To get a feel for some of Einstein's ideas, we must start thinking about the space-time of the Universe. Suppose that I tell you that Astronomy 122 meets in 110 Willamette Hall, Is this enough to get you to class? Well, no, because I didn't tell you when the class meets. In order for you to show up for class, you must know not only where it meets but also when it meets. This is true for all events in the Universe; you must know not only where the event occurs (its spatial position) but also when the event occurs (its temporal position). The space and time positions are equally important and we should think about events in the Universe in terms of their space-time positions. An interesting property of space-time in the Universe is that it has structure and it is not rigid.
Locally, the space-time in this room is fairly flat and so, unless you push on an object, its free motion (unforced motion) is in a straight line. If I were to place a large chunk of mass into the room, the mass would distort the shape of the space-time. In two-dimensions, this is easy to visualize. Imagine a rubber sheet onto which you place a bb. The bb causes a depression to form in the rubber sheet.
Return to the rubber sheet analogy. If I drop a bb on the sheet and it bounces, ripples in the sheet are produced which propagate away from the disturbance. These ripples in the space-time are referred to as gravitational waves.
They almost certainly exist, but there have been no direct measurements of their existence (there is only indirect evidence that they exist).
Possible sources for gravity waves are supernovae, merging neutron stars or black holes ( low amplitude waves, high amplitude waves), unstable rotating neutron stars, ... .