| Literature DB >> 31311437 |
Xiaoyan Lu1, Jianxi Gao1, Boleslaw K Szymanski1,2.
Abstract
The polarization of political opinions among members of the US legislative chambers measured by their voting records is greater today than it was 30 years ago. Previous research efforts to find causes of such increase have suggested diverse contributors, like growth of online media, echo chamber effects, media biases or disinformation propagation. Yet, we lack theoretic tools to understand, quantify and predict the emergence of high political polarization among voters and their legislators. Here, we analyse millions of roll-call votes cast in the US Congress over the past six decades. Our analysis reveals the critical change of polarization patterns that started at the end of 1980s. In earlier decades, polarization within each Congress tended to decrease with time. By contrast, in recent decades, the polarization has been likely to grow within each term. To shed light on the reasons for this change, we introduce here a formal model for competitive dynamics to quantify the evolution of polarization patterns in the legislative branch of the US government. Our model represents dynamics of polarization, enabling us to successfully predict the direction of polarization changes in 28 out of 30 US Congresses elected in the past six decades. From the evolution of polarization level as measured by the Rice index, our model extracts a hidden parameter-polarization utility which determines the convergence point of the polarization evolution. The increase in the polarization utility implied by the model strongly correlates with two current trends: growing polarization of voters and increasing influence of election campaign donors. Two largest peaks of the model's polarization utility correlate with significant political or legislative changes happening at the same time.Entities:
Keywords: dynamical system; equilibrium; political polarization; stability
Mesh:
Year: 2019 PMID: 31311437 PMCID: PMC6685022 DOI: 10.1098/rsif.2019.0010
Source DB: PubMed Journal: J R Soc Interface ISSN: 1742-5662 Impact factor: 4.118
The statistics of the roll-call votes from the 85th to the 114th US Congress. The bills which received less than 30 votes are not included in the above statistics.
| party | #members | #bills | #votes | #votes/members | #votes/years |
|---|---|---|---|---|---|
| Democratic Party | 1498 | 31 879 | 7 368 921 | 4919.17 | 122815.35 |
| Republican Party | 1395 | 31 879 | 6 275 886 | 4498.84 | 104598.1 |
Figure 1.The illustration of the data collections and processing workflow. (a) For each bill voted in the Congress, we measure the mean absolute distance, dist, between the votes of the Democratic and Republican Parties cast for the bill b; (b) the distribution of the political polarization measured using the roll-call votes within each Congress. Labels at the right corner of each sub-plot identify the first year of each Congress. In the 1980s and 1990s, the polarization levels are generally smaller than the levels in the 2000s and 2010s. After 2001, the two peaks of the voting results at the opposite ends of the political spectrum start to emerge, indicating the growth of the number of bills on which two parties strongly disagree; (c) regardless of the content of bills, we compute the average distance of bill votes between two parties within each Congress in a sliding window of 200 days (equation (2.2)); (d) the political polarization levels at 10 evenly distributed sampled time points exhibit an evolution of polarization patterns from one type of behaviour to another: the polarization level decreases in the 93rd Congress as the time from the replacement of members increases, while polarization remains at a relatively stable level in the 96th Congress, and grows in the Congresses with sessions numbered from 102 to 112. (Online version in colour.)
Figure 2.The convergence of the political polarization model in relation to the polarization utility u and initial state x0. The time t is normalized in the plots to the range from 0 to 1. (a) The total energy of the dynamical system in relation to the polarization x and its first-order derivative for a < 1 (equation (3.3)); (b) the total energy of the dynamical system in relation to the polarization x and its first-order derivative for a > 1 (equation (3.3)); (c) for a < 1 the dynamical system always converges to certain polarization level (a = 0.6); (d) for a > 1 the dynamical system reaches either complete consensus or complete polarization depending on the initial state x0 (a = 2.5). (e) When a < 1, the equilibrium points of the dynamical system are stable and the system gets trapped at these equilibrium points as the time approaches infinity; (f) when a > 1, the initial states (on the top of the hills) are the tipping points causing the system to converge either to 0 (full polarization) or 1 (full consensus) from its initial state x0. (Online version in colour.)
