From University of Bath (UK) : “Scrambled magnetic fields and Gamma-Ray Bursts- Space scientists solve a decades long puzzle” 

From University of Bath (UK)

16 June 2021

Vittoria D’Alessio
vda26@bath.ac.uk
+44 (0)1225 383135

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Impression of a GRB outflow showing the prompt phase (gamma-ray flash), reverse shock and forward shock.

An international team of scientists, led by astrophysicists from the University of Bath, has measured the magnetic field in a far-off Gamma-Ray Burst, confirming for the first time a decades-long theoretical prediction – that the magnetic field in these blast waves becomes scrambled after the ejected material crashes into, and shocks, the surrounding medium.

Black holes are formed when massive stars (at least 40 times larger than our Sun) die in a catastrophic explosion that powers a blast wave. These extremely energetic events drive out material at velocities close to the speed of light, and power bright, short-lived gamma-ray flashes that can be detected by satellites orbiting the Earth – hence their name, Gamma-Ray Bursts (GRBs).

Magnetic fields may be threaded through the ejected material and, as the spinning black hole forms, these magnetic fields twist into corkscrew shapes that are thought to focus and accelerate the ejected material.

The magnetic fields can’t be seen directly, but their signature is encoded in the light produced by charged particles (electrons) that whiz around the magnetic field lines. Earth-bound telescopes capture this light, which has travelled for millions of years across the Universe.

Head of Astrophysics at Bath and gamma-ray expert Professor Carole Mundell, said: “We measured a special property of the light – polarisation – to directly probe the physical properties of the magnetic field powering the explosion. This is a great result and solves a long-standing puzzle of these extreme cosmic blasts – a puzzle I’ve been studying for a long time.”

Capturing the light early

The challenge is to capture the light as soon as possible after a burst and decode the physics of the blast, the prediction being that any primordial magnetics fields will ultimately be destroyed as the expanding shock front collides with the surrounding stellar debris.

This model predicts light with high levels of polarisation (>10%) soon after the burst when the large-scale primordial field is still intact and driving the outflow. Later, the light should be mostly unpolarised as the field is scrambled in the collision.

Mundell’s team was first to discover highly polarised light minutes after the burst that confirmed the presence of primordial fields with large-scale structure. But the picture for expanding forward shocks has proved more controversial.

Teams who observed GRBs in slower time – hours to a day after a burst – found low polarisation and concluded the fields had long-since been destroyed, but could not say when or how. In contrast, a team of Japanese astronomers announced an intriguing detection of 10% polarised light in a GRB, which they interpreted as a polarised forward shock with long-lasting ordered magnetic fields.

Lead author of the new study, Bath PhD student Nuria Jordana-Mitjans, said: “These rare observations were difficult to compare, as they probed very different timescales and physics. There was no way to reconcile them in the standard model.”

The mystery remained unsolved for over a decade, until the Bath team’s analysis of GRB 141220A.

In the new paper, published today in the MNRAS, Professor Mundell’s team report the discovery of very low polarisation in forward-shock light detected just 90 seconds after the blast of GRB 141220A. The super-speedy observations were made possible by the team’s intelligent software on the fully autonomous robotic Liverpool Telescope and the novel RINGO3 polarimeter – the instrument that logged the GRB’s colour, brightness, polarisation and rate of fade. Putting together this data, the team was able to prove that:

The light originated in the forward shock.
The magnetic field length scales were much smaller than the Japanese team inferred.
The blast was likely powered by the collapse of ordered magnetic fields in the first moments of the formation of a new black hole.
The mysterious detection of polarisation by the Japanese team could be explained by a contribution of polarised light from the primordial magnetic field before it was destroyed in the shock.

See the full article here.

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The University of Bath (UK) is a public research university located in Bath, Somerset, United Kingdom. It received its royal charter in 1966, along with a number of other institutions following the Robbins Report. Like the University of Bristol (UK) and University of the West of England-Bristol (UK), Bath can trace its roots to the Merchant Venturers’ Technical College, established in Bristol as a school in 1595 by the Society of Merchant Venturers. The university’s main campus is located on Claverton Down, a site overlooking the city of Bath, and was purpose-built, constructed from 1964 in the modernist style of the time.

In the 2014 Research Excellence Framework, 32% of Bath’s submitted research activity achieved the highest possible classification of 4*, defined as world-leading in terms of originality, significance and rigour. 87% was graded 4*/3*, defined as world-leading/internationally excellent. The annual income of the institution for 2017–18 was £287.9 million of which £37.0 million was from research grants and contracts, with an expenditure of £283.1 million.

The university is a member of the Association of Commonwealth Universities (UK), the Association of MBAs, the European Quality Improvement System, the European University Association (EU), Universities UK and GW4 (UK).