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Different kinds of loneliness – Having poor quality relationships is associated with greater distress than having too few

According to a new study, there are 4 different types of loneliness.

Loneliness not only feels bad, experts have characterised it as a disease that increases the risk of a range of physical and psychological disorders. Some national prevalence estimates for loneliness are alarming. Although they can be as low as 4.4 per cent (in Azerbaijan), in other countries (such as Denmark) as many as 20 per cent of adults report being either moderately or severely lonely.


However, there's no established way of identifying loneliness. Most diagnostic methods treat it as a one-dimensional construct: though it can vary in degrees, someone is either "lonely", or they're not. A new approach, outlined in a paper published recently in Social Psychiatry and Psychiatric Epidemiology, suggests that loneliness should in fact be divided into three sub-types, two of which are associated with poor mental health.

Philip Hyland at Trinity College Dublin and colleagues studied a nationally representative sample of 1,839 US adults aged between 18 and 70, all of whom had experienced at least one traumatic event in their lifetime. (This allowed the team to also look for associations between childhood or adult trauma and loneliness.) Most were married or living with a partner.

Participants completed a six-item scale that measured feelings of "social loneliness" (focusing on perceptions of the quantity of one's social relationships) and "emotional loneliness" (which focused on perceptions of the quality of one's relationships). They also completed questionnaires assessing levels of childhood and adult trauma, depression and anxiety, and their psychological wellbeing.

Following convention, the 17.1 per cent of participants who scored a certain amount above the average loneliness score for the sample (by more than one standard deviation) were classified as "lonely" – a figure comparable to that found previously in many other countries.

However, the researchers also used a statistical technique to look for qualitative differences between the participants' loneliness responses, and this revealed four distinct classes.

The first class – which they called "low loneliness" – was characterised by low scores on both types of loneliness, social and emotional. Just over half the participants fell into this category. The second class – "social loneliness" – making up 8.2 per cent of the sample, comprised people low on emotional loneliness, but high on social loneliness. The third class – "emotional loneliness" – made up just over a quarter of the total sample and was characterised by the opposite pattern of high emotional loneliness but low levels of social loneliness. People in the fourth and final "social and emotional loneliness" class, accounting for 12.4 per cent of the sample, scored high for both types of loneliness.

The researchers found a clear gradient of psychological distress across the classes. People in the low loneliness class were, predictably, least distressed, followed by people in the "social loneliness" class, then the "emotional loneliness" class, and finally the "social and emotional loneliness" class. In fact, people in both these last two classes had levels of symptoms of depression, anxiety and negative psychological wellbeing that were reflective of a psychiatric disorder.

In other words, quality of relationships appears more important to mental health than the sheer number of them."These results indicate that while the experience of social loneliness is associated with slight diminutions in overall mental health, relative to the low loneliness class, the experience of emotional loneliness has a substantially greater, and more negative impact on overall mental health status," the researchers write. "The combination of social and emotional loneliness is associated with the poorest mental health status," they note.

People who belonged to the emotional loneliness class were more likely to be female, younger than average for the group, not in a relationship and to have suffered an increased number of childhood traumas. (Every childhood traumatic experience increased the odds of belonging to the emotional loneliness class by 28 per cent.) The same associations were true for the "social and emotional" loneliness class – except they were also characterised by a greater number of adult traumas.

At 39.0 per cent, the total percentage of participants who fell into the two loneliness classes characterised by clinically relevant levels of psychological distress was much higher than the 17.1 per cent loneliness figure obtained using the conventional one-dimensional approach. "This finding indicates that by recognising naturally occurring subtypes of loneliness, the number of people experiencing a form… that is likely to be of clinical relevance is more than double the number identified when loneliness is conceptualised as a unidimensional construct," the researchers note.

The work suggests that in assessing loneliness, whether in an individual or at a national level, it's important to recognise there are various subtypes. It also supports findings from some other studies that it's the quality, not quantity, of your relationships that really matters. As the researchers conclude: "From a societal perspective, and in the interests of reducing the burden of psychological distress, efforts should be made to enhance the quality of social connections as opposed to promoting the virtues of larger social networks."

Quality not quantity: loneliness subtypes, psychological trauma, and mental health in the US adult population

Emma Young (@EmmaELYoung) is Staff Writer at BPS Research Digest

--This article was originally published on BPS Research Digest. Read the original article.

The “new normal” paradox: What COVID-19 has revealed about higher education

Higher education faces challenges that are unlike any other industry. What path will ASU, and universities like ASU, take in a post-COVID world?

Photo: Luis Robayo/AFP via Getty Images
Sponsored by Charles Koch Foundation
  • Everywhere you turn, the idea that coronavirus has brought on a "new normal" is present and true. But for higher education, COVID-19 exposes a long list of pernicious old problems more than it presents new problems.
  • It was widely known, yet ignored, that digital instruction must be embraced. When combined with traditional, in-person teaching, it can enhance student learning outcomes at scale.
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Iranian Tolkien scholar finds intriguing parallels between subcontinental geography and famous map of Middle-earth

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Image: Mohammad Reza Kamali, reproduced with kind permission
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  • J.R.R. Tolkien himself hinted that his stories are set in a really ancient version of Europe.
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An eight-metre-long Whale shark swims with other fish at the Okinawa Churaumi Aquarium on February 26, 2010 in Motobu, Okinawa, Japan.

