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Gravitational waves are ripples in spacetime caused by accelerating massive objects. They were predicted by Einstein and directly detected in 2015.
Пошаговое руководство
- 1Input source characteristics: mass, acceleration, distance
- 2The calculator estimates gravitational wave strength
- 3Results show strain and energy radiated
Решённые примеры
Ввод
Two 30 solar mass black holes merging, distance = 1.3 billion light-years
Результат
Strain ≈ 10⁻²¹ (first detection)
GW150914 event
Распространённые ошибки
- ✕Overestimating gravitational wave amplitude from typical sources
- ✕Confusing waves with radiation pressure effects
Часто задаваемые вопросы
How are gravitational waves detected?
LIGO uses laser interferometry to measure changes in arm length from gravitational wave strain.
Do gravitational waves carry information?
Yes, they encode details about the source: masses, spins, orbital parameters, and cosmological distance.
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