When scientists recorded a rippling in space-time, followed within two seconds by an associated burst of light observed by dozens of telescopes around the globe, they had witnessed, for the first time, the explosive collision and merger of two neutron stars.
The intense cosmological event observed on August 17 also had other reverberations here on Earth: It ruled out a class of dark energy theories that modify gravity, and challenged a large class of theories.
Dark energy, which is driving the accelerating expansion of the universe, is one of the biggest mysteries in physics. It makes up about 68 percent of the total mass and energy of the universe and functions as a sort of antigravity, but we don’t yet have a good explanation for it. Simply put, dark energy acts to push matter away from each other, while gravity acts to pull matter together.
The neutron star merger created gravitational waves – a squiggly distortion in the fabric of space and time, like a tossed stone sending ripples across a pond – that traveled about 130 million light-years through space, and arrived at Earth at almost the same instant as the high-energy light that jetted out from this merger.
The gravity waves signature was detected by a network of Earth-based detectors called LIGO and Virgo, and the first intense burst of light was observed by the Fermi Gamma-ray Space Telescope.
That nearly simultaneous arrival time is a very important test for theories about dark energy and gravity.
“Our results make significant progress to elucidate the nature of dark energy,” said Miguel Zumalacárregui, a theoretical physicist who is part of the Berkeley Center for Cosmological Physics at the Department of Energy’s Lawrence Berkeley National Laboratory (Berkeley Lab) and UC Berkeley.
“The simplest theories have survived,” he said. “It’s really about the timing.”
This simulation shows the final stages of the merging of two neutron stars. The merger shown in the simulation is happening much faster in reality, within less than a hundredth of a second, and produces strong gravitational waves. This illustrates one of the possible scenarios for the merger event GW170817, detected by the LIGO-Virgo gravitational-wave network. The result of the merger could have been a neutron star or a black hole, the latter of which is shown here. (Credit: W. Kastaun/T. Kawamura/B. Giacomazzo/R. Ciolfi/A. Endrizzi)
He and Jose María Ezquiaga, who was a visiting Ph.D. researcher in the Berkeley Center for Cosmological Physics, participated in this study, which was published Dec. 18 in the journal Physical Review Letters.
A 100-year-old “cosmological constant” theory introduced by Albert Einstein in relation to his work on general relativity and some other theories derived from this model remain as viable contenders because they propose that dark energy is a constant in both space and time: Gravitational waves and light waves are affected in the same way by dark energy, and thus travel at the same rate through space.
“The favorite explanation is this cosmological constant,” he said. “That’s as simple as it’s going to get.”
There are some complicated and exotic theories that also hold up to the test presented by the star-merger measurements. Massive gravity, for example – a theory of gravity that assigns a mass to a hypothetical elementary particle called a graviton – still holds a sliver of possibility if the graviton has a very slight mass.
Some other theories, though, which held that the arrival of gravitational waves would be separated in time from the arriving light signature of the star merger by far longer periods – stretching up to millions of years – don’t explain what was seen, and must be modified or scrapped.
The study notes that a class of theories known as scalar-tensor theories is particularly challenged by the neutron-star merger observations, including Einstein-Aether, MOND-like (relating to modified Newtonian dynamics), Galileon, and Horndeski theories, to name a few.
With tweaks, some of the challenged models can survive the latest test by the star merger, Zumalacárregui said, though they “lose some of their simplicity” in the process.
Zumalacárregui joined the cosmological center last year and is a Marie Skłodowska-Curie global research fellow who specializes in studies of gravity and dark energy.
He began studying whether gravitational waves could provide a useful test of dark energy following the February 2016 announcement that the two sets of gravitational-wave detectors called LIGO (the Laser Interferometer Gravitational-Wave Observatory) captured the first confirmed measurement of gravitational waves. Scientists believe those waves were created in the merger of two black holes to create a larger black hole.
But those types of events do not produce an associated burst of light. “You need both – not just gravitational waves to help test theories of gravity and dark energy,” Zumalacárregui said.
Another study, which he published with Ezquiaga and others in April 2017, explored the theoretical conditions under which gravity waves could travel at a different velocity than light.
Another implication for this field of research is that, by collecting gravitational waves from these and possibly other cosmological events, it may be possible to use their characteristic signatures as “standard sirens” for measuring the universe’s expansion rate.
This is analogous to how researchers use the similar light signatures for objects – including a type of exploding stars known as Type Ia supernovae and pulsating stars known as cepheids – as “standard candles” to gauge their distance.
Cosmologists use a combination of such measurements to build a so-called distance ladder for gauging how far away a given object is from Earth, but there are some unresolved discrepancies that are likely due to the presence of space dust and imperfections in calculations.
Gathering more data from events that generate both gravitational waves and light could also help resolve different measurements of the Hubble constant – a popular gauge of the universe’s expansion rate.
The Hubble rate calibrated with supernovae distance measurements differs from the Hubble rate obtained from other cosmological observations, Zumalacárregui noted, so finding more standard sirens like neutron-star mergers could possibly improve the distance measurements.
The August neutron star merger event presented an unexpected but very welcome opportunity, he said.
“Gravitational waves are a very independent confirmation or refutation of the distance ladder measurements,” he said. “I’m really excited for the coming years. At least some of these nonstandard dark energy models could explain this Hubble rate discrepancy.
“Maybe we have underestimated some events, or something is unaccounted for that we’ll need to revise the standard cosmology of the universe,” he added. “If this standard holds, we will need radically new theoretical ideas that are difficult to verify experimentally, like multiple universes – the multiverse. However, if this standard fails, we will have more experimental avenues to test those ideas.”
New instruments and sky surveys are coming online that also aim to improve our understanding of dark energy, including the Berkeley Lab-led Dark Energy Spectroscopic Instrument project that is scheduled to begin operating in 2019. And scientists studying other phenomena, such as optical illusions in space caused by gravitational lensing – a gravity-induced effect that causes light from distant objects to bend and distort around closer objects – will also be useful in making more precise measurements.
“It could change the way we think about our universe and our place in it,” Zumalacárregui said. “It’s going to require new ideas.”
The researchers are also affiliated with Nordita, the KTH Royal Institute of Technology, and Stockholm University in Sweden; University of Paris-Saclay in France; and the Autonomous University of Madrid. The work was supported by the Spanish State Research Agency, Autonomous University of Madrid, and the Marie Skłodowska-Curie Global Fellowship Project.
Publication: Jose María Ezquiaga and Miguel Zumalacárregui, “Dark Energy After GW170817: Dead Ends and the Road Ahead,” Physical Review Letters, 2017; doi:10.1103/PhysRevLett.119.251304
Source: Lawrence Berkeley National Laboratory