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  • Japanese researchers discovered that the whale shark has "tiny teeth"—dermal denticles—protecting its eyes from abrasion.
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A massive star has mysteriously vanished, confusing astronomers

A gigantic star makes off during an eight-year gap in observations.

Image source: ESO/L. Calçada
Surprising Science
  • The massive star in the Kinsman Dwarf Galaxy seems to have disappeared between 2011 and 2019.
  • It's likely that it erupted, but could it have collapsed into a black hole without a supernova?
  • Maybe it's still there, but much less luminous and/or covered by dust.

A "very massive star" in the Kinman Dwarf galaxy caught the attention of astronomers in the early years of the 2000s: It seemed to be reaching a late-ish chapter in its life story and offered a rare chance to observe the death of a large star in a region low in metallicity. However, by the time scientists had the chance to turn the European Southern Observatory's (ESO) Very Large Telescope (VLT) in Paranal, Chile back around to it in 2019 — it's not a slow-turner, just an in-demand device — it was utterly gone without a trace. But how?

The two leading theories about what happened are that either it's still there, still erupting its way through its death throes, with less luminosity and perhaps obscured by dust, or it just up and collapsed into a black hole without going through a supernova stage. "If true, this would be the first direct detection of such a monster star ending its life in this manner," says Andrew Allan of Trinity College Dublin, Ireland, leader of the observation team whose study is published in Monthly Notices of the Royal Astronomical Society.

So, em...

Between astronomers' last look in 2011 and 2019 is a large enough interval of time for something to happen. Not that 2001 (when it was first observed) or 2019 have much meaning, since we're always watching the past out there and the Kinman Dwarf Galaxy is 75 million light years away. We often think of cosmic events as slow-moving phenomena because so often their follow-on effects are massive and unfold to us over time. But things happen just as fast big as small. The number of things that happened in the first 10 millionth of a trillionth of a trillionth of a trillionth of a second after the Big Bang, for example, is insane.

In any event, the Kinsman Dwarf Galaxy, or PHL 293B, is far way, too far for astronomers to directly observe its stars. Their presence can be inferred from spectroscopic signatures — specifically, PHL 293B between 2001 and 2011 consistently featured strong signatures of hydrogen that indicated the presence of a massive "luminous blue variable" (LBV) star about 2.5 times more brilliant than our Sun. Astronomers suspect that some very large stars may spend their final years as LBVs.

Though LBVs are known to experience radical shifts in spectra and brightness, they reliably leave specific traces that help confirm their ongoing presence. In 2019 the hydrogen signatures, and such traces, were gone. Allan says, "It would be highly unusual for such a massive star to disappear without producing a bright supernova explosion."

The Kinsman Dwarf Galaxy, or PHL 293B, is one of the most metal-poor galaxies known. Explosive, massive, Wolf-Rayet stars are seldom seen in such environments — NASA refers to such stars as those that "live fast, die hard." Red supergiants are also rare to low Z environments. The now-missing star was looked to as a rare opportunity to observe a massive star's late stages in such an environment.

Celestial sleuthing

In August 2019, the team pointed the four eight-meter telescopes of ESO's ESPRESSO array simultaneously toward the LBV's former location: nothing. They also gave the VLT's X-shooter instrument a shot a few months later: also nothing.

Still pursuing the missing star, the scientists acquired access to older data for comparison to what they already felt they knew. "The ESO Science Archive Facility enabled us to find and use data of the same object obtained in 2002 and 2009," says Andrea Mehner, an ESO staff member who worked on the study. "The comparison of the 2002 high-resolution UVES spectra with our observations obtained in 2019 with ESO's newest high-resolution spectrograph ESPRESSO was especially revealing, from both an astronomical and an instrumentation point of view."

Examination of this data suggested that the LBV may have indeed been winding up to a grand final sometime after 2011.

Team member Jose Groh, also of Trinity College, says "We may have detected one of the most massive stars of the local Universe going gently into the night. Our discovery would not have been made without using the powerful ESO 8-meter telescopes, their unique instrumentation, and the prompt access to those capabilities following the recent agreement of Ireland to join ESO."

Combining the 2019 data with contemporaneous Hubble Space Telescope (HST) imagery leaves the authors of the reports with the sense that "the LBV was in an eruptive state at least between 2001 and 2011, which then ended, and may have been followed by a collapse into a massive BH without the production of an SN. This scenario is consistent with the available HST and ground-based photometry."

Or...

A star collapsing into a black hole without a supernova would be a rare event, and that argues against the idea. The paper also notes that we may simply have missed the star's supernova during the eight-year observation gap.

LBVs are known to be highly unstable, so the star dropping to a state of less luminosity or producing a dust cover would be much more in the realm of expected behavior.

Says the paper: "A combination of a slightly reduced luminosity and a thick dusty shell could result in the star being obscured. While the lack of variability between the 2009 and 2019 near-infrared continuum from our X-shooter spectra eliminates the possibility of formation of hot dust (⪆1500 K), mid-infrared observations are necessary to rule out a slowly expanding cooler dust shell."

The authors of the report are pretty confident the star experienced a dramatic eruption after 2011. Beyond that, though:

"Based on our observations and models, we suggest that PHL 293B hosted an LBV with an eruption that ended sometime after 2011. This could have been followed by
(1) a surviving star or
(2) a collapse of the LBV to a BH [black hole] without the production of a bright SN, but possibly with a weak transient."

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