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Question

Which of the following statements is/are correct?

1. In June 2016, the LIGO group of scientists announced the detection of a second set of gravitational waves.

2. Gravitational waves were generated due to merger of two black holes at about 1.4 billion light-years distant.

3. Gravitational waves were inserted due to collision of two white dwarf stars at about 14 billion light-years distant.

Select the correct answer using the code given below:

This question was previously asked in
CDS I 2017 General Knowledge Previous Year Paper (05-Feb-2017)
The correct answer is

1 and 2 only

Understanding LIGO and Gravitational Waves

The question asks us to evaluate the correctness of statements related to the detection of gravitational waves by the LIGO (Laser Interferometer Gravitational-Wave Observatory) collaboration.

Gravitational waves are ripples in the fabric of spacetime caused by accelerated masses. Extremely massive and dense objects, like black holes and neutron stars, undergoing violent events like mergers, are strong sources of gravitational waves.

Analyzing Statement 1: Second Gravitational Wave Detection Announcement

Statement 1 says: In June 2016, the LIGO group of scientists announced the detection of a second set of gravitational waves.

Let's examine the facts about LIGO detections around that time:

  • The first direct detection of gravitational waves (event GW150914) was announced by the LIGO/Virgo collaboration in February 2016. This event occurred in September 2015.
  • The second detection of gravitational waves (event GW151226) occurred in December 2015.
  • The scientific paper announcing the detection and analysis of GW151226 was published in June 2016.

Therefore, the announcement/publication of the second detected gravitational wave event did occur in June 2016. This statement is correct.

Analyzing Statement 2: Source and Distance of Gravitational Waves

Statement 2 says: Gravitational waves were generated due to merger of two black holes at about 1.4 billion light-years distant.

LIGO's first two detections, GW150914 and GW151226, were both attributed to the merger of two stellar-mass black holes. The estimated distance to the source of GW150914 was approximately 1.3 billion light-years, and the estimated distance to GW151226 was approximately 1.4 billion light-years.

Since statement 2 mentions a merger of two black holes at about 1.4 billion light-years, which aligns with the characteristics of the second detected event (GW151226), this statement is correct.

Analyzing Statement 3: Alternative Source and Distance

Statement 3 says: Gravitational waves were inserted due to collision of two white dwarf stars at about 14 billion light-years distant.

Let's compare this with what is known about the LIGO detections:

  • The source of the gravitational waves detected by LIGO in its initial runs (including the first two) was the merger of black holes, not the collision or merger of white dwarf stars.
  • While white dwarf mergers are predicted to produce gravitational waves, they typically involve different mass scales and frequencies compared to black hole mergers detectable by ground-based detectors like LIGO. They are expected sources for future space-based detectors like LISA.
  • The distance mentioned, 14 billion light-years, is significantly different from the approximately 1.3-1.4 billion light-years estimated for the first LIGO events. Furthermore, 14 billion light-years is close to the estimated age and size of the observable universe, making a detection at that distance extremely challenging or unlikely for the types of sources LIGO observes with its current sensitivity.

Therefore, statement 3, claiming the source was colliding white dwarfs at 14 billion light-years, is incorrect.

Conclusion on Correct Statements

Based on the analysis:

  • Statement 1 is correct (second detection announced in June 2016).
  • Statement 2 is correct (merger of two black holes at ~1.4 billion light-years).
  • Statement 3 is incorrect (source was black holes, not white dwarfs; distance was ~1.4 billion light-years, not 14 billion).

Thus, the correct statements are 1 and 2 only.

Statement Analysis Correctness
1. Second detection announced in June 2016. The paper announcing the second detection (GW151226, occurred Dec 2015) was published in June 2016. Correct
2. From merger of two black holes at ~1.4 billion light-years. The second detection (GW151226) was from a black hole merger at ~1.4 billion light-years. Correct
3. From collision of two white dwarf stars at ~14 billion light-years. Source was black holes, not white dwarfs. Distance was ~1.4 billion light-years, not 14 billion. Incorrect

Revision Table: Gravitational Wave Detections

Event Date of Event Date of Announcement/Publication Source Approx. Distance
GW150914 (First Detection) Sept 14, 2015 Feb 11, 2016 Binary Black Hole Merger 1.3 billion light-years
GW151226 (Second Detection) Dec 26, 2015 June 15, 2016 Binary Black Hole Merger 1.4 billion light-years

Additional Information on Gravitational Waves and LIGO

What are Gravitational Waves?

Gravitational waves are disturbances in the spacetime curvature, propagating as waves. They carry energy away from their source. They are a prediction of Albert Einstein's General Theory of Relativity.

The LIGO Experiment:

LIGO is a large-scale physics experiment aimed at detecting cosmic gravitational waves. It uses laser interferometry to measure the tiny distortions in spacetime caused by a passing wave. It consists of two detectors in the United States, one in Livingston, Louisiana, and one in Hanford, Washington.

Sources of Gravitational Waves:

The strongest sources of gravitational waves detectable by LIGO include:

  • Merging black holes (like those detected).
  • Merging neutron stars.
  • A black hole merging with a neutron star.
  • Possibly from supernovae (stellar explosions) or even relics from the early universe (though these are harder to detect).

Detection Process:

When a gravitational wave passes through the LIGO detectors, it causes the lengths of the interferometer arms to change slightly. This change affects how the laser light interferes when it is recombined, creating a signal that can be measured.

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