تعداد نتایج: 10785007  

2013
E. Ben-Naim E. G. Daub P. A. Johnson

We investigate the sequence of great earthquakes over the past century. To examine whether the earthquake record includes temporal clustering, we identify aftershocks and remove those from the record. We focus on the recurrence time, defined as the time between two consecutive earthquakes. We study the variance in the recurrence time and the maximal recurrence time. Using these quantities, we c...

2001
N. SANCHEZ

The quantum string emission by Black Holes is computed in the framework of the ‘string analogue model’ (or thermodynamical approach), which is well suited to combine quantum field theory (QFT) and string theory in curved backgrounds (particulary here, as black holes and strings posses intrinsic thermal features and temperatures). String theory properly describes black-hole evaporation. The blac...

2004
Tjeerd Jellema

The neural basis of social perception and understanding. Tjeerd Jellema, Utrecht University. Social scenes usually contain complex stimulus configurations, derived from the postures and actions of one or more agents. A description of the social scene can be made at two successive levels. At the first level, a literal, mechanistic, description is made in terms of causes and consequences of goal-...

Journal: :International Journal of Advances in Medicine 2019

2008
MARTIN BUCHHEIT

The objective of this study was to gather evidence supporting the accuracy of the 30-15 Intermittent Fitness Test (30-15IFT) for individualizing interval training of young intermittent sport players. In 59 young intermittent sport players (age, 16.26 2.3 years), we observed the relationships between the maximal running speed (MRS) reached at the end of the 30-15IFT (MRS30-15IFT) and physiologic...

2004
D. F. A. Boyd A. P. Whitworth

We present a new analysis of the minimum mass for star formation, based on opacity-limited fragmentation. Our analysis differs from the standard one, which considers hierarchical fragmentation of a 3-D medium, and yields MMIN ∼ 0.007 to 0.010 M⊙ for Population I star formation. Instead we analyse the more realistic situation in which there is one-shot fragmentation of a shock-compressed layer, ...

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