BEIJING -- A group of Chinese researchers has reported the discovery of a new pulsar, which exhibits an exceptionally high spin-down rate, two orders of magnitude higher than that of other known millisecond pulsars, according to a recent research article published in the journal Nature Astronomy.

In terms of traditional theory, millisecond pulsars are formed via ordinary pulsars in binary systems that "accrete" matter from their companion stars, much like a spinning top being continuously whipped. This process leads to accretion-driven acceleration.

However, such acceleration is not without limits. Once millisecond pulsars reach the "spin-up line," their rotation periods gradually stabilize, achieving a precision that even surpasses that of atomic clocks.

All previously observed millisecond pulsars are indeed below the "spin-up line," in perfect match with theoretical predictions, said Wang Na, a professor at the Xinjiang Astronomical Observatory (XAO) of the Chinese Academy of Sciences.

This newly discovered millisecond pulsar resides in a binary system with an orbital period of approximately eight days, and of which the companion star is a white dwarf with a mass greater than 0.29 times that of the sun. Its spin period is 3.2 milliseconds, yet exhibiting an extremely high period derivative, placing it far above the "spin-up line."

This suggests that it is an exceptionally young millisecond pulsar with unusually intense energy loss.

All these features stand in contrast to the traditional perception of millisecond pulsars as being old, magnetically weak and rotationally stable.

This study, conducted by researchers from the XAO, Xinjiang University and Tsinghua University, imposes stringent constraints on the classical theories of accretion-driven spin-up in millisecond pulsars.