गुरुत्वाकर्षण-तरंग हिंदी उपयोग और उदाहरण

"" इसमें संचालित की जाने वाली प्रमुख गतिविधियों में ब्रह्माण्डविज्ञान, संस्थापित एवं प्रमात्रा गुरुत्व, गुरुत्वाकर्षण तरंग खगोल विज्ञान तथा उच्च ऊर्जा भौतिक विज्ञान सम्मिलित है।

वें एक गुरुत्वाकर्षण तरंगों के एक प्रमुख विशेषज्ञ हैै।

इसमें संचालित की जाने वाली प्रमुख गतिविधियों में ब्रह्माण्डविज्ञान, संस्थापित एवं प्रमात्रा गुरुत्व, गुरुत्वाकर्षण तरंग खगोल विज्ञान तथा उच्च ऊर्जा भौतिक विज्ञान सम्मिलित है।

गुरुत्वाकर्षण-तरंग इसके अंग्रेजी अर्थ का उदाहरण

A treatment of the helicity of gravitational waves can be found in Weinberg.

In the classical theory, this means that gravitational waves obey a massive wave equation and hence travel at speeds below the speed of light.

Observations of gravitational waves have constrained the Compton wavelength of the graviton to be λg > , which can be interpreted as a bound on the graviton mass mg g > or mg h_{\mu\nu} propagating on Minkowski space.

Relation to gravitational waves.

The 2016 discovery of gravitational waves and subsequent observations have yielded constraints on the maximum mass of gravitons, if they are massive at all.

However, photons, which have only energy and no mass, are fundamentally different from massive gravitons in this respect, since the Compton wavelength of the graviton is not equal to the gravitational wavelength.

Instead, the lower-bound graviton Compton wavelength is about times greater than the gravitational wavelength for the GW170104 event, which was ~ 1,700"nbsp;km.

LIGO is not intended primarily as a test ruling out scalar theories, but is widely expected to do so as a side benefit once it detects unambiguous gravitational wave signals exhibiting the characteristics expected in general relativity.

80386Ex GEO600 is a gravitational wave detector located near Sarstedt South of Hanover, Germany.

GEO600 is capable of detecting gravitational waves in the frequency range 50 Hz to 1.

5"nbsp;kHz, and is part of a worldwide network of gravitational wave detectors.

This instrument, and its sister interferometric detectors, when operational, are some of the most sensitive gravitational wave detectors ever designed.

In the 1970s, two groups in Europe, one led by Heinz Billing in Germany and one led by Ronald Drever in UK, initiated investigations into laser-interferometric gravitational wave detection.

The construction of this British-German gravitational wave detector started in September 1995.