Figure 3.The evolution of the political polarization in the US Congress with subsequent sessions numbered from 85 to 114. (a) Change of polarization within each US Congress based on data and the optimal slope parameters estimated by the Ordinary Least Squares (OLS) linear regression given the 10 evenly distributed in time points of polarization sampling for each Congress. The polarization level is likely to decrease within each Congress after the member replacement in the 1970s and 1980s. However, after the 101th Congress, which started in 1989, the polarization level is likely to increase instead; (b) the estimated values of the polarization utility u are generally increasing, while the periods of sharp growth are often associated with the change of majorities in the Senate and the House of Representatives; (c) when the initial polarization level (dark circles) is smaller than the stable polarization level predicted by our model (solid black curve), we observe an increase of polarization within the corresponding Congress. The direction of such change in 28 out of all 30 Congresses are explained by the model (dark arrows), while the two Congresses in disagreement with prediction have minimal variations of the polarization level (light arrow markers) which indicates weakly formed polarization direction; (d) when the initial polarization level x0 of a Congress is farther away from the corresponding equilibrium point, the absolute change of polarization during the two-year term, i.e. |Δx|, of this Congress is usually higher than of Congresses in which the initial polarization levels are closer to the equilibrium points. The colour of the scatter points indicates the sign of Δx. (Online version in colour.)
The estimated values of the polarization utility u in each Congress. The 14 Congresses with the presidential election held in the preceding year increase u on average by 11.3% compared to the corresponding previous Congresses while the 15 Congresses with midterm elections (during which the President passes half of his term), decrease the polarization utility u by −1.5% on average. Moreover, in the first three decades, the average polarization utility grew slowly by 0.056, so 18.1% on average in Presidential election Congresses. All this growth was gained in four Presidential elections in which the newly elected President and his predecessor belonged to different parties; each of these elections contributed growth of 0.115 so 36.4%, on average. By contrast, the polarization utility decreased by −0.043 or −9.3% in midterm election Congresses, raising only 14.3% over 30 years. In the latest three decades, the polarization utility grew in both types of Congresses with similar average rates, of 0.023 or 4.6% for midterm election Congresses, and 0.21 or 7.3% for Presidential election Congresses. From the 100th Congress to 114th Congress the polarization grew 77.5%, so five times higher than in the earlier period. Notably, 6 of 14 Presidential election Congresses are associated with the polarization utility u > 0.5 while only one of 15 midterm election congresses had such high polarization utility.
| midterm election congresses | presidential election congresses | ||||||
|---|---|---|---|---|---|---|---|
| number | change | percentage (%) | number | change | percentage (%) | ||
| 86th | 0.3 | −0.05 | −14.3 | 0.24 | 80.0 | ||
| 88th | 0.4 | −0.14 | −25.9 | 89th | 0.37 | −0.03 | −7.5 |
| 90th | 0.32 | −0.05 | −13.5 | 91st | 0.43 | 0.11 | 34.4 |
| 92nd | 0.38 | −0.05 | −11.6 | 93rd | 0.31 | −0.07 | −18.4 |
| 94th | 0.33 | 0.02 | 6.5 | 95th | 0.4 | 0.07 | 21.2 |
| 95th | 0.4 | 0.00 | 0.00 | 97th | 0.44 | 0.04 | 10.0 |
| 98th | 0.43 | −0.01 | −2.3 | 99th | 0.46 | 0.03 | 7.0 |
| 100th | 0.4 | −0.06 | −13.0 | 101st | 0.47 | 0.07 | 17.5 |
| 102nd | 0.65 | 0.18 | 38.3 | 103rd* | −0.04 | −6.2 | |
| 104th | 0.54 | −0.07 | −11.5 | 105th* | 0.07 | 13.0 | |
| 106th | 0.5 | −0.11 | −18.0 | 107th* | 0.00 | 0.0 | |
| 108th | 0.52 | 0.02 | 4.0 | 109th* | 0.05 | 9.6 | |
| 110th | 0.48 | −0.09 | −15.8 | 111th | 0.42 | −0.06 | −12.5 |
| 112th* | 0.24 | 57.1 | 113th* | 0.07 | 10.6 | ||
| 114th | 0.71 | −0.02 | −2.74 | ||||
| 86th–100th | 0.370 | −0.043 | −9.3 | 0.421 | 0.056 | 18.1 | |
| 101st–114th | 0.580 | 0.021 | 7.3 | 0.559 | 0.023 | 4.6 | |
| All | 0.468 | −0.013 | −1.5 | 0.481 | 0.039 | 11.3 | |
| 4 positive, 10 negative, 1a | 9 positive, 4 negative, 6a | ||||||
aDenotes the polarization utility u over 0.5, marked by italic font in the u column.